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1. Performance of novel VUV-sensitive Silicon Photo-Multipliers for nEXO

Author: G. Gallina, Y. Guan, F. Retiere, G. Cao, A. Bolotnikov, I. Kotov, S. Rescia, A. K. Soma, T. Tsang, L. Darroch, T. Brunner, J. Bolster, J. R. Cohen, T. Pinto Franco, W. C. Gillis, H. Peltz Smalley, S. Thibado, A. Pocar, A. Bhat, A. Jamil, D. C. Moore, G. Adhikari, S. Al Kharusi, E. Angelico, I. J. Arnquist, P. Arsenault, I. Badhrees, J. Bane, V. Belov, E. P. Bernard, T. Bhatta, P. A. Breur, J. P. Brodsky, E. Brown, E. Caden, L. Cao, C. Chambers, B. Chana, S. A. Charlebois, D. Chernyak, M. Chiu, B. Cleveland, R. Collister, M. Cvitan, J. Dalmasson, T. Daniels, K. Deslandes, R. DeVoe, M. L. di Vacri, Y. Ding, M. J. Dolinski, A. Dragone, J. Echevers, B. Eckert, M. Elbeltagi, L. Fabris, W. Fairbank, J. Farine, Y. S. Fu, D. Gallacher, P. Gautam, G. Giacomini, C. Gingras, D. Goeldi, R. Gornea, G. Gratta, C. A. Hardy, S. Hedges, M. Heffner, E. Hein, J. Holt, E. W. Hoppe, J. Hößl, A. House, W. Hunt, A. Iverson, X. S. Jiang, A. Karelin, L. J. Kaufman, R. Krücken, A. Kuchenkov, K. S. Kumar, A. Larson, K. G. Leach, B. G. Lenardo, D. S. Leonard, G. Lessard, G. Li, S. Li, Z. Li, C. Licciardi, R. Lindsay, R. MacLellan, M. Mahtab, S. Majidi, C. Malbrunot, P. Margetak, P. Martel-Dion, L. Martin, J. Masbou, N. Massacret, K. McMichael, B. Mong, K. Murray, J. Nattress, C. R. Natzke, X. E. Ngwadla, J. C. Nzobadila Ondze, A. Odian, J. L. Orrell, G. S. Ortega, C. T. Overman, S. Parent, A. Perna, A. Piepke, N. Pletskova, J. F. Pratte, V. Radeka, E. Raguzin, G. J. Ramonnye, T. Rao, H. Rasiwala, K. Raymond, B. M. Rebeiro, G. Richardson, J. Ringuette, V. Riot, T. Rossignol, P. C. Rowson, L. Rudolph, R. Saldanha, S. Sangiorgio, X. Shang, F. Spadoni, V. Stekhanov, X. L. Sun, A. Tidball, T. Totev, S. Triambak, R. H. M. Tsang, O. A. Tyuka, F. Vachon, M. Vidal, S. Viel, G. Visser, M. Wagenpfeil, M. Walent, K. Wamba, Q. Wang, W. Wang, Y. Wang, M. Watts, W. Wei, L. J. Wen, U. Wichoski, S. Wilde, M. Worcester, W. H. Wu, X. Wu, L. Xie, W. Yan, H. Yang, L. Yang, O. Zeldovich, J. Zhao, and T. Ziegler
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract Liquid xenon time projection chambers are promising detectors to search for neutrinoless double beta decay (0 $$\nu \beta \beta $$ ν β β ), due to their response uniformity, monolithic sensitive volume, scalability to large target masses, and suitability for extremely low background operations. The nEXO collaboration has designed a tonne-scale time projection chamber that aims to search for 0 $$\nu \beta \beta $$ ν β β of $$^{136}$$ 136 Xe with projected half-life sensitivity of $$1.35\times 10^{28}$$ 1.35 × 10 28 yr. To reach this sensitivity, the design goal for nEXO is $$\le $$ ≤ 1% energy resolution at the decay Q-value ( $$2458.07\pm 0.31$$ 2458.07 ± 0.31 keV). Reaching this resolution requires the efficient collection of both the ionization and scintillation produced in the detector. The nEXO design employs Silicon Photo-Multipliers (SiPMs) to detect the vacuum ultra-violet, 175 nm scintillation light of liquid xenon. This paper reports on the characterization of the newest vacuum ultra-violet sensitive Fondazione Bruno Kessler VUVHD3 SiPMs specifically designed for nEXO, as well as new measurements on new test samples of previously characterised Hamamatsu VUV4 Multi Pixel Photon Counters (MPPCs). Various SiPM and MPPC parameters, such as dark noise, gain, direct crosstalk, correlated avalanches and photon detection efficiency were measured as a function of the applied over voltage and wavelength at liquid xenon temperature (163 K). The results from this study are used to provide updated estimates of the achievable energy resolution at the decay Q-value for the nEXO design.
Published: 2022
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2. Generative Adversarial Networks for Scintillation Signal Simulation in EXO-200.

Author: S. Li, I. Ostrovskiy, Z. Li, L. Yang, S. Al Kharusi, G. Anton, I. Badhrees, P. S. Barbeau, D. Beck, V. Belov, T. Bhatta, M. Breidenbach, T. Brunner, G. F. Cao, W. R. Cen, C. Chambers, B. Cleveland, M. Coon, A. Craycraft, T. Daniels, L. Darroch, S. J. Daugherty, J. Davis, S. Delaquis, A. Der Mesrobian-Kabakian, R. DeVoe, J. Dilling, A. Dolgolenko, M. J. Dolinski, J. Echevers, W. Fairbank Jr., D. Fairbank, J. Farine, S. Feyzbakhsh, P. Fierlinger, Y. S. Fu, D. Fudenberg, P. Gautam, R. Gornea, G. Gratta, C. Hall, E. V. Hansen, J. Hoessl, P. Hufschmidt, M. Hughes, A. Iverson, A. Jamil, C. Jessiman, M. J. Jewell, A. Johnson, A. Karelin, L. J. Kaufman, T. Koffas, R. Krücken, A. Kuchenkov, K. S. Kumar, Y. Lan, A. Larson, B. G. Lenardo, D. S. Leonard, G. S. Li, C. Licciardi, Y. H. Lin, R. MacLellan, T. McElroy, T. Michel, B. Mong, D. C. Moore, K. Murray, O. Njoya, O. Nusair, A. Odian, A. Perna, A. Piepke, A. Pocar, F. Retière, A. L. Robinson, P. C. Rowson, J. Runge, S. Schmidt, D. Sinclair, K. Skarpaas, A. K. Soma, V. Stekhanov, M. Tarka, S. Thibado, J. Todd, T. Tolba, T. I. Totev, and R. Tsang
Published: 2023
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3. Velocity independent constraints on spin-dependent DM-nucleon interactions from IceCube and PICO

Author: M. G. Aartsen, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, C. Alispach, K. Andeen, T. Anderson, I. Ansseau, G. Anton, C. Argüelles, J. Auffenberg, S. Axani, P. Backes, H. Bagherpour, X. Bai, A. Balagopal V., A. Barbano, S. W. Barwick, B. Bastian, V. Baum, S. Baur, R. Bay, J. J. Beatty, K.-H. Becker, J. Becker Tjus, S. BenZvi, D. Berley, E. Bernardini, D. Z. Besson, G. Binder, D. Bindig, E. Blaufuss, S. Blot, C. Bohm, M. Börner, S. Böser, O. Botner, J. Böttcher, E. Bourbeau, J. Bourbeau, F. Bradascio, J. Braun, S. Bron, J. Brostean-Kaiser, A. Burgman, J. Buscher, R. S. Busse, T. Carver, C. Chen, E. Cheung, D. Chirkin, S. Choi, L. Classen, A. Coleman, G. H. Collin, J. M. Conrad, P. Coppin, P. Correa, D. F. Cowen, R. Cross, P. Dave, C. De Clercq, J. J. DeLaunay, H. Dembinski, K. Deoskar, S. De Ridder, P. Desiati, K. D. de Vries, G. de Wasseige, M. de With, T. DeYoung, A. Diaz, J. C. Díaz-Vélez, H. Dujmovic, M. Dunkman, E. Dvorak, B. Eberhardt, T. Ehrhardt, P. Eller, R. Engel, P. A. Evenson, S. Fahey, A. R. Fazely, J. Felde, K. Filimonov, C. Finley, A. Franckowiak, E. Friedman, A. Fritz, T. K. Gaisser, J. Gallagher, E. Ganster, S. Garrappa, L. Gerhardt, K. Ghorbani, T. Glauch, T. Glüsenkamp, A. Goldschmidt, J. G. Gonzalez, D. Grant, Z. Griffith, S. Griswold, M. Günder, M. Gündüz, C. Haack, A. Hallgren, L. Halve, F. Halzen, K. Hanson, A. Haungs, D. Hebecker, D. Heereman, P. Heix, K. Helbing, R. Hellauer, F. Henningsen, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, T. Hoinka, B. Hokanson-Fasig, K. Hoshina, F. Huang, M. Huber, T. Huber, K. Hultqvist, M. Hünnefeld, R. Hussain, S. In, N. Iovine, A. Ishihara, G. S. Japaridze, M. Jeong, K. Jero, B. J. P. Jones, F. Jonske, R. Joppe, D. Kang, W. Kang, A. Kappes, D. Kappesser, T. Karg, M. Karl, A. Karle, U. Katz, M. Kauer, J. L. Kelley, A. Kheirandish, J. Kim, T. Kintscher, J. Kiryluk, T. Kittler, S. R. Klein, R. Koirala, H. Kolanoski, L. Köpke, C. Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, K. Krings, G. Krückl, N. Kulacz, N. Kurahashi, A. Kyriacou, M. Labare, J. L. Lanfranchi, M. J. Larson, F. Lauber, J. P. Lazar, K. Leonard, A. Leszczynska, M. Leuermann, Q. R. Liu, E. Lohfink, C. J. Lozano Mariscal, L. Lu, F. Lucarelli, J. Lünemann, W. Luszczak, Y. Lyu, W. Y. Ma, J. Madsen, G. Maggi, K. B. M. Mahn, Y. Makino, P. Mallik, K. Mallot, S. Mancina, I. C. Mariş, R. Maruyama, K. Mase, R. Maunu, F. McNally, K. Meagher, M. Medici, A. Medina, M. Meier, S. Meighen-Berger, T. Menne, G. Merino, T. Meures, J. Micallef, G. Momenté, T. Montaruli, R. W. Moore, R. Morse, M. Moulai, P. Muth, R. Nagai, U. Naumann, G. Neer, H. Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke Pollmann, M. Oehler, A. Olivas, A. O’Murchadha, E. O’Sullivan, T. Palczewski, H. Pandya, D. V. Pankova, N. Park, P. Peiffer, C. Pérez de los Heros, S. Philippen, D. Pieloth, E. Pinat, A. Pizzuto, M. Plum, A. Porcelli, P. B. Price, G. T. Przybylski, C. Raab, A. Raissi, M. Rameez, L. Rauch, K. Rawlins, I. C. Rea, R. Reimann, B. Relethford, M. Renschler, G. Renzi, E. Resconi, W. Rhode, M. Richman, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, I. Safa, S. E. Sanchez Herrera, A. Sandrock, J. Sandroos, M. Santander, S. Sarkar, K. Satalecka, M. Schaufel, H. Schieler, P. Schlunder, T. Schmidt, A. Schneider, J. Schneider, F. G. Schröder, L. Schumacher, S. Sclafani, D. Seckel, S. Seunarine, S. Shefali, M. Silva, R. Snihur, J. Soedingrekso, D. Soldin, M. Song, G. M. Spiczak, C. Spiering, J. Stachurska, M. Stamatikos, T. Stanev, R. Stein, P. Steinmüller, J. Stettner, A. Steuer, T. Stezelberger, R. G. Stokstad, A. Stössl, N. L. Strotjohann, T. Stürwald, T. Stuttard, G. W. Sullivan, I. Taboada, F. Tenholt, S. Ter-Antonyan, A. Terliuk, S. Tilav, L. Tomankova, C. Tönnis, S. Toscano, D. Tosi, A. Trettin, M. Tselengidou, C. F. Tung, A. Turcati, R. Turcotte, C. F. Turley, B. Ty, E. Unger, M. A. Unland Elorrieta, M. Usner, J. Vandenbroucke, W. Van Driessche, D. van Eijk, N. van Eijndhoven, S. Vanheule, J. van Santen, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, T. B. Watson, C. Weaver, A. Weindl, M. J. Weiss, J. Weldert, C. Wendt, J. Werthebach, B. J. Whelan, N. Whitehorn, K. Wiebe, C. H. Wiebusch, L. Wille, D. R. Williams, L. Wills, M. Wolf, J. Wood, T. R. Wood, K. Woschnagg, G. Wrede, D. L. Xu, X. W. Xu, Y. Xu, J. P. Yanez, G. Yodh, S. Yoshida, T. Yuan, M. Zöcklein, IceCube Collaboration, C. Amole, M. Ardid, I. J. Arnquist, D. M. Asner, D. Baxter, E. Behnke, M. Bressler, B. Broerman, G. Cao, C. J. Chen, U. Chowdhury, K. Clark, J. I. Collar, P. S. Cooper, M. Crisler, G. Crowder, N. A. Cruz-Venegas, C. E. Dahl, M. Das, S. Fallows, J. Farine, I. Felis, R. Filgas, F. Girard, G. Giroux, J. Hall, C. Hardy, O. Harris, E. W. Hoppe, M. Jin, L. Klopfenstein, C. B. Krauss, M. Laurin, I. Lawson, A. Leblanc, I. Levine, W. H. Lippincott, F. Mamedov, D. Maurya, P. Mitra, C. Moore, T. Nania, R. Neilson, A. J. Noble, P. Oedekerk, A. Ortega, M.-C. Piro, A. Plante, R. Podviyanuk, S. Priya, A. E. Robinson, S. Sahoo, O. Scallon, S. Seth, A. Sonnenschein, N. Starinski, I. Štekl, T. Sullivan, F. Tardif, E. Vázquez-Jáuregui, N. Walkowski, U. Wichoski, Y. Yan, V. Zacek, J. Zhang, and PICO Collaboration
Subjects: Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract: Abstract Adopting the Standard Halo Model (SHM) of an isotropic Maxwellian velocity distribution for dark matter (DM) particles in the Galaxy, the most stringent current constraints on their spin-dependent scattering cross-section with nucleons come from the IceCube neutrino observatory and the PICO-60 $$\hbox {C}_3\hbox {F}_8$$ C 3 F 8 superheated bubble chamber experiments. The former is sensitive to high energy neutrinos from the self-annihilation of DM particles captured in the Sun, while the latter looks for nuclear recoil events from DM scattering off nucleons. Although slower DM particles are more likely to be captured by the Sun, the faster ones are more likely to be detected by PICO. Recent N-body simulations suggest significant deviations from the SHM for the smooth halo component of the DM, while observations hint at a dominant fraction of the local DM being in substructures. We use the method of Ferrer et al. (JCAP 1509: 052, 2015) to exploit the complementarity between the two approaches and derive conservative constraints on DM-nucleon scattering. Our results constrain $$\sigma _{\mathrm{SD}} \lesssim 3 \times 10^{-39} \mathrm {cm}^2$$ σ SD ≲ 3 × 10 - 39 cm 2 ( $$6 \times 10^{-38} \mathrm {cm}^2$$ 6 × 10 - 38 cm 2 ) at $$\gtrsim 90\%$$ ≳ 90 % C.L. for a DM particle of mass 1 TeV annihilating into $$\tau ^+ \tau ^-$$ τ + τ - ( $$b\bar{b}$$ b b ¯ ) with a local density of $$\rho _{\mathrm{DM}} = 0.3~\mathrm {GeV/cm}^3$$ ρ DM = 0.3 GeV / cm 3 . The constraints scale inversely with $$\rho _{\mathrm{DM}}$$ ρ DM and are independent of the DM velocity distribution.
Published: 2020
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4. Search for Majoron-emitting modes of Xe136 double beta decay with the complete EXO-200 dataset

Author: S. Al Kharusi, G. Anton, I. Badhrees, P. S. Barbeau, D. Beck, V. Belov, T. Bhatta, M. Breidenbach, T. Brunner, G. F. Cao, W. R. Cen, C. Chambers, B. Cleveland, M. Coon, A. Craycraft, T. Daniels, L. Darroch, S. J. Daugherty, J. Davis, S. Delaquis, A. Der Mesrobian-Kabakian, R. DeVoe, J. Dilling, A. Dolgolenko, M. J. Dolinski, J. Echevers, W. Fairbank, D. Fairbank, J. Farine, S. Feyzbakhsh, P. Fierlinger, D. Fudenberg, P. Gautam, R. Gornea, G. Gratta, C. Hall, E. V. Hansen, J. Hoessl, P. Hufschmidt, M. Hughes, A. Iverson, A. Jamil, C. Jessiman, M. J. Jewell, A. Johnson, A. Karelin, L. J. Kaufman, T. Koffas, R. Krücken, A. Kuchenkov, K. S. Kumar, Y. Lan, A. Larson, B. G. Lenardo, D. S. Leonard, G. S. Li, S. Li, Z. Li, C. Licciardi, Y. H. Lin, R. MacLellan, T. McElroy, T. Michel, B. Mong, D. C. Moore, K. Murray, O. Njoya, O. Nusair, A. Odian, I. Ostrovskiy, A. Perna, A. Piepke, A. Pocar, F. Retière, A. L. Robinson, P. C. Rowson, D. Ruddell, J. Runge, S. Schmidt, D. Sinclair, K. Skarpaas, A. K. Soma, V. Stekhanov, M. Tarka, S. Thibado, J. Todd, T. Tolba, T. I. Totev, R. Tsang, B. Veenstra, V. Veeraraghavan, P. Vogel, J.-L. Vuilleumier, M. Wagenpfeil, J. Watkins, M. Weber, L. J. Wen, U. Wichoski, G. Wrede, S. X. Wu, Q. Xia, D. R. Yahne, L. Yang, Y.-R. Yen, O. Ya. Zeldovich, and T. Ziegler
Subjects: 010308 nuclear & particles physics, 0103 physical sciences, 010306 general physics, 01 natural sciences
Published: 2021
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5. Imaging individual barium atoms in solid xenon for barium tagging in nEXO

Author: X. S. Jiang, A. Der Mesrobian-Kabakian, T. Tolba, S. Rescia, D. Fairbank, A. Piepke, Y. Y. Ding, O. Zeldovich, D. Kodroff, T. Daniels, J. Echevers, R. DeVoe, M. Hughes, Simon Johnston, R. Saldanha, O. Nusair, R. Krücken, Alexis G. Schubert, R. MacLellan, G. St-Hilaire, C. Chambers, I. J. Arnquist, Lorenzo Fabris, J.-L. Vuilleumier, N. Roy, Yuehe Lin, U. Wichoski, L. Cao, David Moore, B. T. Cleveland, John L. Orrell, S. Kravitz, F. Nolet, Veljko Radeka, Jens Dilling, B. Mong, M. Wagenpfeil, J. Dalmasson, T. Ziegler, J. P. Brodsky, T. Bhatta, P. C. Rowson, A.C. Odian, I. Badhrees, M. Heffner, Z. Li, Gerrit Wrede, D. Fudenberg, S. X. Wu, M. Tarka, F. Vachon, G. Li, Douglas H Beck, L. J. Wen, S. Parent, Samuele Sangiorgio, A. House, David Leonard, W. Cree, L. Darroch, J. Todd, G. Gallina, Y-R Yen, Thomas Koffas, W. M. Fairbank, I. Ostrovskiy, K. S. Kumar, D. A. Harris, X.L. Sun, J. B. Zhao, S. Delaquis, T. Stiegler, A. Kuchenkov, M. J. Dolinski, X. F. Wu, A. Larson, Yunyan Zhou, O. Njoya, E. V. Hansen, Giorgio Gratta, K. Skarpaas, Ethan Brown, A. Iverson, Triveni Rao, M. Weber, Shu Li, A. Karelin, P. Hufschmidt, David A. Sinclair, Wei Wu, R.J. Newby, T. Rossignol, M. J. Jewell, Qun-Yao Wang, Zhijun Ning, Y. Ito, L. J. Kaufman, Wei Wei, Rejean Fontaine, S. J. Daugherty, F. Bourque, Y. Lan, Liang Yang, R. Tsang, A. Jamil, S. Feyzbakhsh, C. Licciardi, W. R. Cen, R. Gornea, Guofu Cao, E. Raguzin, J. Farine, Eric W. Hoppe, Gerard Visser, A. Burenkov, T. Brunner, Arun Kumar Soma, Justin Albert, J. Watkins, V.N. Stekhanov, M. Coon, A. Pocar, Cory T. Overman, T. Tsang, A. Craycraft, Venkatesh Veeraraghavan, F. Retiere, Angelo Dragone, Jochen M. Schneider, Qing Xia, X. Zhang, M. Chiu, J. Hößl, P. S. Barbeau, G. S. Ortega, Jean-Francois Pratte, V. A. Belov, M. Oriunno, Serge A. Charlebois, T. I. Totev, K. Murray, Gisela Anton, T. Walton, J. Daughhetee, A. E. Robinson, K. Odgers, M. Côté, Thilo Michel, and Gabriele Giacomini
Subjects: Physics, Sapphire window, Multidisciplinary, 010308 nuclear & particles physics, Analytical chemistry, chemistry.chemical_element, Barium, 01 natural sciences, Particle identification, Background level, Xenon, chemistry, Double beta decay, 0103 physical sciences, Atom, Neutrino, 010306 general physics
Abstract: Author(s): Chambers, C; Walton, T; Fairbank, D; Craycraft, A; Yahne, DR; Todd, J; Iverson, A; Fairbank, W; Alamare, A; Albert, JB; Anton, G; Arnquist, IJ; Badhrees, I; Barbeau, PS; Beck, D; Belov, V; Bhatta, T; Bourque, F; Brodsky, JP; Brown, E; Brunner, T; Burenkov, A; Cao, GF; Cao, L; Cen, WR; Charlebois, SA; Chiu, M; Cleveland, B; Coon, M; Cree, W; Cote, M; Dalmasson, J; Daniels, T; Darroch, L; Daugherty, SJ; Daughhetee, J; Delaquis, S; Mesrobian-Kabakian, A Der; DeVoe, R; Dilling, J; Ding, YY; Dolinski, MJ; Dragone, A; Echevers, J; Fabris, L; Farine, J; Feyzbakhsh, S; Fontaine, R; Fudenberg, D; Giacomini, G; Gornea, R; Gratta, G; Hansen, EV; Heffner, M; Hoppe, EW; Hosl, J; House, A; Hufschmidt, P; Hughes, M; Ito, Y; Jamil, A; Jessiman, C; Jewell, MJ; Jiang, XS; Karelin, A; Kaufman, LJ; Kodroff, D; Koffas, T; Kravitz, S; Krucken, R; Kuchenkov, A; Kumar, KS; Lan, Y; Larson, A; Leonard, DS; Li, G; Li, S; Li, Z; Licciardi, C; Lin, YH; Lv, P; MacLellan, R; Michel, T; Mong, B; Moore, DC | Abstract: The search for neutrinoless double beta decay probes the fundamental properties of neutrinos, including whether or not the neutrino and antineutrino are distinct. Double beta detectors are large and expensive, so background reduction is essential for extracting the highest sensitivity. The identification, or 'tagging', of the $^{136}$Ba daughter atom from double beta decay of $^{136}$Xe provides a technique for eliminating backgrounds in the nEXO neutrinoless double beta decay experiment. The tagging scheme studied in this work utilizes a cryogenic probe to trap the barium atom in solid xenon, where the barium atom is tagged via fluorescence imaging in the solid xenon matrix. Here we demonstrate imaging and counting of individual atoms of barium in solid xenon by scanning a focused laser across a solid xenon matrix deposited on a sapphire window. When the laser sits on an individual atom, the fluorescence persists for $\sim$30~s before dropping abruptly to the background level, a clear confirmation of one-atom imaging. No barium fluorescence persists following evaporation of a barium deposit to a limit of $\leq$0.16\%. This is the first time that single atoms have been imaged in solid noble element. It establishes the basic principle of a barium tagging technique for nEXO.
Published: 2019
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6. The EXO-200 detector, part II: Auxiliary Systems

Author: N. Ackerman, J. Albert, M. Auger, D.J. Auty, I. Badhrees, P.S. Barbeau, L. Bartoszek, E. Baussan, V. Belov, C. Benitez-Medina, T. Bhatta, M. Breidenbach, T. Brunner, G.F. Cao, W.R. Cen, C. Chambers, B. Cleveland, R. Conley, S. Cook, M. Coon, W. Craddock, A. Craycraft, W. Cree, T. Daniels, L. Darroch, S.J. Daugherty, J. Daughhetee, C.G. Davis, J. Davis, S. Delaquis, A. Der Mesrobian-Kabakian, R. deVoe, T. Didberidze, J. Dilling, A. Dobi, A.G. Dolgolenko, M.J. Dolinski, M. Dunford, J. Echevers, L. Espic, W. Fairbank, D. Fairbank, J. Farine, W. Feldmeier, S. Feyzbakhsh, P. Fierlinger, K. Fouts, D. Franco, D. Freytag, D. Fudenberg, P. Gautam, G. Giroux, R. Gornea, K. Graham, G. Gratta, C. Hagemann, C. Hall, K. Hall, G. Haller, E.V. Hansen, C. Hargrove, R. Herbst, S. Herrin, J. Hodgson, M. Hughes, A. Iverson, A. Jamil, C. Jessiman, M.J. Jewell, A. Johnson, T.N. Johnson, S. Johnston, A. Karelin, L.J. Kaufman, R. Killick, T. Koffas, S. Kravitz, R. Krücken, A. Kuchenkov, K.S. Kumar, Y. Lan, A. Larson, D.S. Leonard, F. Leonard, F. LePort, G.S. Li, S. Li, Z. Li, C. Licciardi, Y.H. Lin, D. Mackay, R. MacLellan, M. Marino, J.-M. Martin, Y. Martin, T. McElroy, K. McFarlane, T. Michel, B. Mong, D.C. Moore, K. Murray, R. Neilson, R. Nelson, O. Njoya, O. Nusair, K. O'Sullivan, A. Odian, I. Ostrovskiy, C. Ouellet, A. Piepke, A. Pocar, C.Y. Prescott, K. Pushkin, F. Retiere, A. Rivas, A.L. Robinson, E. Rollin, P.C. Rowson, M.P. Rozo, J. Runge, J.J. Russell, S. Schmidt, A. Schubert, D. Sinclair, K. Skarpaas, S. Slutsky, E. Smith, A.K. Soma, V. Stekhanov, V. Strickland, M. Swift, M. Tarka, J. Todd, T. Tolba, D. Tosi, T.I. Totev, R. Tsang, K. Twelker, B. Veenstra, V. Veeraraghavan, J.-L. Vuilleumier, J.-M. Vuilleumier, M. Wagenpfeil, A. Waite, J. Walton, T. Walton, K. Wamba, J. Watkins, M. Weber, L.J. Wen, U. Wichoski, M. Wittgen, J. Wodin, J. Wood, G. Wrede, S.X. Wu, Q. Xia, L. Yang, Y.-R. Yen, O.Ya. Zeldovich, and T. Ziegler
Subjects: High Energy Physics - Experiment (hep-ex), Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, High Energy Physics::Experiment, Instrumentation and Detectors (physics.ins-det), Nuclear Experiment (nucl-ex), Instrumentation, Nuclear Experiment, Mathematical Physics, High Energy Physics - Experiment
Abstract: The EXO-200 experiment searched for neutrinoless double-beta decay of $^{136}$Xe with a single-phase liquid xenon detector. It used an active mass of 110 kg of 80.6%-enriched liquid xenon in an ultra-low background time projection chamber with ionization and scintillation detection and readout. This paper describes the design and performance of the various support systems necessary for detector operation, including cryogenics, xenon handling, and controls. Novel features of the system were driven by the need to protect the thin-walled detector chamber containing the liquid xenon, to achieve high chemical purity of the Xe, and to maintain thermal uniformity across the detector., Manuscript updated in response to JINST reviewer comments
Published: 2021

7. Reflectivity of VUV-sensitive Silicon Photomultipliers in Liquid Xenon

Author: M. Heffner, Thilo Michel, M. Hughes, F. Vachon, Jean-Francois Pratte, Aleksey E. Bolotnikov, A. Craycraft, R. DeVoe, C. Gingras, C.R. Natzke, A. De St. Croix, T. I. Totev, K. Murray, Gisela Anton, J. C. Nzobadila Ondze, S. Al Kharusi, R. Saldanha, O. Nusair, J. Ringuette, R. Krücken, W. M. Fairbank, M. Worcester, A. Der Mesrobian-Kabakian, N. Massacret, Lorenzo Fabris, David Moore, Wen-Qi Yan, K. Harouaka, R. Gornea, E. Hansen, C. T. Overman, Samuele Sangiorgio, I. Ostrovskiy, H. Rasiwala, M. Tarka, K. S. Kumar, M. Elbeltagi, R. Tsang, A. Larson, John L. Orrell, T. Daniels, E. Caden, F. Retière, Z. Li, Mike Richman, N. Roy, S. Feyzbakhsh, G. Giacomini, M. Murra, G. Li, E. Raguzin, A. Pocar, A. Iverson, Ethan Brown, B. Mong, C. Licciardi, F. Nolet, J. P. Brodsky, A. Tidball, T. McElroy, Shu Li, T. Rossignol, V. A. Belov, R. MacLellan, O. Zeldovich, M. Medina Peregrina, A. Karelin, B. T. Cleveland, K. Odgers, I. Badhrees, Venkatesh Veeraraghavan, D. Fairbank, A. Kuchenkov, M. Wagenpfeil, M. Walent, Giorgio Gratta, Qing Xia, Sergio Ferrara, C. Vivo-Vilches, D. Schulte, Govinda Adhikari, G. S. Ortega, J. Todd, Arun Kumar Soma, C. Weinheimer, T. Brunner, D. S. Leonard, Serge A. Charlebois, A. Odian, L. Darroch, S. Rescia, C. Huhmann, M. J. Dolinski, M. J. Jewell, R. Lindsay, D. Chernyak, L. Althueser, V.N. Stekhanov, M. L. Di Vacri, T. Ziegler, Y. Lan, S. Parent, L. J. Kaufman, A. Gorham, S. X. Wu, P. A. Breur, J. Bane, A. E. Robinson, Eric W. Hoppe, J. Echevers, D. Goeldi, G.J. Ramonnye, Liang Yang, A. Jamil, S. Thibado, C. Richard, M. Chiu, J. Farine, P. Martel-Dion, Guofu Cao, T. Bhatta, J. Nattress, E. Angelico, B. Chana, Douglas H Beck, T. Stiegler, J. Schneider, K. Deslandes, P. C. Rowson, A. House, A. Fieguth, C.A. Hardy, U. Wichoski, S. Viel, G. Gallina, A. Piepke, I. J. Arnquist, P. Gautam, K. G. Leach, R.J. Newby, S. Triambak, F. Spadoni, and C. Chambers
Subjects: Materials science, Physics - Instrumentation and Detectors, APDS, chemistry.chemical_element, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, 030218 nuclear medicine & medical imaging, law.invention, 03 medical and health sciences, 0302 clinical medicine, Optics, Silicon photomultiplier, Xenon, law, 0103 physical sciences, Wafer, Angular resolution, Instrumentation, Mathematical Physics, 010308 nuclear & particles physics, business.industry, Detector, Instrumentation and Detectors (physics.ins-det), Avalanche photodiode, chemistry, Angle of incidence (optics), business
Abstract: Silicon photomultipliers are regarded as a very promising technology for next-generation, cutting-edge detectors for low-background experiments in particle physics. This work presents systematic reflectivity studies of Silicon Photomultipliers (SiPM) and other samples in liquid xenon at vacuum ultraviolet (VUV) wavelengths. A dedicated setup at the University of M\"unster has been used that allows to acquire angle-resolved reflection measurements of various samples immersed in liquid xenon with 0.45{\deg} angular resolution. Four samples are investigated in this work: one Hamamatsu VUV4 SiPM, one FBK VUV-HD SiPM, one FBK wafer sample and one Large-Area Avalanche Photodiode (LA-APD) from EXO-200. The reflectivity is determined to be 25-36% at an angle of incidence of 20{\deg} for the four samples and increases to up to 65% at 70{\deg} for the LA-APD and the FBK samples. The Hamamatsu VUV4 SiPM shows a decline with increasing angle of incidence. The reflectivity results will be incorporated in upcoming light response simulations of the nEXO detector., Comment: 18 pages, 11 figures
Published: 2021

8. NEXO: Neutrinoless double beta decay search beyond $10^{28}$ year half-life sensitivity

Author: G Adhikari, S Al Kharusi, E Angelico, G Anton, I J Arnquist, I Badhrees, J Bane, V Belov, E P Bernard, T Bhatta, A Bolotnikov, P A Breur, J P Brodsky, E Brown, T Brunner, E Caden, G F Cao, L Cao, C Chambers, B Chana, S A Charlebois, D Chernyak, M Chiu, B Cleveland, R Collister, S A Czyz, J Dalmasson, T Daniels, L Darroch, R DeVoe, M L Di Vacri, J Dilling, Y Y Ding, A Dolgolenko, M J Dolinski, A Dragone, J Echevers, M Elbeltagi, L Fabris, D Fairbank, W Fairbank, J Farine, S Ferrara, S Feyzbakhsh, Y S Fu, G Gallina, P Gautam, G Giacomini, W Gillis, C Gingras, D Goeldi, R Gornea, G Gratta, C A Hardy, K Harouaka, M Heffner, E W Hoppe, A House, A Iverson, A Jamil, M Jewell, X S Jiang, A Karelin, L J Kaufman, I Kotov, R Krücken, A Kuchenkov, K S Kumar, Y Lan, A Larson, K G Leach, B G Lenardo, D S Leonard, G Li, S Li, Z Li, C Licciardi, R Lindsay, R MacLellan, M Mahtab, P Martel-Dion, J Masbou, N Massacret, T McElroy, K McMichael, M Medina Peregrina, T Michel, B Mong, D C Moore, K Murray, J Nattress, C R Natzke, R J Newby, K Ni, F Nolet, O Nusair, J C Nzobadila Ondze, K Odgers, A Odian, J L Orrell, G S Ortega, C T Overman, S Parent, A Perna, A Piepke, A Pocar, J-F Pratte, N Priel, V Radeka, E Raguzin, G J Ramonnye, T Rao, H Rasiwala, S Rescia, F Retière, J Ringuette, V Riot, T Rossignol, P C Rowson, N Roy, R Saldanha, S Sangiorgio, X Shang, A K Soma, F Spadoni, V Stekhanov, X L Sun, M Tarka, S Thibado, A Tidball, J Todd, T Totev, S Triambak, R H M Tsang, T Tsang, F Vachon, V Veeraraghavan, S Viel, C Vivo-Vilches, P Vogel, J-L Vuilleumier, M Wagenpfeil, T Wager, M Walent, K Wamba, Q Wang, W Wei, L J Wen, U Wichoski, S Wilde, M Worcester, S X Wu, W H Wu, X Wu, Q Xia, W Yan, H Yang, L Yang, O Zeldovich, J Zhao, T Ziegler, Laboratoire de physique subatomique et des technologies associées (SUBATECH), Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-IMT Atlantique Bretagne-Pays de la Loire (IMT Atlantique), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT), and nEXO
Subjects: Nuclear and High Energy Physics, background: effect, Physics - Instrumentation and Detectors, FOS: Physical sciences, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], time-projection chambers, 01 natural sciences, neutrinoless double beta decay, Monte Carlo simulations, double-beta decay: (0neutrino), 0103 physical sciences, neutrino: mass, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, detector: design, xenon: liquid, 010308 nuclear & particles physics, neutrinos, Instrumentation and Detectors (physics.ins-det), sensitivity, time projection chamber, 3. Good health, photon: scintillation counter, copper, radioactivity, Xe-136, experimental results
Abstract: The nEXO neutrinoless double beta decay experiment is designed to use a time projection chamber and 5000 kg of isotopically enriched liquid xenon to search for the decay in $^{136}$Xe. Progress in the detector design, paired with higher fidelity in its simulation and an advanced data analysis, based on the one used for the final results of EXO-200, produce a sensitivity prediction that exceeds the half-life of $10^{28}$ years. Specifically, improvements have been made in the understanding of production of scintillation photons and charge as well as of their transport and reconstruction in the detector. The more detailed knowledge of the detector construction has been paired with more assays for trace radioactivity in different materials. In particular, the use of custom electroformed copper is now incorporated in the design, leading to a substantial reduction in backgrounds from the intrinsic radioactivity of detector materials. Furthermore, a number of assumptions from previous sensitivity projections have gained further support from interim work validating the nEXO experiment concept. Together these improvements and updates suggest that the nEXO experiment will reach a half-life sensitivity of $1.35\times 10^{28}$ yr at 90% confidence level in 10 years of data taking, covering the parameter space associated with the inverted neutrino mass ordering, along with a significant portion of the parameter space for the normal ordering scenario, for almost all nuclear matrix elements. The effects of backgrounds deviating from the nominal values used for the projections are also illustrated, concluding that the nEXO design is robust against a number of imperfections of the model., Comment: 26 pages, 19 figures, version accepted by Journal of Phys. G
Published: 2021
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9. Search for hep solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory

Author: C. E. Okada, Ilan Levine, David A. Sinclair, D. Chauhan, J. Wendland, J. F. Wilkerson, B. Beltran, F. B. Descamps, Jocelyn Monroe, M. H. Schwendener, N. Gagnon, M. Jerkins, T. Sonley, F. Zhang, N. S. Oblath, G. D. Orebi Gann, H. Deng, B. Aharmim, J. R. Leslie, L. C. Stonehill, R. W. Ollerhead, J. Law, A. L. Hallin, B. T. Cleveland, B. C. Robertson, E. Blucher, Bei Cai, Ryuta Hazama, G. Doucas, K. Boudjemline, N. Tolich, M. Huang, H. Wan Chan Tseung, S. Habib, S. Majerus, Yuen-Dat Chan, K. Graham, T. Kutter, T. J. Winchester, Alain Bellerive, D. L. Wark, M. L. Miller, J. Heise, S. M. Oser, M. Bergevin, L. L. Kormos, R. D. Martin, Andrew Hime, N. McCauley, P. Jagam, S. R. Elliott, G. T. Ewan, C. Kraus, A. Krüger, Keith Rielage, R. G. H. Robertson, S. D. Reitzner, S. N. Ahmed, M. Kos, J. C. Loach, O. Simard, R. Van Berg, P. L. Drouin, K. Gilje, R. L. Hahn, I. Lawson, R. J. Ford, Monica Dunford, C. J. Virtue, E. W. Beier, A. J. Noble, J. Maneira, A. W. P. Poon, J. Caravaca, F. Fleurot, B. L. Wall, A. E. Anthony, Christopher C. M. Kyba, P. J. Doe, G. Prior, N. West, W. J. Heintzelman, Hal Evans, S. J. M. Peeters, C. Howard, J. Farine, H. M. O'Keeffe, K. T. Lesko, S. D. Biller, R. A. Ott, Bernie G. Nickel, P. J. Harvey, Jochen Klein, K. J. Keeter, E. Guillian, H. B. Mak, Minfang Yeh, G. Tešić, N. A. Jelley, S. McGee, J. Tm. Goon, N. Barros, A. B. McDonald, E. D. Hallman, R. MacLellan, T. Tsui, S. R. Seibert, Min Chen, C. B. Krauss, B. A. VanDevender, P. Skensved, D. Waller, B. Jamieson, R. Bonventre, James R. Wilson, B. J. Land, X. Dai, J. A. Secrest, J. A. Detwiler, G. A. Cox, R. Lange, Benjamin Monreal, A. Mastbaum, H. Fergani, R. L. Helmer, Kai Zuber, A. Wright, M. G. Boulay, A. LaTorre, E. J. Callaghan, K. Labe, and Joseph A. Formaggio
Subjects: Physics, Standard solar model, Sudbury Neutrino Observatory, 010308 nuclear & particles physics, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Supernova, 0103 physical sciences, High Energy Physics::Experiment, Nuclear Experiment (nucl-ex), Neutrino, 010306 general physics, Nuclear Experiment
Abstract: A search has been performed for neutrinos from two sources, the $hep$ reaction in the solar $pp$ fusion chain and the $��_e$ component of the diffuse supernova neutrino background (DSNB), using the full dataset of the Sudbury Neutrino Observatory with a total exposure of 2.47 kton-years after fiducialization. The $hep$ search is performed using both a single-bin counting analysis and a likelihood fit. We find a best-fit flux that is compatible with solar model predictions while remaining consistent with zero flux, and set a one-sided upper limit of $��_{hep} < 30\times10^{3}~\mathrm{cm}^{-2}~\mathrm{s}^{-1}$ [90% credible interval (CI)]. No events are observed in the DSNB search region, and we set an improved upper bound on the $��_e$ component of the DSNB flux of $��^\mathrm{DSNB}_{��_e} < 19~\textrm{cm}^{-2}~\textrm{s}^{-1}$ (90% CI) in the energy range $22.9 < E_��< 36.9$~MeV., 11 pages, 6 figures
Published: 2020

10. Measurement of the Spectral Shape of the β -Decay of Xe137 to the Ground State of Cs137 in EXO-200 and Comparison with Theory

Author: T. Tolba, E. V. Hansen, Qing Xia, A. Jamil, A. Pocar, S. Thibado, V. Veeraraghavan, C. Chambers, R. DeVoe, Petr Vogel, David Leonard, R. MacLellan, Thomas Koffas, D. Fudenberg, W. M. Fairbank, M. Coon, J. Davis, M. J. Jewell, T. Daniels, F. Retiere, V.N. Stekhanov, L. J. Kaufman, J. Farine, Jouni Suhonen, A. Piepke, J. Todd, R. Tsang, M. J. Dolinski, Jens Dilling, O. Nusair, L. Darroch, R. Krücken, U. Wichoski, M. Hughes, I. Badhrees, K. Skarpaas, J. Hoessl, V. Belov, A. Robinson, T. Bhatta, A. S. Johnson, T. Ziegler, S. Feyzbakhsh, W. R. Cen, K. Murray, S. Al Kharusi, O. Ya. Zeldovich, G. S. Li, R. Gornea, Martin Breidenbach, M. Wagenpfeil, Gisela Anton, P. Hufschmidt, David A. Sinclair, P. C. Rowson, S. X. Wu, B. Mong, J. L. Vuilleumier, Arun Kumar Soma, C. Licciardi, A. Der Mesrobian-Kabakian, Yuehe Lin, S. J. Daugherty, A. Odian, L. Yang, David Moore, Y. Lan, S. Delaquis, Z. Li, Guofu Cao, Giorgio Gratta, A. Larson, T. Brunner, C. R. Hall, A. Dolgolenko, Thilo Michel, C. Jessiman, I. Ostrovskiy, P. Nakarmi, A. Craycraft, K. S. Kumar, B. T. Cleveland, A. Kuchenkov, O. Njoya, B. G. Lenardo, J. Watkins, A. Iverson, D. R. Yahne, T. McElroy, A. Karelin, Shu Li, S. Schmidt, L. J. Wen, Marc Weber, D. Fairbank, B. Veenstra, J. Kostensalo, J. Echevers, Peter Fierlinger, T. I. Totev, Gerrit Wrede, M. Tarka, Douglas H Beck, P. S. Barbeau, Y-R Yen, D. Ruddell, J. Runge, and P. Gautam
Subjects: Physics, Spectral shape analysis, General Physics and Astronomy, Nuclear data, Context (language use), Electron, 7. Clean energy, 01 natural sciences, Spectral line, 0103 physical sciences, Neutron source, Atomic physics, 010306 general physics, Ground state, Energy (signal processing)
Abstract: We report on a comparison between the theoretically predicted and experimentally measured spectra of the first-forbidden nonunique β-decay transition ^{137}Xe(7/2^{-})→^{137}Cs(7/2^{+}). The experimental data were acquired by the EXO-200 experiment during a deployment of an AmBe neutron source. The ultralow background environment of EXO-200, together with dedicated source deployment and analysis procedures, allowed for collection of a pure sample of the decays, with an estimated signal to background ratio of more than 99 to 1 in the energy range from 1075 to 4175 keV. In addition to providing a rare and accurate measurement of the first-forbidden nonunique β-decay shape, this work constitutes a novel test of the calculated electron spectral shapes in the context of the reactor antineutrino anomaly and spectral bump.
Published: 2020
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11. Measurement of the Spectral Shape of the β-Decay of ^{137}Xe to the Ground State of ^{137}Cs in EXO-200 and Comparison with Theory

Author: S, Al Kharusi, G, Anton, I, Badhrees, P S, Barbeau, D, Beck, V, Belov, T, Bhatta, M, Breidenbach, T, Brunner, G F, Cao, W R, Cen, C, Chambers, B, Cleveland, M, Coon, A, Craycraft, T, Daniels, L, Darroch, S J, Daugherty, J, Davis, S, Delaquis, A, Der Mesrobian-Kabakian, R, DeVoe, J, Dilling, A, Dolgolenko, M J, Dolinski, J, Echevers, W, Fairbank, D, Fairbank, J, Farine, S, Feyzbakhsh, P, Fierlinger, D, Fudenberg, P, Gautam, R, Gornea, G, Gratta, C, Hall, E V, Hansen, J, Hoessl, P, Hufschmidt, M, Hughes, A, Iverson, A, Jamil, C, Jessiman, M J, Jewell, A, Johnson, A, Karelin, L J, Kaufman, T, Koffas, J, Kostensalo, R, Krücken, A, Kuchenkov, K S, Kumar, Y, Lan, A, Larson, B G, Lenardo, D S, Leonard, G S, Li, S, Li, Z, Li, C, Licciardi, Y H, Lin, R, MacLellan, T, McElroy, T, Michel, B, Mong, D C, Moore, K, Murray, P, Nakarmi, O, Njoya, O, Nusair, A, Odian, I, Ostrovskiy, A, Piepke, A, Pocar, F, Retière, A L, Robinson, P C, Rowson, D, Ruddell, J, Runge, S, Schmidt, D, Sinclair, K, Skarpaas, A K, Soma, V, Stekhanov, J, Suhonen, M, Tarka, S, Thibado, J, Todd, T, Tolba, T I, Totev, R, Tsang, B, Veenstra, V, Veeraraghavan, P, Vogel, J-L, Vuilleumier, M, Wagenpfeil, J, Watkins, M, Weber, L J, Wen, U, Wichoski, G, Wrede, S X, Wu, Q, Xia, D R, Yahne, L, Yang, Y-R, Yen, O Ya, Zeldovich, and T, Ziegler
Abstract: We report on a comparison between the theoretically predicted and experimentally measured spectra of the first-forbidden nonunique β-decay transition ^{137}Xe(7/2^{-})→^{137}Cs(7/2^{+}). The experimental data were acquired by the EXO-200 experiment during a deployment of an AmBe neutron source. The ultralow background environment of EXO-200, together with dedicated source deployment and analysis procedures, allowed for collection of a pure sample of the decays, with an estimated signal to background ratio of more than 99 to 1 in the energy range from 1075 to 4175 keV. In addition to providing a rare and accurate measurement of the first-forbidden nonunique β-decay shape, this work constitutes a novel test of the calculated electron spectral shapes in the context of the reactor antineutrino anomaly and spectral bump.
Published: 2020

12. Final results of the PICASSO dark matter search experiment

Author: X. Dai, C. M. Jackson, P. Mitra, M. Fines-Neuschild, U. Wichoski, I. T. Lawson, A. Kamaha, R. Podviyanuk, C. B. Krauss, S. Seth, F. Debris, L. Lessard, N. Dhungana, J. P. Martin, E. Grace, O. Scallon, I. Stekl, M. Lafrenière, Mala Das, Ilan Levine, N. Starinski, E. Behnke, S. Gagnebin, D. Marlisov, A. Davour, J. Farine, A. J. Noble, Stanislav Pospisil, Pijushpani Bhattacharjee, M. Besnier, M. Laurin, A. Plante, V. Zacek, and G. Giroux
Subjects: Physics, Particle physics, Complete data, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Dark matter, Detector, Bubble nucleation, FOS: Physical sciences, Astronomy and Astrophysics, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), WIMP, 0103 physical sciences, PICASSO, 010306 general physics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The PICASSO dark matter search experiment operated an array of 32 superheated droplet detectors containing 3.0 kg of C$_{4}$F$_{10}$ and collected an exposure of 231.4 kgd at SNOLAB between March 2012 and January 2014. We report on the final results of this experiment which includes for the first time the complete data set and improved analysis techniques including \mbox{acoustic} localization to allow fiducialization and removal of higher activity regions within the detectors. No signal consistent with dark matter was observed. We set limits for spin-dependent interactions on protons of $\sigma_p^{SD}$~=~1.32~$\times$~10$^{-2}$~pb (90\%~C.L.) at a WIMP mass of 20 GeV/c$^{2}$. In the spin-independent sector we exclude cross sections larger than $\sigma_p^{SI}$~=~4.86~$\times$~10$^{-5 }$~pb~(90\% C.L.) in the region around 7 GeV/c$^{2}$. The pioneering efforts of the PICASSO experiment have paved the way forward for a next generation detector incorporating much of this technology and experience into larger mass bubble chambers., Comment: 24 pages, 7 figures
Published: 2017
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13. Event Reconstruction in a Liquid Xenon Time Projection Chamber with an Optically-Open Field Cage

Author: B. Chana, N. Roy, L. Cao, O. Nusair, G. St-Hilaire, Douglas H Beck, R. Krücken, F. Nolet, E. Raguzin, P. A. Breur, T. McElroy, T. Bhatta, L. J. Kaufman, Gerard Visser, D. Goeldi, M. Coon, Eric W. Hoppe, F. Vachon, Z. Li, C. Chambers, Veljko Radeka, Cory T. Overman, L. J. Wen, J. L. Vuilleumier, Samuele Sangiorgio, L. Darroch, P. Gautam, P. Nakarmi, Kaixuan Ni, K. S. Kumar, A. De St. Croix, R. Tsang, Haijun Yang, E. V. Hansen, P. Lv, E. Caden, S. X. Wu, J. Hößl, P. S. Barbeau, Lorenzo Fabris, I. J. Arnquist, R. Gornea, P. C. Rowson, V.N. Stekhanov, X. S. Jiang, C. Licciardi, A. Jamil, A. House, A. Piepke, J. Todd, G. Gallina, S. Thibado, Y. Y. Ding, A. Der Mesrobian-Kabakian, N. Massacret, M. Heffner, R. MacLellan, S. Viel, M. Worcester, Thilo Michel, V. Veeraraghavan, Qing Xia, M. Hughes, G. Li, Sergio Ferrara, S. Al Kharusi, R. DeVoe, A. Pocar, M. Walent, B. G. Lenardo, Arun Kumar Soma, S. Feyzbakhsh, Y. Lan, G. S. Ortega, B. T. Cleveland, K. Deslandes, T. Brunner, A. Kuchenkov, M. Medina-Peregrina, Serge A. Charlebois, F. Retiere, David Moore, M. Chiu, J. P. Brodsky, M. Tarka, F. Edaltafar, T. Wager, K. G. Leach, Wei Wu, R.J. Newby, Qun-Yao Wang, Zhijun Ning, M. Oriunno, Aleksey E. Bolotnikov, K. Murray, Gisela Anton, K. Odgers, B. Mong, M. J. Dolinski, David Leonard, Thomas Koffas, W. M. Fairbank, T. Tsang, T. Stiegler, Jean-Francois Pratte, Angelo Dragone, M. Elbeltagi, John L. Orrell, T. Daniels, Wei Wei, H. Rasiwala, I. Ostrovskiy, Yu-Guang Zhou, S. Rescia, D. Fairbank, Guofu Cao, Mike Richman, O. Njoya, T. I. Totev, A. Iverson, K. Skarpaas Viii, Shu Li, Giorgio Gratta, U. Wichoski, L. Yang, T. Rossignol, M. J. Jewell, A. Craycraft, T. Ziegler, Gabriele Giacomini, J. Echevers, Jens Dilling, C.R. Natzke, I. Badhrees, A. Tidball, M. L. di Vacri, C. Vivo-Vilches, S. Parent, A. Odian, O. Zeldovich, R. Saldanha, M. Wagenpfeil, J. Dalmasson, X.L. Sun, J. B. Zhao, X. F. Wu, A. Larson, Ethan Brown, A. Karelin, J. Farine, V. Belov, and A. Robinson
Subjects: Physics, Nuclear and High Energy Physics, Scintillation, Photon, Time projection chamber, Physics - Instrumentation and Detectors, Field (physics), 010308 nuclear & particles physics, chemistry.chemical_element, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, Xenon, chemistry, Double beta decay, Ionization, 0103 physical sciences, Atomic physics, 010306 general physics, Instrumentation, Event reconstruction
Abstract: nEXO is a proposed tonne-scale neutrinoless double beta decay ($0\nu\beta\beta$) experiment using liquid ${}^{136}Xe$ (LXe) in a Time Projection Chamber (TPC) to read out ionization and scintillation signals. Between the field cage and the LXe vessel, a layer of LXe ("skin" LXe) is present, where no ionization signal is collected. Only scintillation photons are detected, owing to the lack of optical barrier around the field cage. In this work, we show that the light originating in the skin LXe region can be used to improve background discrimination by 5% over previous published estimates. This improvement comes from two elements. First, a fraction of the $\gamma$-ray background is removed by identifying light from interactions with an energy deposition in the skin LXe. Second, background from ${}^{222}Rn$ dissolved in the skin LXe can be efficiently rejected by tagging the $\alpha$ decay in the ${}^{214}Bi-{}^{214}Po$ chain in the skin LXe., Comment: 11 pages, 12 figures
Published: 2020
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14. Measurements of electron transport in liquid and gas Xenon using a laser-driven photocathode

Author: R. Saldanha, I. Ostrovskiy, D. Kodroff, M. J. Dolinski, S. Rescia, John L. Orrell, T. Daniels, P. Gautam, D. Fairbank, Z. Li, E. Caden, E. V. Hansen, Gerard Visser, J. Watkins, Mike Richman, O. Njoya, R. MacLellan, He-Run Yang, A. Iverson, Triveni Rao, K. Skarpaas Viii, Liang Yang, R. Tsang, Gabriele Giacomini, A. Jamil, Pengpeng Lv, O. Nusair, R. Krücken, Shu Li, J. Echevers, Yu-Guang Zhou, Sergio Ferrara, B. Chana, Y. Lan, M. L. di Vacri, U. Wichoski, T. Wager, J. P. Brodsky, C. Vivo-Vilches, I. J. Arnquist, D. Beck, Thilo Michel, Y-R Yen, T. Tsang, T. Tolba, J. Runge, Yuehe Lin, T. Ziegler, Qun-Yao Wang, P. Nakarmi, Guofu Cao, M. Hughes, Jens Dilling, R. Fontaine, David Leonard, M. Heffner, Angelo Dragone, J. L. Vuilleumier, M. Walent, S. Al Kharusi, I. Badhrees, M. Tarka, Thomas Koffas, W. M. Fairbank, B. G. Lenardo, S. Viel, Arun Kumar Soma, T. Brunner, D. Goeldi, L. J. Kaufman, T. Stiegler, Samuele Sangiorgio, Xuan Wu, K. S. Kumar, S. Parent, M. Elbeltagi, M. Coon, K. G. Leach, David Moore, Wei Wei, Qing Xia, J. Farine, G. S. Ortega, Cory T. Overman, Wei Wu, R.J. Newby, P. C. Rowson, S. X. Wu, S. J. Daugherty, Serge A. Charlebois, A. House, G. St-Hilaire, S. Feyzbakhsh, P. S. Barbeau, A. Robinson, T. Bhatta, V. A. Belov, A.C. Odian, O. Zeldovich, Eric W. Hoppe, A. Piepke, J. Todd, L. Darroch, Y. Y. Ding, M. Oriunno, C. Chambers, A. Pocar, V.N. Stekhanov, B. T. Cleveland, T. Rossignol, A. Kuchenkov, M. J. Jewell, Veljko Radeka, X. S. Jiang, C. Licciardi, G. Gallina, A. Der Mesrobian-Kabakian, V. Veeraraghavan, A. Fucarino, Giorgio Gratta, M. Chiu, K. Murray, Gisela Anton, K. Odgers, E. Raguzin, J. Hossl, R. DeVoe, W. R. Cen, M. Medina-Peregrina, R. Gornea, F. Retiere, B. Mong, M. Wagenpfeil, J. Dalmasson, M. Ward, G. S. Li, X.L. Sun, J. B. Zhao, A. Larson, A. Craycraft, Ethan Brown, C.R. Natzke, A. Karelin, Jean-Francois Pratte, Z. Ning, T. I. Totev, A. De St. Croix, Lorenzo Fabris, N. Roy, L. Cao, F. Nolet, T. McElroy, F. Vachon, L. J. Wen, and Marc Weber
Subjects: Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, chemistry.chemical_element, Electron, medicine.disease_cause, 7. Clean energy, 01 natural sciences, Photocathode, Xenon, Electric field, 0103 physical sciences, medicine, Nuclear Experiment (nucl-ex), 010306 general physics, Instrumentation, Nuclear Experiment, Physics, Argon, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), Photoelectric effect, chemistry, Quantum efficiency, High Energy Physics::Experiment, Atomic physics, Ultraviolet
Abstract: Measurements of electron drift properties in liquid and gaseous xenon are reported. The electrons are generated by the photoelectric effect in a semi-transparent gold photocathode driven in transmission mode with a pulsed ultraviolet laser. The charges drift and diffuse in a small chamber at various electric fields and a fixed drift distance of 2.0 cm. At an electric field of 0.5 kV/cm, the measured drift velocities and corresponding temperature coefficients respectively are 1 . 97 ± 0 . 04 m m ∕ μ s and ( − 0 . 69 ± 0 . 05 ) %/K for liquid xenon, and 1 . 42 ± 0 . 03 m m ∕ μ s and ( + 0 . 11 ± 0 . 01 ) %/K for gaseous xenon at 1.5 bar. In addition, we measure longitudinal diffusion coefficients of 25 . 7 ± 4 . 6 cm 2 /s and 149 ± 23 cm 2 /s, for liquid and gas, respectively. The quantum efficiency of the gold photocathode is studied at the photon energy of 4.73 eV in liquid and gaseous xenon, and vacuum. These charge transport properties and the behavior of photocathodes in a xenon environment are important in designing and calibrating future large scale noble liquid detectors.
Published: 2019

15. Data-driven modeling of electron recoil nucleation in PICO C3F8 bubble chambers

Author: Mala Das, T. Nania, E. Behnke, L. Klopfenstein, S. Fallows, D. Tiwari, A. Plante, W. H. Lippincott, C. E. Dahl, A. Hagen, D. M. Asner, S. Sahoo, Jie Zhang, C. Licciardi, C. B. Coutu, B. Loer, M. Ardid, D. Baxter, C. B. Krauss, J. Fuentes, S. Pal, C. M. Jackson, F. Tardif, Ilan Levine, N. A. Cruz-Venegas, J. I. Collar, Satyajit Seth, Shashank Priya, K. Wierman, A. Leblanc, G. Cao, U. Chowdhury, F. Mamedov, T. Sullivan, R. Neilson, M.-C. Piro, N. Walkowski, W. Woodley, P. S. Cooper, R. Filgas, E. Weima, Amber M. Ortega, G. Crowder, O. Harris, C. Amole, T. Kozynets, S. Chen, G. Giroux, E. Vázquez-Jáuregui, P. Mitra, M. Jin, J. M. Wagner, P. Oedekerk, N. Starinski, A. Sonnenschein, B. Broerman, C. Cowles, O. Scallon, B. Hackett, A. E. Robinson, M. B. Crisler, I. J. Arnquist, F. Girard, U. Wichoski, T. Hillier, Yongke Yan, I. Stekl, Chujie Chen, C. Hardy, M. Bressler, C. D. Moore, J. Hall, J. Farine, Karl J. Clark, I. Lawson, A. J. Noble, M. Laurin, V. Zacek, and Eric W. Hoppe
Subjects: Physics, 010308 nuclear & particles physics, Endowment, Atomic energy, European Regional Development Fund, Library science, 7. Clean energy, 01 natural sciences, Mine site, 0103 physical sciences, Christian ministry, 010306 general physics, Engineering research, National laboratory, Underground space
Abstract: The PICO Collaboration wishes to thank SNOLAB and its staff for support through underground space, logistical and technical services. SNOLAB operations are supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site. We wish to acknowledge the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI) for funding. We acknowledge the support from National Science Foundation (NSF) (Grants No. 0919526, No. 1506337, No. 1242637, No. 1205987, and No. 1806722). We acknowledge that this work is supported by the U.S. Department of Energy (DOE) Office of Science, Office of High Energy Physics (under Award No. DE-SC-0012161), by DGAPA-UNAM (PAPIIT No. IA100118) and Consejo Nacional de Ciencia y Tecnologia (CONACyT, M?exico, Grants No. 252167 and No. A1-S-8960), by the Department of Atomic Energy (DAE), Government of India, under the Centre for AstroParticle Physics II project (CAPP-II) at the Saha Institute of Nuclear Physics (SINP), European Regional Development Fund?Project ?Engineering Applications of Microworld Physics? (Project No. CZ.02.1.01/0.0/0.0/ 16_019/0000766), and the Spanish Ministerio de Ciencia, Innovacion y Universidades (Red Consolider MultiDark, Grant No. FPA2017-90566-REDC). This work is partially supported by the Kavli Institute for Cosmological Physics at the University of Chicago through NSF Grant No. 1125897, and an endowment from the Kavli Foundation and its founder Fred Kavli. We also wish to acknowledge the support from Fermi National Accelerator Laboratory under Contract No. DE-AC02-07CH11359, and Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05- 76RL01830. We also thank Compute Canada [75] and the Center for Advanced Computing, ACENET, Calcul Qu?ebec, Compute Ontario, and WestGrid for computational support.
Published: 2019
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16. Dark matter search results from the complete exposure of the PICO-60 C3F8 bubble chamber

Author: W. H. Lippincott, J. Hall, O. Harris, E. Behnke, C. B. Coutu, Chujie Chen, M. Jin, T. Sullivan, U. Chowdhury, F. Girard, Ivan Felis, C. Hardy, O. Scallon, C. M. Jackson, J. Farine, G. Cao, F. Mamedov, R. Filgas, R. Neilson, M. Bressler, A. Leblanc, T. Nania, S. Fallows, P. S. Cooper, N. Starinski, E. Weima, Ilan Levine, N. A. Cruz-Venegas, C. D. Moore, M.-C. Piro, F. Tardif, E. Vázquez-Jáuregui, Eric W. Hoppe, G. Crowder, C. Amole, B. Broerman, Shashank Priya, G. Giroux, Jie Zhang, K. Wierman, C. B. Krauss, A. Plante, M. Laurin, B. Loer, Amber M. Ortega, T. Hillier, D. M. Asner, V. Zacek, C. Licciardi, C. Cowles, S. Sahoo, L. Klopfenstein, A. E. Robinson, Karl J. Clark, N. Walkowski, Satyajit Seth, Yongke Yan, I. Stekl, I. Lawson, A. Sonnenschein, J. I. Collar, A. J. Noble, M. B. Crisler, I. J. Arnquist, U. Wichoski, C. E. Dahl, T. Kozynets, R. Podviyanuk, M. Ardid, D. Baxter, P. Mitra, P. Oedekerk, and Mala Das
Subjects: Physics, 010308 nuclear & particles physics, Endowment, Atomic energy, Library science, 01 natural sciences, Mine site, Regional development, 0103 physical sciences, Christian ministry, 010306 general physics, National laboratory, Engineering research, Underground space
Abstract: The PICO Collaboration wishes to thank SNOLAB and its staff for support through underground space, logistical and technical services. SNOLAB operations are supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site. We are grateful to Genevieve Belanger and Alexander Pukhov of the Universit e de Savoie for their useful correspondence regarding the interpretation of PICO results. We wish to acknowledge the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI) for funding. We acknowledge the support from the National Science Foundation (NSF) (Grants No. 0919526, No. 1506337, No. 1242637, No. 1205987, and No. 1806722). We acknowledge that this work is supported by the U.S. Department of Energy (DOE) Office of Science, Office of High Energy Physics (under Award No. DE-SC-0012161), by the DOE Office of Science Graduate Student Research (SCGSR) award, by DGAPA-UNAM (PAPIIT No. IA100118) and Consejo Nacional de Ciencia y Tecnologia (CONACyT, Mexico, Grants No. 252167 and No. A1-S-8960), by the Department of Atomic Energy (DAE), Government of India, under the Centre for AstroParticle Physics II project (CAPP-II) at the Saha Institute of Nuclear Physics (SINP), European Regional Development FundProject "Engineering applications of microworld physics" (No. CZ. 02.1.01/0.0/0.0/16_019/0000766), and the Spanish (Ministry of Science, Innovation and Universities) Ministerio de Ciencia, Innovacion y Universidades (Red Consolider MultiDark, FPA2017-90566-REDC). This work is partially supported by the Kavli Institute for Cosmological Physics at the University of Chicago through NSF Grant No. 1125897, and an endowment from the Kavli Foundation and its founder Fred Kavli. We also wish to acknowledge the support from Fermi National Accelerator Laboratory under Contract No. DE-AC02-07CH11359, and from Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. We also thank Compute Canada (www.computecanada.ca) and the Centre for Advanced Computing, ACENET, Calcul Quebec, Compute Ontario and WestGrid for computational support.
Published: 2019
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17. Search for Neutrinoless Double-Beta Decay with the Complete EXO-200 Dataset

Author: D. R. Yahne, B. T. Cleveland, A. Kuchenkov, V.N. Stekhanov, C. Chambers, J. Watkins, J. Farine, C. R. Hall, A. Dolgolenko, D. Fudenberg, A. Craycraft, Peter Fierlinger, Gerrit Wrede, M. Tarka, J. Hoessl, Jens Dilling, D. Ruddell, V. Belov, I. Badhrees, L. Darroch, R. MacLellan, A. Robinson, A. Karelin, Qing Xia, Thilo Michel, J. Runge, Yuehe Lin, A. Odian, M. Hughes, R. DeVoe, M. Wagenpfeil, U. Wichoski, L. J. Kaufman, I. Ostrovskiy, Z. Li, B. G. Lenardo, Petr Vogel, A. Pocar, T. Ziegler, M. Danilov, T. Brunner, David Leonard, Giorgio Gratta, A. Piepke, J. Todd, A. Larson, O. Nusair, R. Krücken, P. S. Barbeau, O. Njoya, Thomas Koffas, K. S. Kumar, S. X. Wu, David Moore, J. L. Vuilleumier, W. M. Fairbank, O. Ya. Zeldovich, A. Iverson, M. J. Dolinski, P. Gautam, Shu Li, S. Schmidt, J. Davis, C. Jessiman, W. R. Cen, B. Mong, Y. Lan, R. Gornea, E. V. Hansen, T. Tolba, M. J. Jewell, F. Retiere, A. S. Johnson, Liang Yang, A. Jamil, M. Coon, Douglas H Beck, T. Daniels, Guofu Cao, Y-R Yen, S. Feyzbakhsh, Arun Kumar Soma, G. S. Li, P. Hufschmidt, David A. Sinclair, D. Fairbank, C. Licciardi, A. Der Mesrobian-Kabakian, J. Echevers, B. Veenstra, T. I. Totev, T. McElroy, L. J. Wen, Marc Weber, Martin Breidenbach, S. J. Daugherty, T. Bhatta, V. Veeraraghavan, K. Murray, Gisela Anton, P. C. Rowson, and S. Delaquis
Subjects: Physics, Q value, Resolution (electron density), Detector, General Physics and Astronomy, FOS: Physical sciences, 01 natural sciences, Lower limit, ddc, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), 0103 physical sciences, Sensitivity (control systems), Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Energy (signal processing)
Abstract: A search for neutrinoless double-beta decay ($0\nu\beta\beta$) in $^{136}$Xe is performed with the full EXO-200 dataset using a deep neural network to discriminate between $0\nu\beta\beta$ and background events. Relative to previous analyses, the signal detection efficiency has been raised from 80.8% to 96.4$\pm$3.0% and the energy resolution of the detector at the Q-value of $^{136}$Xe $0\nu\beta\beta$ has been improved from $\sigma/E=1.23\%$ to $1.15\pm0.02\%$ with the upgraded detector. Accounting for the new data, the median 90% confidence level $0\nu\beta\beta$ half-life sensitivity for this analysis is $5.0 \cdot 10^{25}$ yr with a total $^{136}$Xe exposure of 234.1 kg$\cdot$yr. No statistically significant evidence for $0\nu\beta\beta$ is observed, leading to a lower limit on the $0\nu\beta\beta$ half-life of $3.5\cdot10^{25}$ yr at the 90% confidence level., Comment: v1, 7 pages, 5 figures; v2, fix references; v3, update to accepted version
Published: 2019

18. Characterization of the Hamamatsu VUV4 MPPCs for nEXO

Author: P. Giampa, G. Li, D. Kodroff, M. Wagenpfeil, J. Dalmasson, Eric W. Hoppe, N. Roy, David Leonard, J. Blatchford, Thomas Koffas, E. V. Hansen, W. M. Fairbank, P. Gautam, B. T. Cleveland, K. Odgers, L. Cao, Liang Yang, A. Jamil, S. Rescia, T. Stiegler, E. Raguzin, M. Elbeltagi, R. MacLellan, A. Kuchenkov, Arun Kumar Soma, F. Nolet, X.L. Sun, T. Bhatta, D. Fairbank, J. B. Zhao, T. McElroy, A. Larson, Jean-Francois Pratte, B. Mong, F. Vachon, Marc Weber, G. St-Hilaire, P. Margetak, P. Nakarmi, M. Chiu, J. Farine, J. Echevers, C. Chambers, G. Zhang, M. Oriunno, P. C. Rowson, A. Robinson, I. J. Arnquist, S. X. Wu, Douglas H Beck, Qing Xia, U. Wichoski, Ethan Brown, A. House, K. Murray, Y-R Yen, L. Darroch, G. S. Ortega, R. DeVoe, Gisela Anton, T. Ziegler, O. Zeldovich, J. P. Brodsky, T. I. Totev, M. Heffner, Qun-Yao Wang, T. Tolba, W. R. Cen, S. J. Daugherty, A. De St. Croix, G. Gallina, R. Gornea, Serge A. Charlebois, T. Rossignol, Zhijun Ning, M. Tarka, M. J. Jewell, Lorenzo Fabris, J. L. Vuilleumier, M. Walent, John L. Orrell, T. Daniels, R. Tsang, B. G. Lenardo, T. Brunner, K. Skarpaas, P. Lv, V. Veeraraghavan, A. Karelin, J. Todd, Y. Y. Ding, O. Nusair, R. Krücken, Veljko Radeka, Wei Wu, R.J. Newby, M. Hughes, R. Saldanha, S. Al Kharusi, Giorgio Gratta, Martin Ward, He-Run Yang, David Moore, M. Alfaris, S. Feyzbakhsh, A. Craycraft, Y. Ito, L. J. Kaufman, Y. Lan, Yuehe Lin, Z. Li, Samuele Sangiorgio, Wei Wei, F. Retière, K. S. Kumar, J. Hößl, P. S. Barbeau, V. A. Belov, Thilo Michel, J. Kroeger, Xuan Wu, A. Pocar, A. Piepke, V.N. Stekhanov, D. Qiu, M. Coon, Cory T. Overman, T. Tsang, Angelo Dragone, Gabriele Giacomini, Jens Dilling, I. Badhrees, S. Parent, A. Odian, I. Ostrovskiy, Gerard Visser, Mike Richman, O. Njoya, A. Iverson, Shu Li, J. Watkins, M. Medina-Peregrina, X. S. Jiang, C. Licciardi, A. Der Mesrobian-Kabakian, Yu-Guang Zhou, Liangjian Wen, Luca Doria, Guofu Cao, Rejean Fontaine, and M. J. Dolinski
Subjects: 010302 applied physics, Physics, Nuclear and High Energy Physics, Scintillation, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Analytical chemistry, FOS: Physical sciences, chemistry.chemical_element, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, Xenon, chemistry, 0103 physical sciences, Saturation (graph theory), Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Instrumentation, Photon detection, Dark current
Abstract: In this paper we report on the characterization of the Hamamatsu VUV4 (S/N: S13370-6152) Vacuum Ultra-Violet (VUV) sensitive Multi-Pixel Photon Counters (MPPC)s as part of the development of a solution for the detection of liquid xenon scintillation light for the nEXO experiment. Various MPPC features, such as: dark noise, gain, correlated avalanches, direct crosstalk and Photon Detection Efficiency (PDE) were measured in a dedicated setup at TRIUMF. MPPCs were characterized in the range 163 K ≤ T ≤ 233 K . At an over voltage of 3 . 1 ± 0 . 2 V and at T = 163 K we report a number of Correlated Avalanches (CAs) per pulse in the 1 μ s interval following the trigger pulse of 0 . 161 ± 0 . 005 . At the same settings the Dark-Noise (DN) rate is 0 . 137 ± 0 . 002 Hz/mm 2 . Both the number of CAs and the DN rate are within nEXO specifications. The PDE of the Hamamatsu VUV4 was measured for two different devices at T = 233 K for a mean wavelength of 189 ± 7 nm . At 3 . 6 ± 0 . 2 V and 3 . 5 ± 0 . 2 V of over voltage we report a PDE of 13 . 4 ± 2 . 6 % and 11 ± 2 % , corresponding to a saturation PDE of 14 . 8 ± 2 . 8 % and 12 . 2 ± 2 . 3 % , respectively. Both values are well below the 24 % saturation PDE advertised by Hamamatsu. More generally, the second device tested at 3 . 5 ± 0 . 2 V of over voltage is below the nEXO PDE requirement. The first one instead yields a PDE that is marginally close to meeting the nEXO specifications. This suggests that with modest improvements the Hamamatsu VUV4 MPPCs could be considered as an alternative to the FBK-LF Silicon Photo-Multipliers for the final design of the nEXO detector.
Published: 2019

19. Reflectance of Silicon Photomultipliers at Vacuum Ultraviolet Wavelengths

Author: E. Caden, S. Rescia, D. Fairbank, G. St-Hilaire, Thilo Michel, A. Craycraft, Jens Dilling, I. Badhrees, A. De St. Croix, X. S. Jiang, C. Licciardi, J. Farine, M. Walent, S. Feyzbakhsh, V. Belov, C.R. Natzke, B. G. Lenardo, A. Robinson, P. Nakarmi, A. Der Mesrobian-Kabakian, T. Brunner, L. Darroch, J. Echevers, Xuan Wu, S. Parent, A. Odian, A. Fucarino, Jean-Francois Pratte, Yu-Guang Zhou, E. Raguzin, T. Rossignol, Z. Li, O. Nusair, J. L. Vuilleumier, R. Krücken, M. Hughes, V. Veeraraghavan, M. J. Jewell, R. Saldanha, T. I. Totev, P. A. Breur, K. Skarpaas, Gerard Visser, S. Al Kharusi, I. Ostrovskiy, B. T. Cleveland, A. Kuchenkov, Liangjian Wen, Luca Doria, Guofu Cao, Samuele Sangiorgio, Wei Wei, K. S. Kumar, Mike Richman, David Moore, O. Njoya, A. Iverson, T. Bhatta, M. Chiu, G. S. Li, Thomas Tsang, Shu Li, Y. Lan, B. Chana, Douglas H Beck, L. Yang, M. Oriunno, J. P. Brodsky, P. S. Barbeau, He-Run Yang, R. DeVoe, K. Murray, J. Watkins, M. Tarka, Gisela Anton, R. Tsang, M. L. di Vacri, K. Odgers, M. J. Dolinski, M. Medina-Peregrina, C. Vivo-Vilches, F. Retiere, U. Wichoski, Sergio Ferrara, O. Zeldovich, K. G. Leach, T. Ziegler, R. Gornea, K. Deslandes, David Leonard, Giorgio Gratta, Thomas Koffas, W. M. Fairbank, Wei Wu, R.J. Newby, P. C. Rowson, T. Stiegler, M. Elbeltagi, Lorenzo Fabris, J. Hobl, A. House, N. Roy, L. Cao, F. Nolet, N. Massacret, T. McElroy, S. X. Wu, F. Vachon, C. Chambers, R. MacLellan, A. Pocar, V.N. Stekhanov, P. Gautam, F. Edaltafar, D. Goeldi, M. Coon, I. J. Arnquist, J. Runge, Cory T. Overman, M. Heffner, S. Viel, G. Gallina, Angelo Dragone, Gabriele Giacomini, P. Lv, A. Piepke, J. Todd, Y. Y. Ding, Veljko Radeka, T. Wager, Qun-Yao Wang, Zhijun Ning, E. V. Hansen, A. Jamil, Arun Kumar Soma, Qing Xia, S. Byrne Mamahit, Ethan Brown, A. Karelin, G. S. Ortega, M. Wagenpfeil, J. Dalmasson, X.L. Sun, J. B. Zhao, A. Larson, Serge A. Charlebois, John L. Orrell, T. Daniels, B. Mong, L. J. Kaufman, and Eric W. Hoppe
Subjects: Nuclear and High Energy Physics, Materials science, Physics - Instrumentation and Detectors, Silicon, chemistry.chemical_element, Photodetector, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Xenon, Silicon photomultiplier, 0103 physical sciences, Wafer, Electrical and Electronic Engineering, 010308 nuclear & particles physics, business.industry, Instrumentation and Detectors (physics.ins-det), Nuclear Energy and Engineering, chemistry, Optoelectronics, Diffuse reflection, Photonics, business, Refractive index
Abstract: Characterization of the vacuum ultraviolet (VUV) reflectance of silicon photomultipliers (SiPMs) is important for large-scale SiPM-based photodetector systems. We report the angular dependence of the specular reflectance in a vacuum of SiPMs manufactured by Fondazionc Bruno Kessler (FBK) and Hamamatsu Photonics K.K. (HPK) over wavelengths ranging from 120 nm to 280 nm. Refractive index and extinction coefficient of the thin silicon-dioxide film deposited on the surface of the FBK SiPMs are derived from reflectance data of a FBK silicon wafer with the same deposited oxide film as SiPMs. The diffuse reflectance of SiPMs is also measured at 193 nm. We use the VUV spectral dependence of the optical constants to predict the reflectance of the FBK silicon wafer and FBK SiPMs in liquid xenon.
Published: 2019
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20. Simulation of charge readout with segmented tiles in nEXO

Author: F. Retière, M. Medina-Peregrina, Venkatesh Veeraraghavan, J. Hößl, Gerard Visser, J. L. Vuilleumier, L. Darroch, M. Chiu, J. Watkins, V. A. Belov, Yang Haibo, A. De St. Croix, V. Radeka, D. Fairbank, T. McElroy, T. Bhatta, A. Pocar, D. S. Leonard, J. Echevers, E. Caden, A. Craycraft, R. DeVoe, Lorenzo Fabris, C. T. Overman, E. Raguzin, C. Vivo-Vilches, Qing Xia, M. J. Jewell, Xiaoyang Sun, R. Gornea, J. Dalmasson, S. Feyzbakhsh, P. Gautam, G. S. Ortega, A. Piepke, I. Ostrovskiy, P. Lv, M. Hughes, Thilo Michel, T. Ziegler, C.R. Natzke, Z. Ning, Xuan Wu, F. Vachon, Sergio Ferrara, Serge A. Charlebois, S. X. Wu, V.N. Stekhanov, M. Walent, S. Al Kharusi, J. B. Zhao, A. Larson, A. Der Mesrobian-Kabakian, A. E. Robinson, Mike Richman, B. G. Lenardo, T. Brunner, A. Fucarino, David Moore, N. Roy, L. Cao, F. Nolet, J. Todd, M. Heffner, D. Kodroff, T. Tolba, Jean-Francois Pratte, M. Oriunno, John L. Orrell, T. Daniels, B. Mong, Rejean Fontaine, Ethan Brown, Qian Wang, Y. Lan, K. Murray, G. Giacomini, T. Stiegler, O. Njoya, A. Iverson, K. Skarpaas Viii, Thomas Tsang, R. Saldanha, Shu Li, Y. Y. Ding, Z. Li, Gisela Anton, O. Zeldovich, Marc Weber, E. Hansen, A. Karelin, O. Nusair, R. Krücken, Jens Dilling, R. MacLellan, B. Chana, Giorgio Gratta, P. S. Barbeau, Yumei Zhou, I. Badhrees, R. Tsang, Martin Ward, T. I. Totev, D. Goeldi, M. Coon, Liangjian Wen, Douglas H Beck, Guofu Cao, Angelo Dragone, W. R. Cen, S. J. Daugherty, Thomas Koffas, Xiaoshan Jiang, W. M. Fairbank, M. Elbeltagi, Y-R Yen, S. Rescia, M. J. Dolinski, A. Odian, S. Parent, J. Runge, J. P. Brodsky, P. Nakarmi, U. Wichoski, S. Viel, C. Licciardi, G. Gallina, T. Rossignol, M. L. Di Vacri, L. J. Kaufman, Eric W. Hoppe, Liang Yang, A. Jamil, Arun Kumar Soma, Yuehe Lin, Samuele Sangiorgio, Wei Wei, K. S. Kumar, J. Farine, I. J. Arnquist, K. G. Leach, G. St-Hilaire, Wei Wu, R.J. Newby, P. C. Rowson, A. House, M. Tarka, G. Li, B. T. Cleveland, K. Odgers, A. Kuchenkov, M. Wagenpfeil, and C. Chambers
Subjects: Physics, Physics - Instrumentation and Detectors, Time projection chamber, 010308 nuclear & particles physics, Detector, chemistry.chemical_element, FOS: Physical sciences, Charge (physics), Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 030218 nuclear medicine & medical imaging, Anode, Nuclear physics, 03 medical and health sciences, 0302 clinical medicine, Xenon, chemistry, Double beta decay, 0103 physical sciences, Beta (velocity), Sensitivity (control systems), Nuclear Experiment (nucl-ex), Nuclear Experiment, Instrumentation, Mathematical Physics
Abstract: nEXO is a proposed experiment to search for the neutrino-less double beta decay ($0\nu\beta\beta$) of $^{136}$Xe in a tonne-scale liquid xenon time projection chamber (TPC). The nEXO TPC will be equipped with charge collection tiles to form the anode. In this work, the charge reconstruction performance of this anode design is studied with a dedicated simulation package. A multi-variate method and a deep neural network are developed to distinguish simulated $0\nu\beta\beta$ signals from backgrounds arising from trace levels of natural radioactivity in the detector materials. These simulations indicate that the nEXO TPC with charge-collection tiles shows promising capability to discriminate the $0\nu\beta\beta$ signal from backgrounds. The estimated half-life sensitivity for $0\nu\beta\beta$ decay is improved by $\sim$20$~(32)\%$ with the multi-variate~(deep neural network) methods considered here, relative to the sensitivity estimated in the nEXO pre-conceptual design report.
Published: 2019
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21. Reflectivity and PDE of VUV4 Hamamatsu SiPMs in Liquid Xenon

Author: Gerard Visser, M. Walent, B. G. Lenardo, T. Brunner, V. Veeraraghavan, T. Bhatta, Giorgio Gratta, F. Edaltafar, T. Rossignol, M. J. Jewell, J. Watkins, P. Nakarmi, Arun Kumar Soma, Ethan Brown, L. Darroch, O. Nusair, R. Krücken, S. X. Wu, David Leonard, J. Blatchford, E. Caden, Thomas Koffas, W. M. Fairbank, T. Stiegler, M. Elbeltagi, L. J. Kaufman, M. Hughes, X. S. Jiang, C. Licciardi, A. Craycraft, Eric W. Hoppe, S. Al Kharusi, A. Karelin, G. Gallina, P. Gautam, R. Saldanha, M. Chiu, J. L. Vuilleumier, T. Wager, A. Der Mesrobian-Kabakian, David Moore, C. Chambers, M. Oriunno, E. V. Hansen, M. Alfaris, M. Wagenpfeil, J. Dalmasson, Sergio Ferrara, R. MacLellan, Qun-Yao Wang, K. Murray, Gabriele Giacomini, I. J. Arnquist, Liang Yang, Y. Lan, U. Wichoski, C.R. Natzke, S. Feyzbakhsh, A. Jamil, Gisela Anton, J. Runge, Zhijun Ning, T. Ziegler, K. G. Leach, R. Tsang, X.L. Sun, J. B. Zhao, M. Heffner, K. Odgers, S. Viel, Wei Wu, R.J. Newby, A. Fucarino, A. Larson, Z. Li, B. Chana, Douglas H Beck, Samuele Sangiorgio, K. S. Kumar, Veljko Radeka, P. C. Rowson, A. House, N. Massacret, Jean-Francois Pratte, P. Lv, J. Todd, Angelo Dragone, B. Mong, Y. Y. Ding, M. Ward, T. I. Totev, G. S. Li, M. L. di Vacri, R. DeVoe, C. Vivo-Vilches, Qing Xia, S. Byrne Mamahit, G. S. Ortega, R. Fontaine, J. Farine, Serge A. Charlebois, John L. Orrell, T. Daniels, V. Belov, A. Robinson, N. Roy, L. Cao, F. Nolet, T. McElroy, F. Vachon, Marc Weber, A. De St. Croix, Lorenzo Fabris, B. T. Cleveland, D. Goeldi, M. Coon, A. Kuchenkov, Cory T. Overman, S. Rescia, D. Fairbank, G. St-Hilaire, J. P. Brodsky, He-Run Yang, A. Piepke, M. Tarka, V.N. Stekhanov, J. Echevers, A. Pocar, O. Zeldovich, Yu-Guang Zhou, Liangjian Wen, Luca Doria, Guofu Cao, Thilo Michel, Wei Wei, I. Ostrovskiy, M. J. Dolinski, E. Raguzin, P. A. Breur, Xuan Wu, Mike Richman, F. Retière, O. Njoya, A. Iverson, M. Medina-Peregrina, J. Hößl, K. Skarpaas Viii, P. S. Barbeau, Thomas Tsang, Shu Li, R. Gornea, Jens Dilling, I. Badhrees, S. Parent, and A. Odian
Subjects: Materials science, Physics - Instrumentation and Detectors, APDS, Physics::Instrumentation and Detectors, Photodetector, chemistry.chemical_element, FOS: Physical sciences, Photodetection, 01 natural sciences, 030218 nuclear medicine & medical imaging, law.invention, High Energy Physics - Experiment, 03 medical and health sciences, High Energy Physics - Experiment (hep-ex), 0302 clinical medicine, Silicon photomultiplier, Optics, Xenon, law, 0103 physical sciences, Specular reflection, Instrumentation, Mathematical Physics, Scintillation, 010308 nuclear & particles physics, business.industry, Instrumentation and Detectors (physics.ins-det), Wavelength, chemistry, business
Abstract: Understanding reflective properties of materials and photodetection efficiency (PDE) of photodetectors is important for optimizing energy resolution and sensitivity of the next generation neutrinoless double beta decay, direct detection dark matter, and neutrino oscillation experiments that will use noble liquid gases, such as nEXO, DARWIN, DarkSide-20k, and DUNE. Little information is currently available about reflectivity and PDE in liquid noble gases, because such measurements are difficult to conduct in a cryogenic environment and at short enough wavelengths. Here we report a measurement of specular reflectivity and relative PDE of Hamamatsu VUV4 silicon photomultipliers (SiPMs) with 50 micrometer micro-cells conducted with xenon scintillation light (~175 nm) in liquid xenon. The specular reflectivity at 15 deg. incidence of three samples of VUV4 SiPMs is found to be 30.4+/-1.4%, 28.6+/-1.3%, and 28.0+/-1.3%, respectively. The PDE at normal incidence differs by +/-8% (standard deviation) among the three devices. The angular dependence of the reflectivity and PDE was also measured for one of the SiPMs. Both the reflectivity and PDE decrease as the angle of incidence increases. This is the first measurement of an angular dependence of PDE and reflectivity of a SiPM in liquid xenon., Comment: 21 pages, 15 figures, 6 tables. As accepted by JINST
Published: 2019
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22. Measurement of the scintillation and ionization response of liquid xenon at MeV energies in the EXO-200 experiment

Author: E. V. Hansen, D. Fudenberg, Liang Yang, A. Jamil, M. J. Jewell, L. Darroch, M. Wagenpfeil, Giorgio Gratta, M. J. Dolinski, P. Hufschmidt, David A. Sinclair, G. S. Li, Thilo Michel, D. Fairbank, J. L. Vuilleumier, M. Hughes, T. Bhatta, R. MacLellan, A.C. Odian, I. Ostrovskiy, A. Larson, T. Tolba, P. C. Rowson, C. Jessiman, A. Pocar, C. Licciardi, J. Echevers, B. Mong, O. Ya. Zeldovich, A. Der Mesrobian-Kabakian, R. Neilson, T. Brunner, S. Delaquis, L. J. Kaufman, T. McElroy, David Moore, A. Karelin, A. S. Johnson, J. Watkins, V. Veeraraghavan, L. J. Wen, Marc Weber, Arun Kumar Soma, V.N. Stekhanov, S. X. Wu, D. R. Yahne, C. R. Hall, R. DeVoe, A. Piepke, J. Todd, Martin Breidenbach, David Leonard, S. J. Daugherty, O. Njoya, J. Farine, A. Dolgolenko, A. Craycraft, D. Beck, Thomas Koffas, Qing Xia, D. Tosi, W. M. Fairbank, A. Iverson, C. Chambers, J. Hoessl, P. S. Barbeau, J. Runge, W. R. Cen, R. Gornea, M. Coon, Y-R Yen, Shu Li, S. Schmidt, Guofu Cao, A. Robinson, F. Retiere, V. A. Belov, O. Nusair, R. Krücken, Jens Dilling, B. Veenstra, K. Murray, I. Badhrees, T. I. Totev, P. Gautam, T. Daniels, J. Davis, Gisela Anton, Z. Li, U. Wichoski, T. Ziegler, B. G. Lenardo, Peter Fierlinger, Gerrit Wrede, M. Tarka, B. T. Cleveland, A. Kuchenkov, Y. Lan, S. Feyzbakhsh, Yuehe Lin, and K. S. Kumar
Subjects: Physics, Scintillation, Range (particle radiation), Physics - Instrumentation and Detectors, Photon, Argon, 010308 nuclear & particles physics, Physics::Instrumentation and Detectors, chemistry.chemical_element, FOS: Physical sciences, Electron, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 7. Clean energy, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Xenon, chemistry, Electric field, Ionization, 0103 physical sciences, 010306 general physics
Abstract: Liquid xenon (LXe) is employed in a number of current and future detectors for rare event searches. We use the EXO-200 experimental data to measure the absolute scintillation and ionization yields generated by $\gamma$ interactions from $^{228}$Th (2615~keV), $^{226}$Ra (1764~keV) and $^{60}$Co (1332~keV and 1173~keV) calibration sources, over a range of electric fields. The $W$-value that defines the recombination-independent energy scale is measured to be $11.5~\pm~0.5$~(syst.)~$\pm~0.1$~(stat.) eV. These data are also used to measure the recombination fluctuations in the number of electrons and photons produced by the calibration sources at the MeV-scale, which deviate from extrapolations of lower-energy data. Additionally, a semi-empirical model for the energy resolution of the detector is developed, which is used to constrain the recombination efficiency, i.e., the fraction of recombined electrons that result in the emission of a detectable photon. Detailed measurements of the absolute charge and light yields for MeV-scale electron recoils are important for predicting the performance of future neutrinoless double beta decay detectors.
Published: 2019
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23. Deep Neural Networks for Energy and Position Reconstruction in EXO-200

Author: P. C. Rowson, Y.-R. Yen, A. Pocar, Douglas H Beck, J. C. Davis, W. Cree, T. Richards, Venkatesh Veeraraghavan, S. Delaquis, P. Hufschmidt, R. Krücken, M. Hughes, A. P. Waite, A. Karelin, Thomas Koffas, David Moore, W. M. Fairbank, Arun Kumar Soma, P. S. Barbeau, D. Fudenberg, A. Piepke, A. Craycraft, David A. Sinclair, M. J. Dolinski, Yuehe Lin, R. Bayerlein, Martin Breidenbach, G. S. Li, S. J. Daugherty, J. Dalmasson, V.N. Stekhanov, G. Wrede, K. S. Kumar, Stefan Schmidt, M. Tarka, A. Der Mesrobian-Kabakian, D. A. Harris, B. Mong, T. Daniels, C. R. Hall, Y. Lan, R. DeVoe, C. Chambers, J. Farine, Giorgio Gratta, Mikhail Danilov, U. Wichoski, A. S. Johnson, J. Todd, B. T. Cleveland, W. R. Cen, A. Kuchenkov, T. Ziegler, T. Tolba, A. Robinson, M. Wagenpfeil, R. MacLellan, M. Coon, J. L. Vuilleumier, E. V. Hansen, M. J. Jewell, J. Watkins, Liang Yang, D. S. Leonard, A. Jamil, S. Feyzbakhsh, Thilo Michel, Qing Xia, P. Fierlinger, C. Licciardi, Liangjian Wen, Guofu Cao, K. Murray, Gisela Anton, T. Brunner, L. J. Kaufman, O. Ya. Zeldovich, A. Dolgolenko, J. Hoessl, A. Schubert, Marc Weber, J. Daughhetee, F. Retière, J. B. Albert, V. A. Belov, R. Gornea, I. Ostrovskiy, O. Njoya, A. Iverson, Shu Li, Jens Dilling, I. Badhrees, A. Odian, and S. Kravitz
Subjects: Physics - Instrumentation and Detectors, Artificial neural network, 010308 nuclear & particles physics, Computer science, Calibration (statistics), Monte Carlo method, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Position (vector), 0103 physical sciences, Pattern recognition (psychology), Waveform, Nuclear Experiment (nucl-ex), 010306 general physics, Instrumentation, Algorithm, Nuclear Experiment, Mathematical Physics, Energy (signal processing), Event reconstruction
Abstract: We apply deep neural networks (DNN) to data from the EXO-200 experiment. In the studied cases, the DNN is able to reconstruct the relevant parameters - total energy and position - directly from raw digitized waveforms, with minimal exceptions. For the first time, the developed algorithms are evaluated on real detector calibration data. The accuracy of reconstruction either reaches or exceeds what was achieved by the conventional approaches developed by EXO-200 over the course of the experiment. Most existing DNN approaches to event reconstruction and classification in particle physics are trained on Monte Carlo simulated events. Such algorithms are inherently limited by the accuracy of the simulation. We describe a unique approach that, in an experiment such as EXO-200, allows to successfully perform certain reconstruction and analysis tasks by training the network on waveforms from experimental data, either reducing or eliminating the reliance on the Monte Carlo., Accepted version. 33 pages, 28 figures
Published: 2018

24. Search for nucleon decays with EXO-200

Author: M. Hughes, E. V. Hansen, A. P. Waite, Simon Johnston, T. Tolba, A.C. Odian, Liang Yang, A. Jamil, C. R. Hall, David Moore, O. Ya. Zeldovich, G. S. Li, T. Didberidze, B. T. Cleveland, L. J. Kaufman, Martin Breidenbach, R. MacLellan, M. Coon, S. J. Daugherty, R. DeVoe, R. H. Nelson, A. Pocar, U. Wichoski, Arun Kumar Soma, C. Chambers, P. C. Rowson, Petr Vogel, P. S. Barbeau, Guofu Cao, M. Danilov, M. J. Jewell, T. Ziegler, W. Cree, Yuehe Lin, David Leonard, V. A. Belov, Thomas Koffas, W. M. Fairbank, S. Delaquis, F. Retiere, K. S. Kumar, J. Zettlemoyer, S. Feyzbakhsh, V.N. Stekhanov, Douglas H Beck, J. C. Davis, Y-R Yen, A. Craycraft, B. Mong, D. Fudenberg, Samuel Homiller, J. Daughhetee, A. Piepke, K. Graham, M. J. Dolinski, C. Licciardi, A. Der Mesrobian-Kabakian, Peter Fierlinger, R. Bayerlein, Gerrit Wrede, A. Johnson, Thilo Michel, A. Karelin, Giorgio Gratta, M. Tarka, J. Farine, A. Dolgolenko, K. Murray, Y. Lan, J. Hoessl, P. Hufschmidt, M. Wagenpfeil, David A. Sinclair, Gisela Anton, A. Robinson, T. Walton, T. Brunner, Alexis G. Schubert, A. Kuchenkov, Justin Albert, R. Tsang, W. R. Cen, R. Gornea, L. J. Wen, Marc Weber, R. Krücken, Jens Dilling, I. Badhrees, T. Daniels, J.-L. Vuilleumier, S. Kravitz, I. Ostrovskiy, O. Njoya, Shu Li, and S. Schmidt
Subjects: Particle physics, Physics - Instrumentation and Detectors, Hadron, FOS: Physical sciences, Elementary particle, nucl-ex, 01 natural sciences, Atomic, High Energy Physics - Experiment, Nuclear physics, Particle decay, High Energy Physics - Experiment (hep-ex), Particle and Plasma Physics, 0103 physical sciences, Isotopes of xenon, Nuclear, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, physics.ins-det, Physics, Quantum Physics, Isotope, 010308 nuclear & particles physics, hep-ex, Molecular, Fermion, Instrumentation and Detectors (physics.ins-det), Nuclear & Particles Physics, ddc, Baryon, Nucleon, Astronomical and Space Sciences
Abstract: A search for instability of nucleons bound in Xe136 nuclei is reported with 223 kg·yr exposure of Xe136 in the EXO-200 experiment. Lifetime limits of 3.3×1023 and 1.9×1023 yr are established for nucleon decay to Sb133 and Te133, respectively. These are the most stringent to date, exceeding the prior decay limits by a factor of 9 and 7, respectively.
Published: 2018
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25. VUV-sensitive Silicon Photomultipliers for Xenon Scintillation Light Detection in nEXO

Author: A. Jamil, T. Ziegler, P. Hufschmidt, G. Li, L. Lupin-Jimenez, T. Michel, I. Ostrovskiy, F. Retiere, J. Schneider, M. Wagenpfeil, A. Alamre, J. B. Albert, G. Anton, I. J. Arnquist, I. Badhrees, P. S. Barbeau, D. Beck, V. Belov, T. Bhatta, F. Bourque, J. P. Brodsky, E. Brown, T. Brunner, A. Burenkov, G. F. Cao, L. Cao, W. R. Cen, C. Chambers, S. A. Charlebois, M. Chiu, B. Cleveland, M. Coon, M. Cote, A. Craycraft, W. Cree, J. Dalmasson, T. Daniels, L. Darroch, S. J. Daugherty, J. Daughhetee, S. Delaquis, A. Der Mesrobian-Kabakian, R. DeVoe, J. Dilling, Y. Y. Ding, M. J. Dolinski, A. Dragone, J. Echevers, L. Fabris, D. Fairbank, W. Fairbank, J. Farine, S. Feyzbakhsh, R. Fontaine, D. Fudenberg, G. Gallina, G. Giacomini, R. Gornea, G. Gratta, E. V. Hansen, D. Harris, M. Hasan, M. Heffner, J. HoBl, E. W. Hoppe, A. House, M. Hughes, Y. Ito, A. Iverson, C. Jessiman, M. J. Jewell, X. S. Jiang, A. Karelin, L. J. Kaufman, T. Koffas, S. Kravitz, R. Krucken, A. Kuchenkov, K. S. Kumar, Y. Lan, A. Larson, D. S. Leonard, S. Li, Z. Li, C. Licciardi, Y. H. Lin, P. Lv, R. MacLellan, B. Mong, D. C. Moore, K. Murray, R. J. Newby, Z. Ning, O. Njoya, F. Nolet, O. Nusair, K. Odgers, A. Odian, M. Oriunno, J. L. Orrell, G. S. Ortega, C. T. Overman, S. Parent, A. Piepke, A. Pocar, J.-F. Pratte, D. Qiu, V. Radeka, E. Raguzin, T. Rao, S. Rescia, A. Robinson, T. Rossignol, P. C. Rowson, N. Roy, R. Saldanha, S. Sangiorgio, S. Schmidt, A. Schubert, D. Sinclair, K. Skarpaas, A. K. Soma, G. St-Hilaire, V. Stekhanov, T. Stiegler, X. L. Sun, M. Tarka, J. Todd, T. Tolba, T. I. Totev, R. Tsang, T. Tsang, F. Vachon, B. Veenstra, V. Veeraraghavan, G. Visser, J.-L. Vuilleumier, Q. Wang, J. Watkins, M. Weber, W. Wei, L. J. Wen, U. Wichoski, G. Wrede, S. X. Wu, W. H. Wu, Q. Xia, L. Yang, Y.-R. Yen, O. Zeldovich, X. Zhang, J. Zhao, and Y. Zhou
Subjects: Physics, Nuclear and High Energy Physics, Photomultiplier, Scintillation, Time projection chamber, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, Noble gas, chemistry.chemical_element, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Avalanche photodiode, 01 natural sciences, Optics, Silicon photomultiplier, Xenon, Nuclear Energy and Engineering, chemistry, Double beta decay, 0103 physical sciences, Electrical and Electronic Engineering, 010306 general physics, business
Abstract: Future tonne-scale liquefied noble gas detectors depend on efficient light detection in the VUV range. In the past years Silicon Photomultipliers (SiPMs) have emerged as a valid alternative to standard photomultiplier tubes or large area avalanche photodiodes. The next generation double beta decay experiment, nEXO, with a 5 tonne liquid xenon time projection chamber, will use SiPMs for detecting the $178\,\text{nm}$ xenon scintillation light, in order to achieve an energy resolution of $\sigma / Q_{\beta\beta} = 1\, \%$. This paper presents recent measurements of the VUV-HD generation SiPMs from Fondazione Bruno Kessler in two complementary setups. It includes measurements of the photon detection efficiency with gaseous xenon scintillation light in a vacuum setup and dark measurements in a dry nitrogen gas setup. We report improved photon detection efficiency at $175\,\text{nm}$ compared to previous generation devices, that would meet the criteria of nEXO. Furthermore, we present the projected nEXO detector light collection and energy resolution that could be achieved by using these SiPMs., Comment: 11 pages, 13 figures, 2 tables
Published: 2018
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26. An RF-only ion-funnel for extraction from high-pressure gases

Author: David Leonard, Thomas Koffas, W. M. Fairbank, T. Daniels, F. Retière, R. MacLellan, D. Fudenberg, J. Farine, P. S. Barbeau, I. Ostrovskiy, F. Leonard, R. Gornea, Marc Weber, D. Tosi, E. Smith, P. C. Rowson, Douglas H Beck, J. Walton, Y-R Yen, K. Graham, U. Wichoski, David A. Sinclair, J. L. Vuilleumier, M. Heffner, A. Craycraft, Monica Dunford, A. Piepke, M. Hughes, A. Sabourov, T. Tolba, A. Schubert, J. B. Albert, W. Feldmeier, L. J. Kaufman, David Moore, T. Didberidze, M. Tarka, B. Mong, D. J. Auty, C. Licciardi, V.N. Stekhanov, T. Brunner, Yuehe Lin, A. Karelin, Martin Breidenbach, S. J. Daugherty, C. Benitez-Medina, Ryan Killick, R. DeVoe, Lorenzo Fabris, C. Chambers, B. T. Cleveland, K. S. Kumar, A. Pocar, C. Ouellet, A. Kuchenkov, Giorgio Gratta, S. Kravitz, V. Varentsov, Liang Yang, Jens Dilling, M. Coon, T. N. Johnson, M. J. Jewell, A. Odian, K. Twelker, X. S. Jiang, R. Krücken, T. Walton, M. P. Rozo, M. J. Dolinski, Michael G. Marino, S. Johnston, P. Fierlinger, Liangjian Wen, and Guofu Cao
Subjects: Physics - Instrumentation and Detectors, Trace Amounts, Physics::Instrumentation and Detectors, FOS: Physical sciences, chemistry.chemical_element, 01 natural sciences, Ion, Xenon, Ionization, 0103 physical sciences, Nuclear Experiment (nucl-ex), Physical and Theoretical Chemistry, 010306 general physics, Nuclear Experiment, Instrumentation, Spectroscopy, Time projection chamber, Chemistry, 010401 analytical chemistry, Extraction (chemistry), Barium, Instrumentation and Detectors (physics.ins-det), Condensed Matter Physics, 0104 chemical sciences, 13. Climate action, Atomic physics, Bar (unit)
Abstract: An RF ion-funnel technique has been developed to extract ions from a high-pressure (10 bar) noble-gas environment into a vacuum (10(-6) mbar). Detailed simulations have been performed and a prototype has been developed for the purpose of extracting Ba-136 ions from Xe gas with high efficiency. With this prototype, ions have been extracted for the first time from high-pressure xenon gas and argon gas. Systematic studies have been carried out and compared to simulations. This demonstration of extraction of ions, with mass comparable to that of the gas generating the high-pressure, has applications to Ba tagging from a Xe-gas time-projection chamber for double-beta decay, as well as to the general problem of recovering trace amounts of an ionized element in a heavy (m > 40 u) carrier gas. (C) 2015 Elsevier B.V. All rights reserved.
Published: 2015
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27. Searching for Dark Matter with PICASSO

Author: P. Mitra, Stanislav Pospisil, Pijushpani Bhattacharjee, I. Levine, S. Gagnebin, U. Wichoski, I. Stekl, M. Besnier, S. Archambault, C. B. Krauss, F. Debris, I. T. Lawson, N. Dhungana, A. Davour, G. Giroux, A. Kamaha, S. Seth, O. Scallon, E. Behnke, E. Grace, L. Lessard, D. Marlisov, M.-C. Piro, Mala Das, M. Lafrenière, C. M. Jackson, M. Laurin, V. Zacek, C. Levy, S. Kumaratunga, J. P. Martin, N. Starinski, J. Farine, T. Xie, A. Plante, A. J. Noble, R. Podviyanuk, X. Dai, and M. Fines-Neuschild
Subjects: Physics, Particle physics, Physics::Instrumentation and Detectors, Dark matter, Massive particle, PICASSO, Electron, SNOLAB, Physics and Astronomy(all), WIMPs, Nuclear physics, Superheated Liquids, WIMP, Weakly interacting massive particles, Dark Matter, Bubble chamber, Particle
Abstract: The Project In CAnada to Search for Supersymmetric Objects (PICASSO) at SNOLAB searches for Weakly Interacting Massive Particle (WIMP) interactions with 19 F. It is particularly sensitive to spin-dependent particle interactions. It uses a droplet technique, based on the principle of a bubble chamber, in which phase transitions in superheated liquids can be triggered by WIMP induced nuclear recoils. The detection process allows a highly e ffi cient suppression of backgrounds from cosmic muons, γ rays and electrons. Recent results and progress are presented and future plans to scale this technique to large masses with the PICO collaboration are briefly discussed.
Published: 2015
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28. Searches for double beta decay of Xe134 with EXO-200

Author: L. J. Kaufman, Yuehe Lin, J. J. Russell, K. S. Kumar, T. Michel, Douglas H Beck, T. Daniels, Y-R Yen, J. Walton, M. Danilov, M. J. Jewell, I. Ostrovskiy, C. R. Hall, Y. Lan, David Leonard, A. S. Johnson, P. C. Rowson, J. Daughhetee, R. DeVoe, J. B. Albert, Petr Vogel, O. Ya. Zeldovich, A. Schubert, R. MacLellan, W. Cree, Thomas Koffas, W. M. Fairbank, J. Hoessl, O. Njoya, S. Delaquis, A.C. Odian, F. Retiere, P. Hufschmidt, Shu Li, R. Krücken, M. Hughes, Peter Fierlinger, S. Feyzbakhsh, J. Zettlemoyer, A. P. Waite, David A. Sinclair, A. Der Mesrobian-Kabakian, J. L. Vuilleumier, C. Licciardi, M. Tarka, P. S. Barbeau, A. Craycraft, K. Graham, Jens Dilling, I. Badhrees, C. Chambers, E. Smith, Martin Breidenbach, R. Bayerlein, A. Piepke, A. Karelin, Michael G. Marino, S. J. Daugherty, K. Murray, S. Johnston, David Moore, T. Didberidze, R. H. Nelson, B. T. Cleveland, Gisela Anton, T. Walton, A. Kuchenkov, J. Davis, M. Wagenpfeil, Guofu Cao, U. Wichoski, A. Dolgolenko, B. Mong, Giorgio Gratta, T. Ziegler, T. Tolba, L. J. Wen, Marc Weber, D. Fudenberg, M. J. Dolinski, S. Kravitz, Liang Yang, A. Jamil, R. Tsang, W. R. Cen, R. Gornea, M. Coon, A. Pocar, J. Farine, V. Belov, V.N. Stekhanov, and T. Brunner
Subjects: Physics, Particle physics, Isotope, 010308 nuclear & particles physics, chemistry.chemical_element, 01 natural sciences, Beta decay, Particle detector, 3. Good health, Nuclear physics, Xenon, chemistry, Double beta decay, 0103 physical sciences, Isotopes of xenon, Nuclear astrophysics, 010306 general physics, Radioactive decay
Abstract: Searches for double beta decay of ^(134)Xe were performed with EXO-200, a single-phase liquid xenon detector designed to search for neutrinoless double beta decay of ^(136)Xe. Using an exposure of 29.6 kg⋅yr, the lower limits of T^(2νββ_+(1/2) > 8.7×10^(20) yr and T^(0νββ)_(1/2) > 1.1×10^(23) yr at 90% confidence level were derived, with corresponding half-life sensitivities of 1.2×10^(21) yr and 1.9×10^(23) yr. These limits exceed those in the literature for ^(134)Xe, improving by factors of nearly 105 and 2 for the two antineutrino and neutrinoless modes, respectively.
Published: 2017
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29. Sensitivity and discovery potential of the proposed nEXO experiment to neutrinoless double beta decay

Author: J. L. Vuilleumier, B. Mong, M. Wagenpfeil, J. Dalmasson, A. Piepke, J. Todd, Y. Y. Ding, M. Heffner, Yuehe Lin, John L. Orrell, E. Raguzin, X.L. Sun, J. B. Zhao, C. T. Overman, R. Krücken, D. Qiu, Z. Li, Giorgio Gratta, A. Burenkov, M. Hasan, Arun Kumar Soma, L. J. Kaufman, R. DeVoe, S. J. Daugherty, Samuele Sangiorgio, M. Hughes, K. S. Kumar, V. Veeraraghavan, Y. Lan, Wei Wei, Petr Vogel, Rejean Fontaine, J. Daughhetee, A. Craycraft, U. Wichoski, Ethan Brown, F. Bourque, M. J. Jewell, M. Coon, D. Harris, Yu-Guang Zhou, T. Ziegler, T. Tolba, G. St-Hilaire, T. Tsang, Qun-Yao Wang, T. Stiegler, M. Chiu, J. P. Brodsky, David Moore, F. Retiere, Y. Ito, J. Zettlemoyer, Douglas H Beck, M. Oriunno, Zhijun Ning, S. Johnston, O. Zeldovich, G. Visser, A. Karelin, J. Hößl, A. Pocar, R. Tsang, T. Didberidze, S. Kravitz, Guofu Cao, T. N. Johnson, J. Schneider, P. Hufschmidt, E. V. Hansen, Y-R Yen, David A. Sinclair, F. Vachon, Ryan Killick, David Leonard, K. Murray, Liang Yang, R. J. Newby, Thomas Koffas, A. Jamil, D. Fudenberg, W. M. Fairbank, Gisela Anton, M. Côté, P. C. Rowson, T. Daniels, K. Graham, G. S. Ortega, B. T. Cleveland, M. J. Dolinski, V.N. Stekhanov, K. Odgers, Angelo Dragone, A. House, S. Rescia, A. Kuchenkov, W. Cree, Jean-Francois Pratte, Veljko Radeka, T. Rossignol, S. Feyzbakhsh, R. Saldanha, S. Delaquis, T. Brunner, W. R. Cen, Serge A. Charlebois, C. Licciardi, G. S. Li, R. Gornea, K. Skarpaas, G. Wrede, I. J. Arnquist, M. Tarka, Wei Wu, X. S. Jiang, A. Der Mesrobian-Kabakian, C. Chambers, A.C. Odian, G. Giacomini, A. Schubert, S. Parent, J. Farine, V. Belov, A. Robinson, L. Cao, F. Nolet, L. J. Wen, Marc Weber, S. X. Wu, Lorenzo Fabris, J. B. Albert, R. MacLellan, Thilo Michel, P. S. Barbeau, Jens Dilling, Xuan Zhang, I. Badhrees, I. Ostrovskiy, O. Njoya, A. Iverson, Shu Li, S. Schmidt, T. Rao, N. Roy, and E. W. Hoppe
Subjects: Physics, Time projection chamber, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, Active medium, Detector, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 7. Clean energy, 3. Good health, Nuclear physics, Homogeneous, 0103 physical sciences, Sensitivity (control systems), Nuclear Experiment (nucl-ex), 010306 general physics, Enriched Xenon Observatory, Nuclear Experiment, Order of magnitude
Abstract: The next-generation Enriched Xenon Observatory (nEXO) is a proposed experiment to search for neutrinoless double beta ($0\nu\beta\beta$) decay in $^{136}$Xe with a target half-life sensitivity of approximately $10^{28}$ years using $5\times10^3$ kg of isotopically enriched liquid-xenon in a time projection chamber. This improvement of two orders of magnitude in sensitivity over current limits is obtained by a significant increase of the $^{136}$Xe mass, the monolithic and homogeneous configuration of the active medium, and the multi-parameter measurements of the interactions enabled by the time projection chamber. The detector concept and anticipated performance are presented based upon demonstrated realizable background rates., Comment: v2 as published
Published: 2017

30. Dark Matter Search Results from the PICO−60 C3F8 Bubble Chamber

Author: T. Nania, M. Laurin, U. Chowdhury, G. Giroux, V. Zacek, Amber M. Ortega, O. Scallon, Eric W. Hoppe, W. H. Lippincott, J. Hall, M. Ardid, D. Baxter, G. Cao, P. Campion, J. Farine, Yongke Yan, I. Stekl, F. Mamedov, Satyajit Seth, A. E. Robinson, Deepam Maurya, A. Roeder, Jie Zhang, F. Tardif, P. S. Cooper, C. B. Krauss, S. Olson, Shashank Priya, H. Borsodi, F. Girard, C. E. Dahl, Ilan Levine, E. Vázquez-Jáuregui, J. I. Collar, R. Podviyanuk, O. Harris, J. Wells, R. Rucinski, Ivan Felis, R. Filgas, Manuel Bou-Cabo, G. Crowder, R. Neilson, C. Amole, N. Starinski, M. Jin, Karl J. Clark, Chujie Chen, I. Lawson, A. J. Noble, S. Fallows, A. Plante, D. M. Asner, Mala Das, Pijushpani Bhattacharjee, M. B. Crisler, I. J. Arnquist, U. Wichoski, P. Mitra, A. Sonnenschein, A. Leblanc, and E. Behnke
Subjects: 010308 nuclear & particles physics, Endowment, Atomic energy, 0103 physical sciences, General Physics and Astronomy, Library science, Christian ministry, 010306 general physics, National laboratory, Student research, 01 natural sciences, Mine site, Underground space
Abstract: The PICO Collaboration wishes to thank SNOLAB and its staff for support through underground space, logistical, and technical services. SNOLAB operations are supported by the Canada Foundation for Innovation and the Province of Ontario Ministry of Research and Innovation, with underground access provided by Vale at the Creighton mine site. We are grateful to Kristian Hahn and Stanislava Sevova of Northwestern University and Bjorn Penning of the University of Bristol for their assistance and useful discussion. We wish to acknowledge the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) and the Canada Foundation for Innovation (CFI) for funding. We acknowledge the support from National Science Foundation (NSF) (Grants No. 0919526, No. 1506337, No. 1242637, and No. 1205987). We acknowledge that this work is supported by the U.S. Department of Energy (DOE) Office of Science, Office of High Energy Physics (under Award No. DE-SC-0012161), by a DOE Office of Science Graduate Student Research (SCGSR) award, by Direccion General Asuntos del Personal Academico, Universidad Nacional Autonoma de Mexico (DGAPA-UNAM) through the grant Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPIIT) No. IA100316 and by Consejo Nacional de Ciencia y Tecnologia (CONACyT) (Mexico) through Grant No. 252167, by the Department of Atomic Energy (DAE), the Government of India, under the Center of AstroParticle Physics II project (CAPP-II) at Saha Institute of Nuclear Physics (SINP), by the Czech Ministry of Education, Youth and Sports (Grant No. LM2015072), and by the Spanish Ministerio de Economia y Competitividad, Consolider MultiDark (Grant No. CSD2009-00064). This work is partially supported by the Kavli Institute for Cosmological Physics at the University of Chicago through NSF Grant No. 1125897, and an endowment from the Kavli Foundation and its founder Fred Kavli. We also wish to acknowledge the support from Fermi National Accelerator Laboratory under Contract No. De-AC02-07CH11359, and Pacific Northwest National Laboratory, which is operated by Battelle for the U.S. Department of Energy under Contract No. DE-AC05-76RL01830. We also thank Compute Canada and the Center for Advanced Computing, ACENET, Calcul Quebec, Compute Ontario, and WestGrid for the computational support.
Published: 2017
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31. Search for Neutrinoless Double-Beta Decay with the Upgraded EXO-200 Detector

Author: M. Wagenpfeil, S. Feyzbakhsh, S. Johnston, Martin Breidenbach, M. Coon, P. Fierlinger, Liangjian Wen, S. J. Daugherty, Guofu Cao, K. Graham, C. Licciardi, S. Kravitz, O. Ya. Zeldovich, R. Bayerlein, A. Piepke, R. H. Nelson, A. Schubert, U. Wichoski, Marc Weber, B. T. Cleveland, E. V. Hansen, B. Mong, P. C. Rowson, Giorgio Gratta, A. Kuchenkov, T. Ziegler, P. S. Barbeau, W. Cree, J. Davis, R. Krücken, S. Delaquis, K. Murray, David Leonard, R. Tsang, M. J. Jewell, A. Karelin, V. A. Belov, Gisela Anton, Liang Yang, A. Jamil, J. J. Russell, J. Farine, J. B. Albert, T. Walton, Thomas Koffas, W. M. Fairbank, M. Danilov, W. R. Cen, R. Gornea, J. Hoessl, Y. Lan, P. Hufschmidt, R. DeVoe, L. J. Kaufman, Douglas H Beck, J. Zettlemoyer, David A. Sinclair, Y-R Yen, J. Daughhetee, Yuehe Lin, C. Chambers, J. L. Vuilleumier, C. R. Hall, R. MacLellan, K. S. Kumar, A. Craycraft, T. Tolba, Thilo Michel, T. Brunner, A. S. Johnson, A. Dolgolenko, V.N. Stekhanov, A. Pocar, D. Fudenberg, M. Hughes, A. P. Waite, David Moore, T. Didberidze, Petr Vogel, F. Retiere, G. S. Li, M. J. Dolinski, A. Der Mesrobian-Kabakian, I. Ostrovskiy, O. Njoya, Shu Li, S. Schmidt, Jens Dilling, I. Badhrees, A. Odian, Gerrit Wrede, M. Tarka, and T. Daniels
Subjects: Cryostat, Physics, Particle physics, 010308 nuclear & particles physics, Detector, General Physics and Astronomy, chemistry.chemical_element, FOS: Physical sciences, Radon, 01 natural sciences, Confidence interval, High Energy Physics - Experiment, ddc, Nuclear physics, Lead shielding, High Energy Physics - Experiment (hep-ex), Upgrade, chemistry, Double beta decay, 0103 physical sciences, Nuclear astrophysics, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment
Abstract: Results from a search for neutrinoless double-beta decay $0\nu\beta\beta$ of $^{136}$Xe are presented using the first year of data taken with the upgraded EXO-200 detector. Relative to previous searches by EXO-200, the energy resolution of the detector has been improved to $\sigma/E$=1.23%, the electric field in the drift region has been raised by 50%, and a system to suppress radon in the volume between the cryostat and lead shielding has been implemented. In addition, analysis techniques that improve topological discrimination between $0\nu\beta\beta$ and background events have been developed. Incorporating these hardware and analysis improvements, the median 90% confidence level $0\nu\beta\beta$ half-life sensitivity after combining with the full data set acquired before the upgrade has increased 2-fold to $3.7 \times 10^{25}$ yr. No statistically significant evidence for $0\nu\beta\beta$ is observed, leading to a lower limit on the $0\nu\beta\beta$ half-life of $1.8\times10^{25}$ yr at the 90% confidence level., Comment: 6 pages, 4 figures, final version submitted to PRL
Published: 2017
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32. Dark Matter Search Results from the PICO-60 C$_3$F$_8$ Bubble Chamber

Author: C, Amole, M, Ardid, I J, Arnquist, D M, Asner, D, Baxter, E, Behnke, P, Bhattacharjee, H, Borsodi, M, Bou-Cabo, P, Campion, G, Cao, C J, Chen, U, Chowdhury, K, Clark, J I, Collar, P S, Cooper, M, Crisler, G, Crowder, C E, Dahl, M, Das, S, Fallows, J, Farine, I, Felis, R, Filgas, F, Girard, G, Giroux, J, Hall, O, Harris, E W, Hoppe, M, Jin, C B, Krauss, M, Laurin, I, Lawson, A, Leblanc, I, Levine, W H, Lippincott, F, Mamedov, D, Maurya, P, Mitra, T, Nania, R, Neilson, A J, Noble, S, Olson, A, Ortega, A, Plante, R, Podviyanuk, S, Priya, A E, Robinson, A, Roeder, R, Rucinski, O, Scallon, S, Seth, A, Sonnenschein, N, Starinski, I, Štekl, F, Tardif, E, Vázquez-Jáuregui, J, Wells, U, Wichoski, Y, Yan, V, Zacek, and J, Zhang
Subjects: High Energy Physics - Experiment (hep-ex), Physics - Instrumentation and Detectors, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics::Instrumentation and Detectors, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Experiment
Abstract: New results are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 52 kg of C$_3$F$_8$ located in the SNOLAB underground laboratory. As in previous PICO bubble chambers, PICO-60 C$_3$F$_8$ exhibits excellent electron recoil and alpha decay rejection, and the observed multiple-scattering neutron rate indicates a single-scatter neutron background of less than 1 event per month. A blind analysis of an efficiency-corrected 1167-kg-day exposure at a 3.3-keV thermodynamic threshold reveals no single-scattering nuclear recoil candidates, consistent with the predicted background. These results set the most stringent direct-detection constraint to date on the WIMP-proton spin-dependent cross section at 3.4 $\times$ 10$^{-41}$ cm$^2$ for a 30-GeV$\thinspace$c$^{-2}$ WIMP, more than one order of magnitude improvement from previous PICO results., Comment: 6 pages, 6 figures
Published: 2017
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33. Characterization of an Ionization Readout Tile for nEXO

Author: T. Stiegler, Douglas H Beck, R. Tsang, K. Murray, Gisela Anton, D. Fudenberg, R. Saldanha, Angelo Dragone, J. Todd, Y. Y. Ding, R. Krücken, Jochen M. Schneider, Y-R Yen, Jean-Francois Pratte, P. C. Rowson, K. Skarpaas, S. Kravitz, E. V. Hansen, Liang Yang, S. Feyzbakhsh, A. House, V. Veeraraghavan, R. J. Newby, A. Jamil, Ethan Brown, M. Chiu, W. Cree, A. Burenkov, S. Delaquis, M. Hughes, M. Côté, T. Daniels, Gabriele Giacomini, A. Pocar, Maulik R. Patel, M. Hasan, J. Farine, A. Karelin, R. DeVoe, Jens Dilling, Arun Kumar Soma, Zhijun Ning, T. Tolba, M. J. Jewell, I. Badhrees, David Moore, A. Robinson, T. Didberidze, B. Mong, M. Wagenpfeil, J. Dalmasson, I. J. Arnquist, Xiaoshan Jiang, Yuehe Lin, Veljko Radeka, A. Piepke, Gerrit Wrede, V.N. Stekhanov, J. B. Zhao, S. Parent, U. Wichoski, M. Oriunno, W. R. Cen, C. Chambers, R. Gornea, M. Heffner, A. Odian, D. Qiu, M. Tarka, S. Johnston, T. Ziegler, I. Ostrovskiy, John L. Orrell, E. Raguzin, Z. Li, T. Brunner, S. Rescia, S. X. Wu, Eric W. Hoppe, M. Coon, S. J. Daugherty, A. Schubert, O. Zeldovich, Cory T. Overman, G. Visser, Wei Wu, O. Njoya, A. Iverson, Triveni Rao, Y. Lan, Thomas Tsang, Shu Li, S. Schmidt, J. Daughhetee, Qian Wang, David Leonard, G. S. Ortega, Thomas Koffas, W. M. Fairbank, Samuele Sangiorgio, Giorgio Gratta, J. L. Vuilleumier, B. T. Cleveland, K. Odgers, Serge A. Charlebois, R. MacLellan, Yumei Zhou, Wei Wei, K. S. Kumar, Rejean Fontaine, A. Kuchenkov, P. Hufschmidt, David A. Sinclair, F. Bourque, J. P. Brodsky, G. St-Hilaire, D. Harris, Y. Ito, L. J. Kaufman, M. J. Dolinski, A. Craycraft, Liangjian Wen, Guofu Cao, G. S. Li, Thilo Michel, T. Rossignol, Xiaoyang Sun, C. Licciardi, A. Der Mesrobian-Kabakian, N. Roy, L. Cao, F. Nolet, F. Vachon, Marc Weber, F. Retière, J. B. Albert, X. Zhang, J. Hößl, P. S. Barbeau, V. A. Belov, and Lorenzo Fabris
Subjects: Physics - Instrumentation and Detectors, Materials science, Physics::Instrumentation and Detectors, chemistry.chemical_element, FOS: Physical sciences, STRIPS, 01 natural sciences, law.invention, Optics, Xenon, law, Ionization, 0103 physical sciences, Wafer, 010306 general physics, Instrumentation, Mathematical Physics, Time projection chamber, 010308 nuclear & particles physics, business.industry, Detector, Instrumentation and Detectors (physics.ins-det), Anode, chemistry, visual_art, visual_art.visual_art_medium, Tile, business
Abstract: A new design for the anode of a time projection chamber, consisting of a charge-detecting "tile", is investigated for use in large scale liquid xenon detectors. The tile is produced by depositing 60 orthogonal metal charge-collecting strips, 3~mm wide, on a 10~\si{\cm} $\times$ 10~\si{\cm} fused-silica wafer. These charge tiles may be employed by large detectors, such as the proposed tonne-scale nEXO experiment to search for neutrinoless double-beta decay. Modular by design, an array of tiles can cover a sizable area. The width of each strip is small compared to the size of the tile, so a Frisch grid is not required. A grid-less, tiled anode design is beneficial for an experiment such as nEXO, where a wire tensioning support structure and Frisch grid might contribute radioactive backgrounds and would have to be designed to accommodate cycling to cryogenic temperatures. The segmented anode also reduces some degeneracies in signal reconstruction that arise in large-area crossed-wire time projection chambers. A prototype tile was tested in a cell containing liquid xenon. Very good agreement is achieved between the measured ionization spectrum of a $^{207}$Bi source and simulations that include the microphysics of recombination in xenon and a detailed modeling of the electrostatic field of the detector. An energy resolution $\sigma/E$=5.5\% is observed at 570~\si{keV}, comparable to the best intrinsic ionization-only resolution reported in literature for liquid xenon at 936~V/\si{cm}., Comment: 18 pages, 13 figures, as published
Published: 2017
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34. First results from EXO-200

Author: J. Farine
Subjects: Physics, Nuclear physics, Nuclear and High Energy Physics, MAJORANA, Matrix element, Atomic and Molecular Physics, and Optics, Lower limit
Abstract: We report on a search for neutrinoless double-beta decay of 136 Xe with EXO-200. No signal is observed for a 136 Xe exposure of 26.3 kg-yr, with a background of ∼ 1.5 × 10 − 3 kg ( e n r LXe ) − 1 yr − 1 keV − 1 in the ± 1 σ region of interest. This sets a lower limit on the half-life of the neutrinoless double-beta decay T 1 / 2 0 ν β β ( 136 Xe ) > 1.6 × 10 25 yr (90% CL) , corresponding to effective Majorana masses of less than 140–380 meV, depending on the matrix element calculation.
Published: 2013
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35. Measurement of radium concentration in water with Mn-coated beads at the Sudbury Neutrino Observatory

Author: T.C. Andersen, I. Blevis, J. Boger, E. Bonvin, M. Chen, B.T. Cleveland, X. Dai, F. Dalnoki-Veress, G. Doucas, J. Farine, H. Fergani, A.P. Ferraris, M.M. Fowler, R.L. Hahn, E.D. Hallman, C.K. Hargrove, P. Jagam, N.A. Jelley, A.B. Knox, H.W. Lee, I. Levine, S. Majerus, K. McFarlane, C. Mifflin, G.G. Miller, A.J. Noble, P. Palmer, J.K. Rowley, M. Shatkay, J.J. Simpson, D. Sinclair, J.-X. Wang, J.B. Wilhelmy, and M. Yeh
Subjects: Detection limit, Physics, Heavy water, Nuclear and High Energy Physics, Sudbury Neutrino Observatory, 010308 nuclear & particles physics, Solar neutrino, Counting efficiency, Analytical chemistry, FOS: Physical sciences, chemistry.chemical_element, 01 natural sciences, Ion, Radium, chemistry.chemical_compound, Adsorption, chemistry, 0103 physical sciences, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Instrumentation
Abstract: We describe a method to measure the concentration of 224Ra and 226Ra in the heavy water target used to detect solar neutrinos at the Sudbury Neutrino Observatory and in the surrounding light water shielding. A water volume of (50-400) m^3 from the detector is passed through columns which contain beads coated with a compound of manganese oxide onto which the Ra dissolved in the water is adsorbed. The columns are removed, dried, and mounted below an electrostatic chamber into which the Rn from the decay of trapped Ra is continuously flowed by a stream of nitrogen gas. The subsequent decay of Rn gives charged Po ions which are swept by the electric field onto a solid-state alpha counter. The content of Ra in the water is inferred from the measured decay rates of 212Po, 214Po, 216Po, and 218Po. The Ra extraction efficiency is >95%, the counting efficiency is 24% for 214Po and 6% for 216Po, and the method can detect a few atoms of 224Ra per m^3 and a few tens of thousands of atoms of 226Ra per m^3. Converted to equivalent equilibrium values of the topmost elements of the natural radioactive chains, the detection limit in a single assay is a few times 10^(-16) g Th or U/cm^3. The results of some typical assays are presented and the contributions to the systematic error are discussed., 25 pages, 8 figures. V2 shortened to 17 pages, 5 figures
Published: 2016
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36. Neutral current and day night measurements from the pure D2O phase of SNO

Author: B. C. Robertson, J. R. Leslie, M. Dunford, Eric B. Norman, J. B. Wilhelmy, T. Kutter, J. Manor, J. Farine, S. D. Biller, C. W. Nally, T. V. Bullard, A. S. Hamer, D. R. Grant, Guthrie Miller, S. J. Brice, James R. Wilson, E. W. Beier, P. J. Harvey, J. Cameron, C. E. Okada, J. F. Wilkerson, E. D. Hallman, X. Chen, W. J. Heintzelman, S. R. Elliott, R. G. Stokstad, David A. Sinclair, J. A. Formaggio, P. Jagam, Reda Tafirout, Christopher C. M. Kyba, M. W. Smith, C. J. Virtue, Ilan Levine, H. B. Mak, R. G. Van de Water, N. Starinsky, G. Doucas, P. Skensved, G. T. Ewan, K. K. Schaffer, G. A. Cox, K. Kazkaz, M. M. Fowler, F. Dalnoki-Veress, M. G. Bowler, C. K. Hargrove, K. Graham, S. M. Oser, P. T. Keener, S. S.E. Rosendahl, S. Majerus, John L. Orrell, Hal Evans, W. Frati, S. Luoma, B. T. Cleveland, W. B. Handler, D. L. Wark, K. T. Lesko, N. Tagg, E. D. Earle, N. Gagnon, Y.D. Chan, K. M. Heeger, A. Hime, Mark Guy Boulay, X. Dai, J. J. Simpson, R. L. Hahn, R. Hazama, Minfang Yeh, J. A. Dunmore, N. A. Jelley, K. Frame, A. L. Hallin, M. Howe, J. M. Wouters, Peter Wittich, A. B. McDonald, N. McCauley, A. D. Marino, R. Van Berg, H. Fergani, M. L. Chen, I. Lawson, A. J. Noble, Jochen Klein, V. L. Rusu, J. Maneira, A. W. P. Poon, F. A. Duncan, R. G. H. Robertson, M. R. Dragowsky, T. Spreitzer, T.J. Bowles, G. McGregor, Chris Waltham, L. C. Stonehill, R. L. Helmer, M. H. Schwendener, J. Law, C. J. Sims, J. Heise, C. A. Duba, N. West, and P. J. Doe
Subjects: Physics, Elastic scattering, Nuclear and High Energy Physics, Sudbury Neutrino Observatory, Solar neutrino, Atomic and Molecular Physics, and Optics, Massless particle, Nuclear physics, Neutrino detector, High Energy Physics::Experiment, Astrophysics::Earth and Planetary Astrophysics, Neutrino, Nuclear Experiment, Charged current, Lepton
Abstract: The Sudbury Neutrino Observatory is a 1000 T D 2 O Cerenkov detector that is sensitive to 8 B solar neutrinos. The energy, radius, and direction with respect to the sun is measured for each neutrino event; these distributions are used to separately determine the rates of the charged current, neutral current and electron scattering reactions of neutrinos on deuterium. Assuming an undistorted 8 B spectrum, the ν e component of the 8 B solar flux is φ e = 1.76 +0.05 −0.05 (stat.) +0.09 −0.09 (syst.) × 10 6 cm −2 s −1 based on events with a measured kinetic enegy above 5 MeV. The non- ν e component is φ μτ = 3.41 +0.45 −0.45 (stat.) +0.48 −0.45 (syst.) × 10 6 cm −2 s −1 , 5.3 σ greater than zero, providing strong evidence for solar ν e flavor transformation. The total flux measured with the NC reaction is φ NC = 5.09 +0.044 −0.43 (stat.) +0.46 −0.43 (syst.) × 10 6 cm −2 s −1 , consistent with solar models. The night minus day rate is 14.0% ± 6.3% +1.5 −1.4 % of the average rate. If the total flux of active neutrinos is additionally constrained to have no asymmetry, the ν e asymmetry is found to be 7.0% ± 4.9% +1.3 −1.2 %. A global solar neutrino analysis is terms of matter-enhanced oscillations of two active flavors strongly favors the Large Mixing Angle (LMA) solution.
Published: 2016
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37. The calibration of the Sudbury Neutrino Observatory using uniformly distributed radioactive sources

Author: I. T. Lawson, Joshua R. Klein, K. J. Keeter, A. L. Hallin, R. Ford, E. Guillian, C. B. Krauss, M. J. Thomson, Keith Rielage, B. T. Cleveland, R. G. H. Robertson, P. Skensved, V. l. Rusu, J. C. Loach, Bei Cai, N. A. Jelley, K. Boudjemline, H. M. O'Keeffe, C. Howard, J. Farine, E. D. Hallman, A. J. Noble, P. Jagam, S. D. Reitzner, S. J. M. Peeters, C. Kraus, Alan Poon, R. Lange, Hal Evans, G. T. Ewan, G. McGregor, A. B. McDonald, and S. R. Seibert
Subjects: Physics, Nuclear and High Energy Physics, Sudbury Neutrino Observatory, 010308 nuclear & particles physics, Solar neutrino, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Proportional counter, FOS: Physical sciences, 01 natural sciences, Nuclear physics, Neutrino detector, 13. Climate action, 0103 physical sciences, Neutron detection, Neutron, Neutrino, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Instrumentation, Cherenkov radiation
Abstract: The production and analysis of distributed sources of 24Na and 222Rn in the Sudbury Neutrino Observatory (SNO) are described. These unique sources provided accurate calibrations of the response to neutrons, produced through photodisintegration of the deuterons in the heavy water target, and to low energy betas and gammas. The application of these sources in determining the neutron detection efficiency and response of the 3He proportional counter array, and the characteristics of background Cherenkov light from trace amounts of natural radioactivity is described., Comment: 24 pages, 13 figures
Published: 2016
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38. Constraints on nucleon decay via invisible modes from the Sudbury Neutrino Observatory

Author: X. Chen, H. Wan Chan Tseung, H. Labranche, D. L. Wark, F. Dalnoki-Veress, A. D. Marino, B. C. Robertson, N. McCauley, R. L. Helmer, G. Doucas, R. Van Berg, R. G. H. Robertson, J. B. Wilhelmy, T. Kutter, M. G. Bowler, I. Levine, M. L. Chen, Monica Dunford, S. S.E. Rosendahl, Chris Waltham, C. J. Virtue, S. J. Brice, A. W. P. Poon, J. A. Dunmore, R. L. Hahn, R. W. Ollerhead, C. W. Nally, G. McGregor, P. Jagam, K.K.S. Miknaitis, J. M. Wouters, S. Majerus, P. Skensved, X. Dai, J. F. Wilkerson, R. G. Van de Water, Joshua R. Klein, N. Gagnon, Reda Tafirout, N. Starinsky, Darren Grant, Alain Bellerive, R. S. Dosanjh, R. Lange, Mark Neubauer, W. Frati, S. N. Ahmed, R. Hazama, E. D. Earle, E. Rollin, W. B. Handler, H. B. Mak, T. J. Bowles, Andrew Hime, J. R. Wilson, Guthrie Miller, M. W.E. Smith, F. A. Duncan, M. A. Howe, A. B. McDonald, Christopher C. M. Kyba, R. MacLellan, M. A. Thomson, J. Heise, S. D. Biller, J. R. Leslie, B. A. Moffat, Bernie G. Nickel, J. Boger, F. Fleurot, M. H. Schwendener, B. T. Cleveland, Malcolm M. Fowler, N. S. Oblath, A. E. Anthony, N. West, A. V. Krumins, C. A. Duba, S. Luoma, Joseph A. Formaggio, C. Ouellet, Minfang Yeh, C. E. Okada, P. J. Harvey, W. J. Heintzelman, S. R. Elliott, O. Simard, David A. Sinclair, G. T. Ewan, I. T. Lawson, G. Tešić, A. L. Hallin, C. Mifflin, S. J. M. Peeters, N. A. Jelley, M. Thorman, D. Waller, V. L. Rusu, J. C. Hall, J. Law, M. R. Dragowsky, G. A. Cox, K. T. Lesko, L. C. Stonehill, J. Farine, C. J. Sims, C. K. Hargrove, A. J. Noble, T. V. Bullard, R. J. Hemingway, Kai Zuber, H. Fergani, J. Maneira, M. Kos, A. S. Hamer, Hal Evans, E. W. Beier, S. McGee, R. G. Stokstad, B. L. Wall, Peter Wittich, Eric B. Norman, E. D. Hallman, P. J. Doe, Y. Takeuchi, J. J. Simpson, Yuen-Dat Chan, K. Graham, S. M. Oser, M.G. Boulay, B. G. Fulsom, K. Frame, K. M. Heeger, and John L. Orrell
Subjects: Physics, Sudbury Neutrino Observatory, Particle physics, Proton, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Gamma ray, FOS: Physical sciences, General Physics and Astronomy, Elementary particle, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, Baryon, High Energy Physics - Experiment (hep-ex), Particle decay, 0103 physical sciences, Neutron, High Energy Physics::Experiment, 010306 general physics, Nucleon, Nuclear Experiment
Abstract: Data from the Sudbury Neutrino Observatory have been used to constrain the lifetime for nucleon decay to ``invisible'' modes, such as n -> 3 nu. The analysis was based on a search for gamma-rays from the de-excitation of the residual nucleus that would result from the disappearance of either a proton or neutron from O16. A limit of tau_inv > 2 x 10^{29} years is obtained at 90% confidence for either neutron or proton decay modes. This is about an order of magnitude more stringent than previous constraints on invisible proton decay modes and 400 times more stringent than similar neutron modes., Update includes missing efficiency factor (limits change by factor of 2) Submitted to Physical Review Letters
Published: 2016
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39. SEARCHES FOR HIGH-FREQUENCY VARIATIONS IN THE B-8 SOLAR NEUTRINO FLUX AT THE SUDBURY NEUTRINO OBSERVATORY

Author: E. D. Hallman, G. Prior, Benjamin Monreal, E. D. Earle, P. J. Doe, S. J. M. Peeters, K. J. Keeter, T. Tsui, F. A. Duncan, P. Skensved, M. DiMarco, K. Boudjemline, Yuen-Dat Chan, J. M. Wouters, J. Heise, S. Habib, K. Graham, X. Dai, S. M. Oser, J. A. Detwiler, Keith Rielage, H. Wan Chan Tseung, M. L. Miller, A. B. McDonald, R. D. Martin, Andrew Hime, I. Levine, Jocelyn Monroe, Alain Bellerive, D. L. Wark, R. J. Ford, T. J. Sonley, R. L. Hahn, H. Fergani, R. G. H. Robertson, M. H. Schwendener, R. MacLellan, Monica Dunford, J. Maneira, B. Beltran, Mark Guy Boulay, Bei Cai, David A. Sinclair, C. A. Duba, F. Zhang, J. Law, D. Chauhan, Peter Watson, B. Jamieson, A. W. P. Poon, Christopher C. M. Kyba, P.-L. Drouin, N. Tolich, C. B. Krauss, N. S. Oblath, B. Aharmim, T.H. Burritt, Kai Zuber, C. D. Tunnell, A. L. Hallin, R. L. Helmer, B. Morissette, J. A. Secrest, I. T. Lawson, C. Kraus, B. T. Cleveland, S. R. Seibert, D. Waller, G. A. Cox, R. A. Ott, N. West, W. J. Heintzelman, K. T. Lesko, J. R. Wilson, M. Kos, A. Wright, O. Simard, E. W. Beier, B.A. VanDevender, L. C. Stonehill, C. Howard, J. Farine, A. J. Noble, C. J. Virtue, B. C. Robertson, G. Doucas, E. Guillian, T. Kutter, N. Barros, Joseph A. Formaggio, Minfang Yeh, J. C. Loach, N. A. Jelley, Hal Evans, S. D. Reitzner, S. N. Ahmed, Joshua R. Klein, M. Bergevin, N. McCauley, R. Van Berg, M. L. Chen, S. Majerus, L. L. Kormos, G. T. Ewan, N. Gagnon, R. Hazama, G. D. Orebi Gann, H. Deng, B. L. Wall, H. M. O'Keeffe, H. B. Mak, S. McGee, S. D. Biller, Bernie G. Nickel, P. J. Harvey, J. F. Wilkerson, Steven Elliott, M. A. Howe, M. Huang, G. Tešić, J. R. Leslie, F. Fleurot, A. E. Anthony, and J. Tm. Goon
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Solar neutrino, FOS: Physical sciences, Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Observatory, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Nuclear Experiment (nucl-ex), 010303 astronomy & astrophysics, Nuclear Experiment, Solar and Stellar Astrophysics (astro-ph.SR), Physics, Sudbury Neutrino Observatory, Solar observatory, 010308 nuclear & particles physics, Astronomy, Astronomy and Astrophysics, Solar neutrino problem, Neutrino detector, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, Physics::Space Physics, Measurements of neutrino speed, Neutrino
Abstract: We have performed three searches for high-frequency signals in the solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO), motivated by the possibility that solar $g$-mode oscillations could affect the production or propagation of solar $^8$B neutrinos. The first search looked for any significant peak in the frequency range 1/day to 144/day, with a sensitivity to sinusoidal signals with amplitudes of 12% or greater. The second search focused on regions in which $g$-mode signals have been claimed by experiments aboard the SoHO satellite, and was sensitive to signals with amplitudes of 10% or greater. The third search looked for extra power across the entire frequency band. No statistically significant signal was detected in any of the three searches., 37 pages, 17 figures, submitted to ApJ
Published: 2016
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40. Study of silicon photomultiplier performance in external electric fields

Author: A. Alamre, T. Stiegler, John L. Orrell, T. Daniels, M. Côté, J. Schneider, Z. Li, N. Roy, L. Cao, F. Nolet, M. Oriunno, M. Hughes, Ethan Brown, J. Farine, D. Fairbank, D. Qiu, Y. Ito, M. Coon, Thilo Michel, Qing Xia, V.N. Stekhanov, C. T. Overman, M. Chiu, G. S. Ortega, A. Karelin, A. Pocar, D. S. Leonard, T. Tolba, Venkatesh Veeraraghavan, J. Hößl, Marc Weber, S. Kravitz, Yuehe Lin, David Moore, Y. Lan, R. DeVoe, Serge A. Charlebois, K. Murray, A. Craycraft, J. Echevers, Gisela Anton, M. Wagenpfeil, J. Dalmasson, T. Brunner, E. Raguzin, O. Nusair, Jens Dilling, R. Krücken, Z. Ning, Samuele Sangiorgio, Wei Wei, K. S. Kumar, S. X. Wu, Gerard Visser, P. S. Barbeau, D. A. Harris, A. Der Mesrobian-Kabakian, J. B. Zhao, A. Larson, D. Fudenberg, O. Zeldovich, A. Piepke, I. Badhrees, Angelo Dragone, M. J. Jewell, F. Vachon, Rejean Fontaine, Jean-Francois Pratte, R. Saldanha, L. Darroch, D. Kodroff, B. Veenstra, F. Bourque, S. Parent, S. Rescia, Lorenzo Fabris, T. Bhatta, A. Odian, S. J. Daugherty, J. Watkins, I. Ostrovskiy, R. MacLellan, G. Giacomini, J. P. Brodsky, T. I. Totev, Stefan Schmidt, R. Tsang, O. Njoya, A. Iverson, Triveni Rao, K. Skarpaas Viii, T. Rossignol, G. Wrede, B. Mong, Thomas Tsang, Shu Li, P. Fierlinger, W. R. Cen, Liangjian Wen, Guofu Cao, L. J. Kaufman, A. E. Robinson, M. Tarka, J. B. Albert, Qian Wang, G. Li, S. Feyzbakhsh, Giorgio Gratta, Yumei Zhou, M. J. Dolinski, P. Hufschmidt, David A. Sinclair, B. T. Cleveland, K. Odgers, A. Kuchenkov, U. Wichoski, G. St-Hilaire, C. Licciardi, V. Radeka, T. Ziegler, Thomas Koffas, W. M. Fairbank, Xilei Sun, I. J. Arnquist, Wei Wu, R.J. Newby, P. C. Rowson, A. House, W. Cree, S. Delaquis, Xiaoshan Jiang, C. Chambers, G. Gallina, P. Lv, J. Todd, Y. Y. Ding, E. V. Hansen, Liang Yang, A. Jamil, Douglas H Beck, A. Burenkov, Y-R Yen, J. L. Vuilleumier, Arun Kumar Soma, C. Jessiman, M. K. Moe, Eric W. Hoppe, M. Heffner, J. Daughhetee, R. Gornea, F. Retière, and V. A. Belov
Subjects: 010302 applied physics, Physics - Instrumentation and Detectors, Materials science, 010308 nuclear & particles physics, business.industry, FOS: Physical sciences, Observable, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 7. Clean energy, Silicon photomultiplier, Electric field, 0103 physical sciences, Optoelectronics, business, Instrumentation, Photon detection, Mathematical Physics
Abstract: We report on the performance of silicon photomultiplier (SiPM) light sensors operating in electric field strength up to 30 kV/cm and at a temperature of 149K, relative to their performance in the absence of an external electric field. The SiPM devices used in this study show stable gain, photon detection efficiency, and rates of correlated pulses, when exposed to external fields, within the estimated uncertainties. No observable physical damage to the bulk or surface of the devices was caused by the exposure., Comment: 16 pages, 12 figures, 2 tables and two conferences (INPC2016 and TIPP2017)
Published: 2018
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41. Dark matter spin-dependent limits for WIMP interactions on 19F by PICASSO

Author: R. Gornea, M. Auger, I. Stekl, T. Shepherd, I. Levine, M. H. Genest, S. Kumaratunga, G. Giroux, Stanislav Pospisil, B. Beltran, Karl J. Clark, Claude Leroy, L. Lessard, F. Aubin, C. B. Krauss, P. Nadeau, A. Davour, U. Wichoski, C. Storey, C. Levy, E. Behnke, J. Farine, M.-C. Piro, A. J. Noble, S. Archambault, V. Zacek, N. Starinski, J. P. Martin, R. MacDonald, X. Dai, I. Lawson, and R. Faust
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Hadron, Dark matter, FOS: Physical sciences, Elementary particle, 01 natural sciences, High Energy Physics - Experiment, Nuclear physics, Baryon, High Energy Physics - Experiment (hep-ex), WIMP, 0103 physical sciences, Neutralino, Neutron, 010306 general physics, Nucleon
Abstract: The PICASSO experiment at SNOLAB reports new results for spin-dependent WIMP interactions on $^{19}$F using the superheated droplet technique. A new generation of detectors and new features which enable background discrimination via the rejection of non-particle induced events are described. First results are presented for a subset of two detectors with target masses of $^{19}$F of 65 g and 69 g respectively and a total exposure of 13.75 $\pm$ 0.48 kgd. No dark matter signal was found and for WIMP masses around 24 GeV/c$^2$ new limits have been obtained on the spin-dependent cross section on $^{19}$F of $\sigma_F$ = 13.9 pb (90% C.L.) which can be converted into cross section limits on protons and neutrons of $\sigma_p$ = 0.16 pb and $\sigma_n$ = 2.60 pb respectively (90% C.L). The obtained limits on protons restrict recent interpretations of the DAMA/LIBRA annual modulations in terms of spin-dependent interactions., Comment: Revised version, accepted for publication in Phys. Lett. B, 20 pages, 7 figures
Published: 2009
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42. Systematic study of trace radioactive impurities in candidate construction materials for EXO-200

Author: David A. Sinclair, Giorgio Gratta, A. Burenkov, J. Wodin, K. O'Sullivan, C. R. Hall, D. Schenker, A. Piepke, J. Hodgson, J. Farine, E. Baussan, M. Danilov, D. Akimov, K. Hall, M. P. Green, P. C. Rowson, Z. Djurcic, Patricia Grinberg, A. G. Kovalenko, David Leonard, Alain Bellerive, W. M. Fairbank, M. Montero Díez, R. Herbst, I. Ekchtout, J. M. Vuilleumier, G. Smirnov, F. LePort, K. Wamba, Shimon Kolkowitz, L. Ounalli, K. Skarpaas, P. Weber, Shie-Chang Jeng, D. Kovalenko, B. Flatt, D. Mackay, R. DeVoe, D. Hallman, M. Bowcock, G. Keefer, W. Craddock, C. K. Hargrove, V.N. Stekhanov, A. Pocar, A. Odian, M. K. Moe, J.-L. Vuilleumier, R. Neilson, M. S. Dixit, P. Fierlinger, V. Strickland, C. J. Virtue, Martin Breidenbach, C. Y. Prescott, R. Conley, and A. Dolgolenko
Subjects: Physics, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Trace (linear algebra), Trace Amounts, fungi, Radiochemistry, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Mass spectrometry, Nuclear physics, Impurity, Double beta decay, Trace analysis, Nuclear Experiment (nucl-ex), Neutron activation analysis, Nuclear Experiment, Instrumentation, Enriched Xenon Observatory
Abstract: The Enriched Xenon Observatory (EXO) will search for double beta decays of 136Xe. We report the results of a systematic study of trace concentrations of radioactive impurities in a wide range of raw materials and finished parts considered for use in the construction of EXO-200, the first stage of the EXO experimental program. Analysis techniques employed, and described here, include direct gamma counting, alpha counting, neutron activation analysis, and high-sensitivity mass spectrometry., Comment: 32 pages, 6 figures. Expanded introduction, added missing table entry. Accepted for publication in Nucl. Instrum. Meth. A
Published: 2008
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43. Improved dark matter search results from PICO-2L Run 2

Author: J. Farine, A. J. Noble, M. Laurin, M. Ruschman, V. Zacek, W. H. Lippincott, J. Hall, Jie Zhang, C. B. Krauss, F. Girard, Deepam Maurya, J. Wells, J. I. Collar, C. M. Jackson, K. Clark, D. Baxter, I. Levine, M. Jin, A. E. Robinson, Eric W. Hoppe, R. B. Podviianiuk, Daniel Broemmelsiek, A. Leblanc, C. Amole, F. Debris, S. J. Brice, G. Giroux, Miguel Ardid, S. Fallows, R. Neilson, I. Lawson, E. Mann, H. Borsodi, M. B. Crisler, I. J. Arnquist, U. Wichoski, S. Olson, D. M. Asner, O. Scallon, Pijushpani Bhattacharjee, M. Fines-Neuschild, I. Stekl, Mala Das, J. P. Martin, Manuel Bou-Cabo, P. Mitra, Shashank Priya, E. Behnke, Ivan Felis, R. Filgas, A. Plante, N. Starinski, P. S. Cooper, E. Vázquez-Jáuregui, Andrew Sonnenschein, M. Lafrenière, O. Harris, and C. E. Dahl
Subjects: Physics, Particle physics, Physics - Instrumentation and Detectors, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Atomic energy, FOS: Physical sciences, Library science, Instrumentation and Detectors (physics.ins-det), 01 natural sciences, 7. Clean energy, Technical support, FISICA APLICADA, 0103 physical sciences, Christian ministry, 010306 general physics, National laboratory, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: New data are reported from a second run of the 2-liter PICO-2L C3F8 bubble chamber with a total exposure of 129 kg-days at a thermodynamic threshold energy of 3.3 keV. These data show that measures taken to control particulate contamination in the superheated fluid resulted in the absence of the anomalous background events observed in the first run of this bubble chamber. One single nuclear-recoil event was observed in the data, consistent both with the predicted background rate from neutrons and with the observed rate of unambiguous multiple-bubble neutron scattering events. The chamber exhibits the same excellent electron-recoil and alpha decay rejection as was previously reported. These data provide the most stringent direct detection constraints on weakly interacting massive particle (WIMP)-proton spin-dependent scattering to date for WIMP masses < 50 GeV/c(2)., The PICO Collaboration thanks SNOLAB for their exceptional laboratory space and technical support. We also thank Fermi National Accelerator Laboratory (Contract No. DE-AC02-07CH11359) and Pacific Northwest National Laboratory for their support. This work is supported by the National Sciences and Engineering Research Council of Canada (NSERC), the Canada Foundation for Innovation (CFI), the National Science Foundation (NSF) under the Grants No. PHY-1242637, No. PHY-0919526, No. PHY-1205987, and No. PHY-1506377 and by the U.S. Department of Energy under Award No. DE-SC-0012161. We also acknowledge the support of Department of Atomic Energy (DAE), Government of India, under the Center of AstroParticle Physics II project (CAPP-II) at Saha Institute of Physics (SINP); the Czech Ministry of Education, Youth and Sports (Grant No. LM2011027); the Spanish Ministerio de Economia y Competitividad, Consolider MultiDark (Grant No. CSD2009-00064) and DGAPA-UNAM through grant PAPIIT No. IA100316.
Published: 2016
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44. Search for2νββdecay ofXe136to the01+excited state ofBa136with the EXO-200 liquid xenon detector

Author: A.C. Odian, I. Ostrovskiy, David Leonard, Thomas Koffas, W. M. Fairbank, O. Ya. Zeldovich, S. Feyzbakhsh, E. Smith, R. Krücken, D. Beck, M. Coon, D. Fudenberg, T. Brunner, J. King, O. Njoya, R. DeVoe, Peter Fierlinger, Justin Albert, K. Graham, Monica Dunford, A. Pocar, R. H. Nelson, U. Wichoski, M. Weber, T. Walton, Petr Vogel, M. Tarka, C. Licciardi, C. R. Hall, T. Tolba, C. Chambers, Q. Y. Xu, Ryan Killick, R. Tsang, M. Danilov, J. Walton, P. C. Rowson, D. J. Auty, A. Kuchenkov, Jens Dilling, J. Chaves, W. Feldmeier, F. Retiere, B. Mong, C.Y. Prescott, A. Craycraft, Martin Breidenbach, S. J. Daugherty, R. Gornea, L. J. Kaufman, T. Daniels, M. Hughes, J. Farine, S. Delaquis, A. P. Waite, Simon Johnston, J. C. Davis, Y-R Yen, Guofu Cao, T. N. Johnson, Yuehe Lin, Giorgio Gratta, J. L. Wood, David Moore, J. J. Russell, T. Didberidze, A. Der Mesrobian-Kabakian, J.-L. Vuilleumier, K. S. Kumar, B. T. Cleveland, Liang Yang, M. J. Dolinski, S. Kravitz, A. Piepke, A. Burenkov, A. Karelin, A. Johnson, V.N. Stekhanov, David A. Sinclair, T. A. Winick, M. J. Jewell, K. Twelker, L. J. Wen, Alexis G. Schubert, R. MacLellan, M. G. Marino, P. S. Barbeau, V. A. Belov, and A. Dolgolenko
Subjects: Semileptonic decay, Physics, 010308 nuclear & particles physics, Detector, chemistry.chemical_element, 7. Clean energy, 01 natural sciences, Lower limit, Xenon, chemistry, Excited state, 0103 physical sciences, Single phase, Atomic physics, Neutrino, 010306 general physics, Ground state
Abstract: EXO-200 is a single phase liquid xenon detector designed to search for neutrinoless ββ decay of ^(136)Xe to the ground state of ^(136)Ba. We report here on a search for the two-neutrino ββ decay of 136Xe to the first 0+ excited state, 0^+_1, of ^(136)Ba based on a 100 kg yr exposure of ^(136)Xe. Using a specialized analysis employing a machine learning algorithm, we obtain a 90% CL half-life sensitivity of 1.7 × 10^(24) yr. We find no statistically significant evidence for the 2νββ decay to the excited state resulting in a lower limit of T^(2ν)_(1/2)(0^+ → 0^+_1) > 6.9 ×10^(23) yr at 90% CL. This observed limit is consistent with the estimated half-life of 2.5 × 10^(25) yr.
Published: 2016
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45. An Optimal Energy Estimator to Reduce Correlated Noise for the EXO-200 Light Readout

Author: A. Der Mesrobian-Kabakian, Yuehe Lin, A. Pocar, S. Kravitz, Monica Dunford, C. Y. Prescott, M. Coon, R. Tsang, A. Craycraft, J. L. Wood, V.N. Stekhanov, Liang Yang, K. S. Kumar, W. R. Cen, R. Gornea, K. Graham, J. J. Russell, J. Farine, M. Danilov, Peter Fierlinger, A. Karelin, A. Dolgolenko, R. DeVoe, Douglas H Beck, David Leonard, V. Belov, M. Tarka, Thomas Koffas, W. M. Fairbank, Y-R Yen, Michael G. Marino, T. Daniels, S. Johnston, T. Brunner, C. G. Davis, O. Ya. Zeldovich, T. Walton, Liangjian Wen, A. S. Johnson, Guofu Cao, Martin Breidenbach, S. J. Daugherty, L. J. Kaufman, A. Burenkov, B. Mong, E. Smith, R. Krücken, F. Retière, J. B. Albert, David A. Sinclair, A. Schubert, Ryan Killick, R. H. Nelson, M. J. Dolinski, U. Wichoski, B. T. Cleveland, P. S. Barbeau, T. Tolba, A. Kuchenkov, S. Feyzbakhsh, Marc Weber, C. Licciardi, C. R. Hall, J. L. Vuilleumier, J. Walton, A. Piepke, Giorgio Gratta, W. Feldmeier, J. Davis, M. Hughes, A. P. Waite, M. J. Jewell, K. Twelker, David Moore, T. Didberidze, T. N. Johnson, D. Fudenberg, R. MacLellan, C. Chambers, P. C. Rowson, S. Delaquis, Jens Dilling, A. Odian, I. Ostrovskiy, and O. Njoya
Subjects: Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, 01 natural sciences, Noise (electronics), Particle detector, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Optics, Double beta decay, 0103 physical sciences, Nuclear Experiment (nucl-ex), 010306 general physics, Instrumentation, Nuclear Experiment, Mathematical Physics, Physics, Scintillation, 010308 nuclear & particles physics, business.industry, Detector, Estimator, Instrumentation and Detectors (physics.ins-det), High Energy Physics::Experiment, business, Energy (signal processing), Radioactive decay
Abstract: The energy resolution of the EXO-200 detector is limited by electronics noise in the measurement of the scintillation response. Here we present a new technique to extract optimal scintillation energy measurements for signals split across multiple channels in the presence of correlated noise. The implementation of these techniques improves the energy resolution of the detector at the neutrinoless double beta decay Q-value from $\left[1.9641\pm 0.0039\right]\%$ to $\left[1.5820\pm 0.0044\right]\%$., Comment: 21 pages, 8 figures, 1 table
Published: 2016
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46. A linear RFQ ion trap for the Enriched Xenon Observatory

Author: David A. Sinclair, S. Waldman, C. R. Hall, K. O'Sullivan, B. Flatt, M. Montero Díez, F. LePort, V. Strickland, A. Odian, J. Wodin, David Leonard, D. Hallman, Yul Martin, L. Ounalli, M. Hauger, W. M. Fairbank, Martin Breidenbach, F. Juget, M. P. Green, P. C. Rowson, J.-M. Vuilleuimier, K. Wamba, D. Mackay, C. Y. Prescott, C. Virtue, Giorgio Gratta, K. Skarpaas, C. K. Hargrove, R. Neilson, J.-L. Vuilleuimier, R. DeVoe, A. Pocar, P. Fierlinger, J. Hodgson, J. Farine, E. Baussan, R. Conley, A. Piepke, B. Mong, P. Weber, D. Schenker, and K. Hall
Subjects: Physics, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Detector, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Fluorescence spectroscopy, Ion, Decay energy, Double beta decay, Ion trap, Atomic physics, Spectroscopy, Instrumentation, Enriched Xenon Observatory
Abstract: The design, construction, and performance of a linear radio-frequency ion trap (RFQ) intended for use in the Enriched Xenon Observatory (EXO) are described. EXO aims to detect the neutrinoless double-beta decay of $^{136}$Xe to $^{136}$Ba. To suppress possible backgrounds EXO will complement the measurement of decay energy and, to some extent, topology of candidate events in a Xe filled detector with the identification of the daughter nucleus ($^{136}$Ba). The ion trap described here is capable of accepting, cooling, and confining individual Ba ions extracted from the site of the candidate double-beta decay event. A single trapped ion can then be identified, with a large signal-to-noise ratio, via laser spectroscopy., Comment: 18 pages, pdflatex, submitted to NIM A
Published: 2007
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47. Measurements of the ion fraction and mobility ofα−andβ-decay products in liquid xenon using the EXO-200 detector

Author: A. Craycraft, James G. Davis, I. Ostrovskiy, M. J. Dolinski, A. Karelin, C. G. Davis, Martin Breidenbach, S. J. Daugherty, David A. Sinclair, T. Walton, R. MacLellan, Liang Yang, M. J. Jewell, K. Twelker, B. Mong, A. Schubert, K. Graham, Giorgio Gratta, David Leonard, R. DeVoe, M. Weber, M. G. Marino, V.N. Stekhanov, Douglas H Beck, M. Danilov, P. Fierlinger, Thomas Koffas, W. M. Fairbank, R. Nelson, Y-R Yen, K. O'Sullivan, Guofu Cao, S. Johnston, X. S. Jiang, J. Wood, D. J. Auty, A. Der Mesrobian-Kabakian, Ryan Killick, L. J. Kaufman, R. Tsang, E. Smith, A. Burenkov, M. Coon, B. T. Cleveland, R. Gornea, Yuehe Lin, C. Chambers, A. Kuchenkov, T. Tolba, W. Feldmeier, A. Piepke, P. C. Rowson, L. J. Wen, A. Pocar, J. J. Russell, J.-L. Vuilleumier, K. S. Kumar, S. Delaquis, S. Kravitz, C. Licciardi, O. Ya. Zeldovich, A. Dolgolenko, M. Tarka, J. Farine, V. Belov, A. Robinson, T. Brunner, Justin Albert, Monica Dunford, U. Wichoski, J. D. Wright, T. N. Johnson, A.C. Odian, A. S. Johnson, P. S. Barbeau, C.Y. Prescott, T. Daniels, C. R. Hall, J. Walton, D. Fudenberg, M. Hughes, A. P. Waite, David Moore, and T. Didberidze
Subjects: Physics, Semileptonic decay, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Branching fraction, 01 natural sciences, Charged particle, Ion, Ionization, Double beta decay, 0103 physical sciences, Alpha decay, Atomic physics, 010306 general physics, Crystal Ball
Abstract: Alpha decays in the EXO-200 detector are used to measure the fraction of charged $^{218}\text{Po}$ and $^{214}\text{Bi}$ daughters created from $\ensuremath{\alpha}$ and $\ensuremath{\beta}$ decays, respectively. $^{222}\text{Rn} \ensuremath{\alpha}$ decays in liquid xenon (LXe) are found to produce $^{218}\text{Po}^{+}$ ions $50.3\ifmmode\pm\else\textpm\fi{}3.0%$ of the time, while the remainder of the $^{218}\text{Po}$ atoms are neutral. The fraction of $^{214}\text{Bi}^{+}$ from $^{214}\text{Pb} \ensuremath{\beta}$ decays in LXe is found to be $76.4\ifmmode\pm\else\textpm\fi{}5.7%$, inferred from the relative rates of $^{218}\text{Po}$ and $^{214}\text{Po} \ensuremath{\alpha}$ decays in the LXe. The average velocity of $^{218}\text{Po}$ ions is observed to decrease for longer drift times. Initially the ions have a mobility of $0.390\ifmmode\pm\else\textpm\fi{}0.006\phantom{\rule{4pt}{0ex}}{\text{cm}}^{2}/(\text{kV}\text{s})$, and at long drift times the mobility is $0.219\ifmmode\pm\else\textpm\fi{}0.004\phantom{\rule{4pt}{0ex}}{\text{cm}}^{2}/(\text{kV}\text{s})$. Time constants associated with the change in mobility during drift of the $^{218}\text{Po}^{+}$ ions are found to be proportional to the electron lifetime in the LXe.
Published: 2015
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48. Dark Matter Search Results from the PICO-2LC3F8Bubble Chamber

Author: R. Neilson, M. Lafrenière, N. Starinski, C. M. Jackson, P. S. Cooper, E. Vázquez-Jáuregui, A. E. Robinson, J. P. Martin, J. I. Collar, M. Hai, M. Fines-Neuschild, S. Daley, M. Laurin, M. Ruschman, M. Jin, K. Clark, O. Harris, V. Zacek, U. Wichoski, D. Baxter, O. Scallon, Shashank Priya, Daniel Broemmelsiek, I. Levine, J. Hall, J. Wells, M. Bou-Cabo, Francoise Girard, J. Farine, G. Giroux, P. S. Bhattacharjee, A. Plante, C. Amole, R. B. Podviianiuk, Madhusmita Das, S. J. Brice, Andrew Sonnenschein, A. J. Noble, S. Seth, David M. Asner, Ivan Felis, R. Filgas, M. Crisler, E. Behnke, C. E. Dahl, F. Debris, Pitam Mitra, N. Dhungana, Miguel Ardid, E. Mann, I. Lawson, Jie Zhang, C. B. Krauss, W. H. Lippincott, Deepam Maurya, H. Borsodi, and I. Stekl
Subjects: Physics, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Dark matter, General Physics and Astronomy, 7. Clean energy, 01 natural sciences, Nuclear physics, Recoil, WIMP, Weakly interacting massive particles, DAMA/NaI, 0103 physical sciences, Bubble chamber, Neutron, Alpha decay, 010306 general physics
Abstract: New results are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 52 kg of C_{3}F_{8} located in the SNOLAB underground laboratory. As in previous PICO bubble chambers, PICO-60 C_{3}F_{8} exhibits excellent electron recoil and alpha decay rejection, and the observed multiple-scattering neutron rate indicates a single-scatter neutron background of less than one event per month. A blind analysis of an efficiency-corrected 1167-kg day exposure at a 3.3-keV thermodynamic threshold reveals no single-scattering nuclear recoil candidates, consistent with the predicted background. These results set the most stringent direct-detection constraint to date on the weakly interacting massive particle (WIMP)-proton spin-dependent cross section at 3.4×10^{-41} cm^{2} for a 30-GeV c^{-2} WIMP, more than 1 order of magnitude improvement from previous PICO results.
Published: 2015
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49. Measurement of dissolved in water at the Sudbury Neutrino Observatory

Author: M. Liu, H.W. Lee, K. McFarlane, I. Blevis, R. L. Hahn, I. Levine, X Zhu, E. Bonvin, S. Majerus, J. Boger, P. Jagam, A. B. Knox, David A. Sinclair, H. Fergani, J. K. Rowley, J. J. Simpson, H. Heron, C. K. Hargrove, A.S Hamer, J.-X Wang, Bhaskar Sur, S Noël, Minfang Yeh, V. M. Novikov, B. T. Cleveland, Darren Grant, N. A. Jelley, J. Farine, A. J. Noble, G. Doucas, A. B. McDonald, F. Dalnoki-Veress, C. Jillings, M. Shatkay, X Dai, and C. Mifflin
Subjects: Heavy water, Physics, Nuclear and High Energy Physics, Sudbury Neutrino Observatory, 010308 nuclear & particles physics, Degasser, Solar neutrino, Analytical chemistry, chemistry.chemical_element, Radon, Lucas cell, 7. Clean energy, 01 natural sciences, 6. Clean water, Nuclear physics, chemistry.chemical_compound, chemistry, 0103 physical sciences, 010306 general physics, Instrumentation, Water vapor, Cold trap
Abstract: The technique used at the Sudbury Neutrino Observatory (SNO) to measure the concentration of 222 Rn in water is described. Water from the SNO detector is passed through a vacuum degasser (in the light water system) or a membrane contact degasser (in the heavy water system) where dissolved gases, including radon, are liberated. The degasser is connected to a vacuum system which collects the radon on a cold trap and removes most other gases, such as water vapor and N2. After roughly 0.5 tonnes of H2O or 6 tonnes of D2O have been sampled, the accumulated radon is transferred to a Lucas cell. The cell is mounted on a photomultiplier tube which detects the α-particles from the decay of 222 Rn and its progeny. The overall degassing and concentration efficiency is about 38% and the single-α counting efficiency is approximately 75%. The sensitivity of the radon assay system for D2O is equivalent to ∼3×10 −15 g U/g water. The radon concentration in both the H2O and D2O is sufficiently low that the rate of background events from U-chain elements is a small fraction of the interaction rate of solar neutrinos by the neutral current reaction.
Published: 2004
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50. Investigation of radioactivity-induced backgrounds in EXO-200

Author: T. Daniels, C. Y. Prescott, A. S. Johnson, Douglas H Beck, T. N. Johnson, M. J. Jewell, A. Dolgolenko, D. Fudenberg, Y-R Yen, K. Twelker, J. B. Albert, P. C. Rowson, A. Pocar, M. Hughes, A. Piepke, A. P. Waite, I. Ostrovskiy, J. Farine, R. MacLellan, B. Mong, R. Nelson, U. Wichoski, S. Delaquis, V. Belov, S. Herrin, A Rivas, M. Danilov, A. Craycraft, C. R. Hall, David Moore, A. Schubert, T. Didberidze, A.C. Odian, C. G. Davis, Yuehe Lin, C. Benitez-Medina, Giorgio Gratta, J. Wood, Martin Breidenbach, D. J. Auty, T. Tolba, S. J. Daugherty, J. L. Vuilleumier, P. S. Barbeau, T. Walton, G. Giroux, J. Walton, V.N. Stekhanov, T. Brunner, J. J. Russell, R. Gornea, K. S. Kumar, W. Feldmeier, Marc Weber, David A. Sinclair, Ryan Killick, David Leonard, Thomas Koffas, B. T. Cleveland, W. M. Fairbank, Monica Dunford, A. Kuchenkov, C. Chambers, K. Graham, M. Coon, O. Ya. Zeldovich, A. Karelin, J. Davis, M. Tarka, C. Licciardi, L. J. Kaufman, R. DeVoe, X. S. Jiang, A. Der Mesrobian-Kabakian, E. Smith, S. Kravitz, Liang Yang, M. J. Dolinski, Michael G. Marino, S. Johnston, P. Fierlinger, Liangjian Wen, Guofu Cao, A. Burenkov, and R. Tsang
Subjects: Physics, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, 010308 nuclear & particles physics, FOS: Physical sciences, Instrumentation and Detectors (physics.ins-det), Parameter space, 01 natural sciences, Beta decay, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Double beta decay, 0103 physical sciences, Beta (velocity), Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment
Abstract: The search for neutrinoless double-beta decay (0{\nu}{\beta}{\beta}) requires extremely low background and a good understanding of their sources and their influence on the rate in the region of parameter space relevant to the 0{\nu}{\beta}{\beta} signal. We report on studies of various {\beta}- and {\gamma}-backgrounds in the liquid- xenon-based EXO-200 0{\nu}{\beta}{\beta} experiment. With this work we try to better understand the location and strength of specific background sources and compare the conclusions to radioassay results taken before and during detector construction. Finally, we discuss the implications of these studies for EXO-200 as well as for the next-generation, tonne-scale nEXO detector., Comment: 9 pages, 7 figures, 3 tables
Published: 2015

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