Search

Your search keyword '"Gladstone, L"' showing total 16 results
Start Over Author "Gladstone, L" Journal physical review letters
16 results on '"Gladstone, L"'

1. First Results from CUORE: A Search for Lepton Number Violation via 0νββ Decay of Te130

Author

Alduino, C, Alessandria, F, Alfonso, K, Andreotti, E, Arnaboldi, C, Avignone, FT, Azzolini, O, Balata, M, Bandac, I, Banks, TI, Bari, G, Barucci, M, Beeman, JW, Bellini, F, Benato, G, Bersani, A, Biare, D, Biassoni, M, Bragazzi, F, Branca, A, Brofferio, C, Bryant, A, Buccheri, A, Bucci, C, Bulfon, C, Camacho, A, Caminata, A, Canonica, L, Cao, XG, Capelli, S, Capodiferro, M, Cappelli, L, Cardani, L, Cariello, M, Carniti, P, Carrettoni, M, Casali, N, Cassina, L, Cereseto, R, Ceruti, G, Chiarini, A, Chiesa, D, Chott, N, Clemenza, M, Conventi, D, Copello, S, Cosmelli, C, Cremonesi, O, Crescentini, C, Creswick, RJ, Cushman, JS, D’Addabbo, A, D’Aguanno, D, Dafinei, I, Datskov, V, Davis, CJ, Del Corso, F, Dell’Oro, S, Deninno, MM, Di Domizio, S, Di Vacri, ML, Di Paolo, L, Drobizhev, A, Ejzak, L, Faccini, R, Fang, DQ, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, MA, Freedman, SJ, Fujikawa, BK, Gaigher, R, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Goett, J, Gorla, P, Gotti, C, Guandalini, C, Guerzoni, M, Gutierrez, TD, Haller, EE, Han, K, Hansen, EV, Heeger, KM, Hennings-Yeomans, R, Hickerson, KP, Huang, HZ, Iannone, M, Ioannucci, L, Kadel, R, Keppel, G, Kogler, L, Kolomensky, Yu G, Leder, A, Ligi, C, and Lim, KE

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, CUORE Collaboration, nucl-ex, hep-ex, physics.ins-det, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract

The CUORE experiment, a ton-scale cryogenic bolometer array, recently began operation at the Laboratori Nazionali del Gran Sasso in Italy. The array represents a significant advancement in this technology, and in this work we apply it for the first time to a high-sensitivity search for a lepton-number-violating process: ^{130}Te neutrinoless double-beta decay. Examining a total TeO_{2} exposure of 86.3 kg yr, characterized by an effective energy resolution of (7.7±0.5)  keV FWHM and a background in the region of interest of (0.014±0.002)  counts/(keV kg yr), we find no evidence for neutrinoless double-beta decay. Including systematic uncertainties, we place a lower limit on the decay half-life of T_{1/2}^{0ν}(^{130}Te)>1.3×10^{25}  yr (90% C.L.); the median statistical sensitivity of this search is 7.0×10^{24}  yr. Combining this result with those of two earlier experiments, Cuoricino and CUORE-0, we find T_{1/2}^{0ν}(^{130}Te)>1.5×10^{25}  yr (90% C.L.), which is the most stringent limit to date on this decay. Interpreting this result as a limit on the effective Majorana neutrino mass, we find m_{ββ}

Published
2018

2. First Results from CUORE: A Search for Lepton Number Violation via 0νββ Decay of ^{130}Te.

Author

Alduino, C, Alessandria, F, Alfonso, K, Andreotti, E, Arnaboldi, C, Avignone, FT, Azzolini, O, Balata, M, Bandac, I, Banks, TI, Bari, G, Barucci, M, Beeman, JW, Bellini, F, Benato, G, Bersani, A, Biare, D, Biassoni, M, Bragazzi, F, Branca, A, Brofferio, C, Bryant, A, Buccheri, A, Bucci, C, Bulfon, C, Camacho, A, Caminata, A, Canonica, L, Cao, XG, Capelli, S, Capodiferro, M, Cappelli, L, Cardani, L, Cariello, M, Carniti, P, Carrettoni, M, Casali, N, Cassina, L, Cereseto, R, Ceruti, G, Chiarini, A, Chiesa, D, Chott, N, Clemenza, M, Conventi, D, Copello, S, Cosmelli, C, Cremonesi, O, Crescentini, C, Creswick, RJ, Cushman, JS, D'Addabbo, A, D'Aguanno, D, Dafinei, I, Datskov, V, Davis, CJ, Del Corso, F, Dell'Oro, S, Deninno, MM, Di Domizio, S, Di Vacri, ML, Di Paolo, L, Drobizhev, A, Ejzak, L, Faccini, R, Fang, DQ, Faverzani, M, Ferri, E, Ferroni, F, Fiorini, E, Franceschi, MA, Freedman, SJ, Fujikawa, BK, Gaigher, R, Giachero, A, Gironi, L, Giuliani, A, Gladstone, L, Goett, J, Gorla, P, Gotti, C, Guandalini, C, Guerzoni, M, Gutierrez, TD, Haller, EE, Han, K, Hansen, EV, Heeger, KM, Hennings-Yeomans, R, Hickerson, KP, Huang, HZ, Iannone, M, Ioannucci, L, Kadel, R, Keppel, G, Kogler, L, Kolomensky, Yu G, Leder, A, Ligi, C, and Lim, KE

Subjects
CUORE Collaboration, nucl-ex, hep-ex, physics.ins-det, General Physics, Mathematical Sciences, Physical Sciences, Engineering
Abstract

The CUORE experiment, a ton-scale cryogenic bolometer array, recently began operation at the Laboratori Nazionali del Gran Sasso in Italy. The array represents a significant advancement in this technology, and in this work we apply it for the first time to a high-sensitivity search for a lepton-number-violating process: ^{130}Te neutrinoless double-beta decay. Examining a total TeO_{2} exposure of 86.3 kg yr, characterized by an effective energy resolution of (7.7±0.5)  keV FWHM and a background in the region of interest of (0.014±0.002)  counts/(keV kg yr), we find no evidence for neutrinoless double-beta decay. Including systematic uncertainties, we place a lower limit on the decay half-life of T_{1/2}^{0ν}(^{130}Te)>1.3×10^{25}  yr (90% C.L.); the median statistical sensitivity of this search is 7.0×10^{24}  yr. Combining this result with those of two earlier experiments, Cuoricino and CUORE-0, we find T_{1/2}^{0ν}(^{130}Te)>1.5×10^{25}  yr (90% C.L.), which is the most stringent limit to date on this decay. Interpreting this result as a limit on the effective Majorana neutrino mass, we find m_{ββ}

Published
2018

3. Constraints on Ultrahigh-Energy Cosmic-Ray Sources from a Search for Neutrinos above 10 PeV with IceCube

Author

Aartsen, MG, Abraham, K, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Archinger, M, Argüelles, C, Auffenberg, J, Axani, S, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Becker Tjus, J, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blot, S, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Braun, J, Brayeur, L, Bretz, H-P, Burgman, A, Carver, T, Casier, M, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Coenders, S, Collin, GH, Conrad, JM, Cowen, DF, Cross, R, Day, M, de André, JPAM, De Clercq, C, Del Pino Rosendo, E, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, di Lorenzo, V, Dujmovic, H, Dumm, JP, Dunkman, M, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eller, P, Euler, S, Evenson, PA, Fahey, S, Fazely, AR, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Flis, S, Fösig, C-C, Franckowiak, A, Friedman, E, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Ghorbani, K, Giang, W, Gladstone, L, Glagla, M, Glüsenkamp, T, Goldschmidt, A, Golup, G, and Gonzalez, JG

Subjects
IceCube Collaboration, astro-ph.HE, astro-ph.CO, Mathematical Sciences, Physical Sciences, Engineering, General Physics
Abstract

We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 10^{9}  GeV, based on an analysis of seven years of IceCube data. This analysis efficiently selects very high- energy neutrino-induced events which have deposited energies from 5×10^{5}  GeV to above 10^{11}  GeV. Two neutrino-induced events with an estimated deposited energy of (2.6±0.3)×10^{6}  GeV, the highest neutrino energy observed so far, and (7.7±2.0)×10^{5}  GeV were detected. The atmospheric background-only hypothesis of detecting these events is rejected at 3.6σ. The hypothesis that the observed events are of cosmogenic origin is also rejected at >99% CL because of the limited deposited energy and the nonobservation of events at higher energy, while their observation is consistent with an astrophysical origin. Our limits on cosmogenic neutrino fluxes disfavor the UHECR sources having a cosmological evolution stronger than the star formation rate, e.g., active galactic nuclei and γ-ray bursts, assuming proton-dominated UHECRs. Constraints on UHECR sources including mixed and heavy UHECR compositions are obtained for models of neutrino production within UHECR sources. Our limit disfavors a significant part of parameter space for active galactic nuclei and new-born pulsar models. These limits on the ultrahigh-energy neutrino flux models are the most stringent to date.

Published
2016

4. Searches for Sterile Neutrinos with the IceCube Detector

Author

Aartsen, MG, Abraham, K, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Andeen, K, Anderson, T, Ansseau, I, Anton, G, Archinger, M, Argüelles, C, Arlen, TC, Auffenberg, J, Axani, S, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Becker Tjus, J, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Blaufuss, E, Blot, S, Boersma, DJ, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Braun, J, Brayeur, L, Bretz, H-P, Burgman, A, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Clark, K, Classen, L, Coenders, S, Collin, GH, Conrad, JM, Cowen, DF, Cruz Silva, AH, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, Del Pino Rosendo, E, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, di Lorenzo, V, Dujmovic, H, Dumm, JP, Dunkman, M, Eberhardt, B, Ehrhardt, T, Eichmann, B, Euler, S, Evenson, PA, Fahey, S, Fazely, AR, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Flis, S, Fösig, C-C, Fuchs, T, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Ghorbani, K, Giang, W, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, and Gonzalez, JG

Subjects
IceCube Collaboration, Mathematical Sciences, Physical Sciences, Engineering, General Physics
Abstract

The IceCube neutrino telescope at the South Pole has measured the atmospheric muon neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to 20 TeV range, to search for the oscillation signatures of light sterile neutrinos. No evidence for anomalous ν_{μ} or ν[over ¯]_{μ} disappearance is observed in either of two independently developed analyses, each using one year of atmospheric neutrino data. New exclusion limits are placed on the parameter space of the 3+1 model, in which muon antineutrinos experience a strong Mikheyev-Smirnov-Wolfenstein-resonant oscillation. The exclusion limits extend to sin^{2}2θ_{24}≤0.02 at Δm^{2}∼0.3  eV^{2} at the 90% confidence level. The allowed region from global analysis of appearance experiments, including LSND and MiniBooNE, is excluded at approximately the 99% confidence level for the global best-fit value of |U_{e4}|^{2}.

Published
2016

5. Evidence for Astrophysical Muon Neutrinos from the Northern Sky with IceCube

Author

Aartsen, MG, Abraham, K, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Archinger, M, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Tjus, J Becker, Becker, K-H, Beiser, E, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Börner, M, Bos, F, Bose, D, Böser, S, Botner, O, Braun, J, Brayeur, L, Bretz, H-P, Brown, AM, Buzinsky, N, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Coenders, S, Cowen, DF, Silva, AH Cruz, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de Wasseige, G, de With, M, DeYoung, T, Díaz-Vélez, JC, Dumm, JP, Dunkman, M, Eagan, R, Eberhardt, B, Ehrhardt, T, Eichmann, B, Euler, S, Evenson, PA, Fadiran, O, Fahey, S, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Fuchs, T, Glagla, M, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Ghorbani, K, Gier, D, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, and Goodman, JA

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, IceCube Collaboration, astro-ph.HE, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract

Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern Hemisphere data set consisting primarily of ν(e) and ν(τ) charged-current and neutral-current (cascade) neutrino interactions. In the analysis presented here, a data sample of approximately 35,000 muon neutrinos from the Northern sky is extracted from data taken during 659.5 days of live time recorded between May 2010 and May 2012. While this sample is composed primarily of neutrinos produced by cosmic ray interactions in Earth's atmosphere, the highest energy events are inconsistent with a hypothesis of solely terrestrial origin at 3.7σ significance. These neutrinos can, however, be explained by an astrophysical flux per neutrino flavor at a level of Φ(E(ν))=9.9(-3.4)(+3.9)×10(-19)  GeV(-1) cm(-2) sr(-1) s(-1)(E(ν)/100  TeV(-2), consistent with IceCube's Southern-Hemisphere-dominated result. Additionally, a fit for an astrophysical flux with an arbitrary spectral index is performed. We find a spectral index of 2.2(-0.2)(+0.2), which is also in good agreement with the Southern Hemisphere result.

Published
2015

6. Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

Author

Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Bay, R, Beatty, JJ, Becker Tjus, J, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bos, F, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Buzinsky, N, Casey, J, Casier, M, Cheung, E, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Clevermann, F, Coenders, S, Cowen, DF, Cruz Silva, AH, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, Dembinski, H, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dumm, JP, Dunkman, M, Eagan, R, Eberhardt, B, Ehrhardt, T, Eichmann, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Frantzen, K, Fuchs, T, Gaisser, TK, Gaior, R, Gallagher, J, Gerhardt, L, Gier, D, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grant, D, Gretskov, P, Groh, JC, Groß, A, and Ha, C

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, IceCube Collaboration, astro-ph.HE, hep-ex, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract

A diffuse flux of astrophysical neutrinos above 100 TeV has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to 35 TeV and analyze its flavor composition by classifying events as showers or tracks. Taking advantage of lower atmospheric backgrounds for showerlike events, we obtain a shower-biased sample containing 129 showers and 8 tracks collected in three years from 2010 to 2013. We demonstrate consistency with the (fe:fμ:fτ)⊕≈(1:1:1)⊕ flavor ratio at Earth commonly expected from the averaged oscillations of neutrinos produced by pion decay in distant astrophysical sources. Limits are placed on nonstandard flavor compositions that cannot be produced by averaged neutrino oscillations but could arise in exotic physics scenarios. A maximally tracklike composition of (0:1:0)⊕ is excluded at 3.3σ, and a purely showerlike composition of (1:0:0)⊕ is excluded at 2.3σ.

Published
2015

7. Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

Author

Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Arguelles, C, Arlen, TC, Auffenberg, J, Bai, X, Barwick, SW, Baum, V, Beatty, JJ, Becker Tjus, J, Becker, K-H, BenZvi, S, Berghaus, P, Berley, D, Bernardini, E, Bernhard, A, Besson, DZ, Binder, G, Bindig, D, Bissok, M, Blaufuss, E, Blumenthal, J, Boersma, DJ, Bohm, C, Bose, D, Böser, S, Botner, O, Brayeur, L, Bretz, H-P, Brown, AM, Casey, J, Casier, M, Chirkin, D, Christov, A, Christy, B, Clark, K, Classen, L, Clevermann, F, Coenders, S, Cowen, DF, Cruz Silva, AH, Danninger, M, Daughhetee, J, Davis, JC, Day, M, de André, JPAM, De Clercq, C, De Ridder, S, Desiati, P, de Vries, KD, de With, M, DeYoung, T, Díaz-Vélez, JC, Dunkman, M, Eagan, R, Eberhardt, B, Eichmann, B, Eisch, J, Euler, S, Evenson, PA, Fadiran, O, Fazely, AR, Fedynitch, A, Feintzeig, J, Felde, J, Feusels, T, Filimonov, K, Finley, C, Fischer-Wasels, T, Flis, S, Franckowiak, A, Frantzen, K, Fuchs, T, Gaisser, TK, Gallagher, J, Gerhardt, L, Gier, D, Gladstone, L, Glüsenkamp, T, Goldschmidt, A, Golup, G, Gonzalez, JG, Goodman, JA, Góra, D, Grandmont, DT, Grant, D, Gretskov, P, Groh, JC, Groß, A, Ha, C, Haack, C, Haj Ismail, A, Hallen, P, and Hallgren, A

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, IceCube Collaboration, astro-ph.HE, astro-ph.CO, hep-ex, Mathematical Sciences, Engineering, General Physics, Mathematical sciences, Physical sciences
Abstract

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012-2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV-PeV range at the level of 10(-8)  GeV cm-2 s-1 sr-1 per flavor and reject a purely atmospheric explanation for the combined three-year data at 5.7σ. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotropic arrival directions, suggesting either numerous or spatially extended sources. The three-year data set, with a live time of 988 days, contains a total of 37 neutrino candidate events with deposited energies ranging from 30 to 2000 TeV. The 2000-TeV event is the highest-energy neutrino interaction ever observed.

Published
2014

8. Measurement of Atmospheric Neutrino Oscillations with IceCube

Author

Aartsen, M. G., primary, Abbasi, R., additional, Abdou, Y., additional, Ackermann, M., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Altmann, D., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Baum, V., additional, Bay, R., additional, Beatty, J. J., additional, Bechet, S., additional, Becker Tjus, J., additional, Becker, K.-H., additional, Bell, M., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bernhard, A., additional, Bertrand, D., additional, Besson, D. Z., additional, Binder, G., additional, Bindig, D., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohaichuk, S., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Brayeur, L., additional, Bretz, H.-P., additional, Brown, A. M., additional, Bruijn, R., additional, Brunner, J., additional, Carson, M., additional, Casey, J., additional, Casier, M., additional, Chirkin, D., additional, Christov, A., additional, Christy, B., additional, Clark, K., additional, Clevermann, F., additional, Coenders, S., additional, Cohen, S., additional, Cowen, D. F., additional, Cruz Silva, A. H., additional, Danninger, M., additional, Daughhetee, J., additional, Davis, J. C., additional, De Clercq, C., additional, De Ridder, S., additional, Desiati, P., additional, de With, M., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dunkman, M., additional, Eagan, R., additional, Eberhardt, B., additional, Eisch, J., additional, Ellsworth, R. W., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feintzeig, J., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Fischer-Wasels, T., additional, Flis, S., additional, Franckowiak, A., additional, Franke, R., additional, Frantzen, K., additional, Fuchs, T., additional, Gaisser, T. K., additional, Gallagher, J., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Golup, G., additional, Gonzalez, J. G., additional, Goodman, J. A., additional, Góra, D., additional, Grandmont, D. T., additional, Grant, D., additional, Groß, A., additional, Ha, C., additional, Haj Ismail, A., additional, Hallen, P., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Heereman, D., additional, Heinen, D., additional, Helbing, K., additional, Hellauer, R., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Hoffmann, R., additional, Homeier, A., additional, Hoshina, K., additional, Huelsnitz, W., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobi, E., additional, Jacobsen, J., additional, Jagielski, K., additional, Japaridze, G. S., additional, Jero, K., additional, Jlelati, O., additional, Kaminsky, B., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kiryluk, J., additional, Kislat, F., additional, Kläs, J., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kopper, C., additional, Kopper, S., additional, Koskinen, D. J., additional, Kowalski, M., additional, Krasberg, M., additional, Krings, K., additional, Kroll, G., additional, Kunnen, J., additional, Kurahashi, N., additional, Kuwabara, T., additional, Labare, M., additional, Landsman, H., additional, Larson, M. J., additional, Lesiak-Bzdak, M., additional, Leuermann, M., additional, Leute, J., additional, Lünemann, J., additional, Madsen, J., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McNally, F., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Miarecki, S., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Mohrmann, L., additional, Montaruli, T., additional, Morse, R., additional, Nahnhauer, R., additional, Naumann, U., additional, Niederhausen, H., additional, Nowicki, S. C., additional, Nygren, D. R., additional, Obertacke, A., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, O’Murchadha, A., additional, Palazzo, A., additional, Paul, L., additional, Pepper, J. A., additional, Pérez de los Heros, C., additional, Pfendner, C., additional, Pieloth, D., additional, Pinat, E., additional, Pirk, N., additional, Posselt, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rädel, L., additional, Rameez, M., additional, Rawlins, K., additional, Redl, P., additional, Reimann, R., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Richman, M., additional, Riedel, B., additional, Rodrigues, J. P., additional, Rott, C., additional, Ruhe, T., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Saba, S. M., additional, Salameh, T., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Scheel, M., additional, Scheriau, F., additional, Schmidt, T., additional, Schmitz, M., additional, Schoenen, S., additional, Schöneberg, S., additional, Schönwald, A., additional, Schukraft, A., additional, Schulte, L., additional, Schulz, O., additional, Seckel, D., additional, Sestayo, Y., additional, Seunarine, S., additional, Sheremata, C., additional, Smith, M. W. E., additional, Soldin, D., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stasik, A., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stößl, A., additional, Strahler, E. A., additional, Ström, R., additional, Sullivan, G. W., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Tešić, G., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Usner, M., additional, van der Drift, D., additional, van Eijndhoven, N., additional, Van Overloop, A., additional, van Santen, J., additional, Vehring, M., additional, Voge, M., additional, Vraeghe, M., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Wasserman, R., additional, Weaver, Ch., additional, Wellons, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Williams, D. R., additional, Wissing, H., additional, Wolf, M., additional, Wood, T. R., additional, Woschnagg, K., additional, Xu, C., additional, Xu, D. L., additional, Xu, X. W., additional, Yanez, J. P., additional, Yodh, G., additional, Yoshida, S., additional, Zarzhitsky, P., additional, Ziemann, J., additional, Zierke, S., additional, and Zoll, M., additional

Published
2013
Full Text
View/download PDF

9. First Observation of PeV-Energy Neutrinos with IceCube

Author

Aartsen, M. G., primary, Abbasi, R., additional, Abdou, Y., additional, Ackermann, M., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Altmann, D., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Baum, V., additional, Bay, R., additional, Beatty, J. J., additional, Bechet, S., additional, Becker Tjus, J., additional, Becker, K.-H., additional, Bell, M., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bernhard, A., additional, Bertrand, D., additional, Besson, D. Z., additional, Binder, G., additional, Bindig, D., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohaichuk, S., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Brayeur, L., additional, Bretz, H.-P., additional, Brown, A. M., additional, Bruijn, R., additional, Brunner, J., additional, Carson, M., additional, Casey, J., additional, Casier, M., additional, Chirkin, D., additional, Christov, A., additional, Christy, B., additional, Clark, K., additional, Clevermann, F., additional, Coenders, S., additional, Cohen, S., additional, Cowen, D. F., additional, Cruz Silva, A. H., additional, Danninger, M., additional, Daughhetee, J., additional, Davis, J. C., additional, De Clercq, C., additional, De Ridder, S., additional, Desiati, P., additional, de With, M., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dunkman, M., additional, Eagan, R., additional, Eberhardt, B., additional, Eisch, J., additional, Ellsworth, R. W., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feintzeig, J., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Fischer-Wasels, T., additional, Flis, S., additional, Franckowiak, A., additional, Franke, R., additional, Frantzen, K., additional, Fuchs, T., additional, Gaisser, T. K., additional, Gallagher, J., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Golup, G., additional, Gonzalez, J. G., additional, Goodman, J. A., additional, Góra, D., additional, Grant, D., additional, Groß, A., additional, Gurtner, M., additional, Ha, C., additional, Haj Ismail, A., additional, Hallen, P., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Heereman, D., additional, Heinen, D., additional, Helbing, K., additional, Hellauer, R., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Hoffmann, R., additional, Homeier, A., additional, Hoshina, K., additional, Huelsnitz, W., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobi, E., additional, Jacobsen, J., additional, Jagielski, K., additional, Japaridze, G. S., additional, Jero, K., additional, Jlelati, O., additional, Kaminsky, B., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kiryluk, J., additional, Kislat, F., additional, Kläs, J., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kopper, C., additional, Kopper, S., additional, Koskinen, D. J., additional, Kowalski, M., additional, Krasberg, M., additional, Krings, K., additional, Kroll, G., additional, Kunnen, J., additional, Kurahashi, N., additional, Kuwabara, T., additional, Labare, M., additional, Landsman, H., additional, Larson, M. J., additional, Lesiak-Bzdak, M., additional, Leuermann, M., additional, Leute, J., additional, Lünemann, J., additional, Madsen, J., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McNally, F., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Miarecki, S., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Mohrmann, L., additional, Montaruli, T., additional, Morse, R., additional, Nahnhauer, R., additional, Naumann, U., additional, Niederhausen, H., additional, Nowicki, S. C., additional, Nygren, D. R., additional, Obertacke, A., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, O’Murchadha, A., additional, Paul, L., additional, Pepper, J. A., additional, Pérez de los Heros, C., additional, Pfendner, C., additional, Pieloth, D., additional, Pinat, E., additional, Pirk, N., additional, Posselt, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rädel, L., additional, Rameez, M., additional, Rawlins, K., additional, Redl, P., additional, Reimann, R., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Richman, M., additional, Riedel, B., additional, Rodrigues, J. P., additional, Rott, C., additional, Ruhe, T., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Saba, S. M., additional, Salameh, T., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Scheel, M., additional, Scheriau, F., additional, Schmidt, T., additional, Schmitz, M., additional, Schoenen, S., additional, Schöneberg, S., additional, Schönwald, A., additional, Schukraft, A., additional, Schulte, L., additional, Schulz, O., additional, Seckel, D., additional, Sestayo, Y., additional, Seunarine, S., additional, Sheremata, C., additional, Smith, M. W. E., additional, Soiron, M., additional, Soldin, D., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stasik, A., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stößl, A., additional, Strahler, E. A., additional, Ström, R., additional, Sullivan, G. W., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Ter-Antonyan, S., additional, Tešić, G., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Usner, M., additional, van der Drift, D., additional, van Eijndhoven, N., additional, Van Overloop, A., additional, van Santen, J., additional, Vehring, M., additional, Voge, M., additional, Vraeghe, M., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Wasserman, R., additional, Weaver, Ch., additional, Wellons, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Williams, D. R., additional, Wissing, H., additional, Wolf, M., additional, Wood, T. R., additional, Woschnagg, K., additional, Xu, C., additional, Xu, D. L., additional, Xu, X. W., additional, Yanez, J. P., additional, Yodh, G., additional, Yoshida, S., additional, Zarzhitsky, P., additional, Ziemann, J., additional, Zierke, S., additional, Zilles, A., additional, and Zoll, M., additional

Published
2013
Full Text
View/download PDF

10. Measurement of the AtmosphericνeFlux in IceCube

Author

Aartsen, M. G., primary, Abbasi, R., additional, Abdou, Y., additional, Ackermann, M., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Altmann, D., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Baum, V., additional, Bay, R., additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker Tjus, J., additional, Becker, K.-H., additional, Bell, M., additional, Benabderrahmane, M. L., additional, BenZvi, S., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bernhard, A., additional, Bertrand, D., additional, Besson, D. Z., additional, Bindig, D., additional, Bissok, M., additional, Blaufuss, E., additional, Blumenthal, J., additional, Boersma, D. J., additional, Bohaichuk, S., additional, Bohm, C., additional, Bose, D., additional, Böser, S., additional, Botner, O., additional, Brayeur, L., additional, Brown, A. M., additional, Bruijn, R., additional, Brunner, J., additional, Buitink, S., additional, Carson, M., additional, Casey, J., additional, Casier, M., additional, Chirkin, D., additional, Christy, B., additional, Clark, K., additional, Clevermann, F., additional, Cohen, S., additional, Cowen, D. F., additional, Cruz Silva, A. H., additional, Danninger, M., additional, Daughhetee, J., additional, Davis, J. C., additional, De Clercq, C., additional, De Ridder, S., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, de With, M., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dreyer, J., additional, Dunkman, M., additional, Eagan, R., additional, Eberhardt, B., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Fedynitch, A., additional, Feintzeig, J., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Fischer-Wasels, T., additional, Flis, S., additional, Franckowiak, A., additional, Franke, R., additional, Frantzen, K., additional, Fuchs, T., additional, Gaisser, T. K., additional, Gallagher, J., additional, Gerhardt, L., additional, Gladstone, L., additional, Glüsenkamp, T., additional, Goldschmidt, A., additional, Golup, G., additional, Goodman, J. A., additional, Góra, D., additional, Grant, D., additional, Groß, A., additional, Gurtner, M., additional, Ha, C., additional, Haj Ismail, A., additional, Hallgren, A., additional, Halzen, F., additional, Hanson, K., additional, Heereman, D., additional, Heimann, P., additional, Heinen, D., additional, Helbing, K., additional, Hellauer, R., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Hoffmann, R., additional, Homeier, A., additional, Hoshina, K., additional, Huelsnitz, W., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Ishihara, A., additional, Jacobi, E., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Jero, K., additional, Jlelati, O., additional, Kaminsky, B., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kiryluk, J., additional, Kislat, F., additional, Kläs, J., additional, Klein, S. R., additional, Köhne, J.-H., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kopper, C., additional, Kopper, S., additional, Koskinen, D. J., additional, Kowalski, M., additional, Krasberg, M., additional, Kroll, G., additional, Kunnen, J., additional, Kurahashi, N., additional, Kuwabara, T., additional, Labare, M., additional, Landsman, H., additional, Larson, M. J., additional, Lesiak-Bzdak, M., additional, Leute, J., additional, Lünemann, J., additional, Madsen, J., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McNally, F., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Miarecki, S., additional, Middell, E., additional, Milke, N., additional, Miller, J., additional, Mohrmann, L., additional, Montaruli, T., additional, Morse, R., additional, Nahnhauer, R., additional, Naumann, U., additional, Niederhausen, H., additional, Nowicki, S. C., additional, Nygren, D. R., additional, Obertacke, A., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, O’Murchadha, A., additional, Panknin, S., additional, Paul, L., additional, Pepper, J. A., additional, Pérez de los Heros, C., additional, Pfendner, C., additional, Pieloth, D., additional, Pirk, N., additional, Posselt, J., additional, Price, P. B., additional, Przybylski, G. T., additional, Rädel, L., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Richman, M., additional, Riedel, B., additional, Rodrigues, J. P., additional, Rott, C., additional, Ruhe, T., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Saba, S. M., additional, Salameh, T., additional, Sander, H.-G., additional, Santander, M., additional, Sarkar, S., additional, Schatto, K., additional, Scheel, M., additional, Scheriau, F., additional, Schmidt, T., additional, Schmitz, M., additional, Schoenen, S., additional, Schöneberg, S., additional, Schönherr, L., additional, Schönwald, A., additional, Schukraft, A., additional, Schulte, L., additional, Schulz, O., additional, Seckel, D., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Sheremata, C., additional, Smith, M. W. E., additional, Soiron, M., additional, Soldin, D., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stasik, A., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stößl, A., additional, Strahler, E. A., additional, Ström, R., additional, Sullivan, G. W., additional, Taavola, H., additional, Taboada, I., additional, Tamburro, A., additional, Ter-Antonyan, S., additional, Tilav, S., additional, Toale, P. A., additional, Toscano, S., additional, Usner, M., additional, van der Drift, D., additional, van Eijndhoven, N., additional, Van Overloop, A., additional, van Santen, J., additional, Vehring, M., additional, Voge, M., additional, Vraeghe, M., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Wasserman, R., additional, Weaver, Ch., additional, Wellons, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Williams, D. R., additional, Wissing, H., additional, Wolf, M., additional, Wood, T. R., additional, Woschnagg, K., additional, Xu, C., additional, Xu, D. L., additional, Xu, X. W., additional, Yanez, J. P., additional, Yodh, G., additional, Yoshida, S., additional, Zarzhitsky, P., additional, Ziemann, J., additional, Zierke, S., additional, Zilles, A., additional, and Zoll, M., additional

Published
2013
Full Text
View/download PDF

11. Limits on Neutrino Emission from Gamma-Ray Bursts with the 40 String IceCube Detector

Author

Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J.A., Ahlers, M., Andeen, K., Auffenberg, J., Bai, X., Baker, M., Barwick, S.W., Bay, R., Alba, J.L.B., Beattie, K., Beatty, J.J., Bechet, S., Becker, J.K., Becker, K.H., Benabderrahmane, M.L., BenZvi, S., Berdermann, J., Berghaus, P., Berley, D., Bernardini, E., Bertrand, D., Besson, D.Z., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D.J., Bohm, C., Bose, D., Boser, S., Botner, O., Braun, J., Brown, A.M., Buitink, S., Carson, M., Chirkin, D., Christy, B., Clem, J., Clevermann, F., Cohen, S., Colnard, C., Cowen, D.F., D'Agostino, M.V., Danninger, M., Daughhetee, J., Davis, J.C., Clercq, C. De, Demirors, L., Depaepe, O., Descamps, F., Desiati, P., Vries-Uiterweerd, G. de, DeYoung, T., Diaz-Velez, J.C., Dierckxsens, M., Dreyer, J., Dumm, J.P., Ehrlich, R., Eisch, J., Ellsworth, R.W., Engdegard, O., Euler, S., Evenson, P.A., Fadiran, O., Fazely, A.R., Fedynitch, A., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Foerster, M.M., Fox, B.D., Franckowiak, A., Franke, R., Gaisser, T.K., Gallagher, J., Geisler, M., Gerhardt, L., Gladstone, L., Glusenkamp, T., Goldschmidt, A., Goodman, J.A., Grant, D., Griesel, T., Gross, A., Grullon, S., Gurtner, M., Ha, C., Hallgren, A., Halzen, F., Han, K., Hanson, K., Heinen, D., Helbing, K., Herquet, P., Hickford, S., and Lafebre, S.J.

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, High Energy Physics::Experiment, Aetiology, screening and detection [ONCOL 5]
Abstract

Contains fulltext : 98055.pdf (Publisher’s version ) (Open Access) IceCube has become the first neutrino telescope with a sensitivity below the TeV neutrino flux predicted from gamma-ray bursts if gamma-ray bursts are responsible for the observed cosmic-ray flux above 10(18) eV. Two separate analyses using the half-complete IceCube detector, one a dedicated search for neutrinos from p gamma interactions in the prompt phase of the gamma-ray burst fireball and the other a generic search for any neutrino emission from these sources over a wide range of energies and emission times, produced no evidence for neutrino emission, excluding prevailing models at 90% confidence.

Published
2011

12. Extending the Search for Neutrino Point Sources with IceCube above the Horizon

Author

Abbasi, R., primary, Abdou, Y., additional, Abu-Zayyad, T., additional, Adams, J., additional, Aguilar, J. A., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Alba, J. L. Bazo, additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bissok, M., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Botner, O., additional, Bradley, L., additional, Braun, J., additional, Breder, D., additional, Carson, M., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cohen, S., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Díaz-Vélez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Gerhardt, L., additional, Gladstone, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hasegawa, Y., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Homeier, A., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Imlay, R. L., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kemming, N., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Knops, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Koskinen, D. J., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Krings, T., additional, Kroll, G., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Lafebre, S., additional, Laihem, K., additional, Landsman, H., additional, Lauer, R., additional, Lehmann, R., additional, Lennarz, D., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McParland, C. P., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Meures, T., additional, Middell, E., additional, Milke, N., additional, Miyamoto, H., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, Ono, M., additional, Panknin, S., additional, Patton, S., additional, Paul, L., additional, de los Heros, C. Pérez, additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Potthoff, N., additional, Price, P. B., additional, Prikockis, M., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Roucelle, C., additional, Rutledge, D., additional, Ruzybayev, B., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Schatto, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Schukraft, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taboada, I., additional, Tamburro, A., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Terranova, C., additional, Tilav, S., additional, Toale, P. A., additional, Tooker, J., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, van Santen, J., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Wallraff, M., additional, Walter, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebe, K., additional, Wiebusch, C. H., additional, Wiedemann, A., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, C., additional, Xu, X. W., additional, Yodh, G., additional, and Yoshida, S., additional

Published
2009
Full Text
View/download PDF

13. Limits on a Muon Flux from Neutralino Annihilations in the Sun with the IceCube 22-String Detector

Author

Abbasi, R., primary, Abdou, Y., additional, Ackermann, M., additional, Adams, J., additional, Ahlers, M., additional, Andeen, K., additional, Auffenberg, J., additional, Bai, X., additional, Baker, M., additional, Barwick, S. W., additional, Bay, R., additional, Bazo Alba, J. L., additional, Beattie, K., additional, Beatty, J. J., additional, Bechet, S., additional, Becker, J. K., additional, Becker, K.-H., additional, Benabderrahmane, M. L., additional, Berdermann, J., additional, Berghaus, P., additional, Berley, D., additional, Bernardini, E., additional, Bertrand, D., additional, Besson, D. Z., additional, Bissok, M., additional, Blaufuss, E., additional, Boersma, D. J., additional, Bohm, C., additional, Bolmont, J., additional, Böser, S., additional, Botner, O., additional, Bradley, L., additional, Braun, J., additional, Breder, D., additional, Burgess, T., additional, Castermans, T., additional, Chirkin, D., additional, Christy, B., additional, Clem, J., additional, Cohen, S., additional, Cowen, D. F., additional, D’Agostino, M. V., additional, Danninger, M., additional, Day, C. T., additional, De Clercq, C., additional, Demirörs, L., additional, Depaepe, O., additional, Descamps, F., additional, Desiati, P., additional, de Vries-Uiterweerd, G., additional, DeYoung, T., additional, Diaz-Velez, J. C., additional, Dreyer, J., additional, Dumm, J. P., additional, Duvoort, M. R., additional, Edwards, W. R., additional, Ehrlich, R., additional, Eisch, J., additional, Ellsworth, R. W., additional, Engdegård, O., additional, Euler, S., additional, Evenson, P. A., additional, Fadiran, O., additional, Fazely, A. R., additional, Feusels, T., additional, Filimonov, K., additional, Finley, C., additional, Foerster, M. M., additional, Fox, B. D., additional, Franckowiak, A., additional, Franke, R., additional, Gaisser, T. K., additional, Gallagher, J., additional, Ganugapati, R., additional, Gerhardt, L., additional, Gladstone, L., additional, Goldschmidt, A., additional, Goodman, J. A., additional, Gozzini, R., additional, Grant, D., additional, Griesel, T., additional, Groß, A., additional, Grullon, S., additional, Gunasingha, R. M., additional, Gurtner, M., additional, Ha, C., additional, Hallgren, A., additional, Halzen, F., additional, Han, K., additional, Hanson, K., additional, Hasegawa, Y., additional, Heise, J., additional, Helbing, K., additional, Herquet, P., additional, Hickford, S., additional, Hill, G. C., additional, Hoffman, K. D., additional, Hoshina, K., additional, Hubert, D., additional, Huelsnitz, W., additional, Hülß, J.-P., additional, Hulth, P. O., additional, Hultqvist, K., additional, Hussain, S., additional, Imlay, R. L., additional, Inaba, M., additional, Ishihara, A., additional, Jacobsen, J., additional, Japaridze, G. S., additional, Johansson, H., additional, Joseph, J. M., additional, Kampert, K.-H., additional, Kappes, A., additional, Karg, T., additional, Karle, A., additional, Kelley, J. L., additional, Kenny, P., additional, Kiryluk, J., additional, Kislat, F., additional, Klein, S. R., additional, Klepser, S., additional, Knops, S., additional, Kohnen, G., additional, Kolanoski, H., additional, Köpke, L., additional, Kowalski, M., additional, Kowarik, T., additional, Krasberg, M., additional, Kuehn, K., additional, Kuwabara, T., additional, Labare, M., additional, Lafebre, S., additional, Laihem, K., additional, Landsman, H., additional, Lauer, R., additional, Leich, H., additional, Lennarz, D., additional, Lucke, A., additional, Lundberg, J., additional, Lünemann, J., additional, Madsen, J., additional, Majumdar, P., additional, Maruyama, R., additional, Mase, K., additional, Matis, H. S., additional, McParland, C. P., additional, Meagher, K., additional, Merck, M., additional, Mészáros, P., additional, Middell, E., additional, Milke, N., additional, Miyamoto, H., additional, Mohr, A., additional, Montaruli, T., additional, Morse, R., additional, Movit, S. M., additional, Münich, K., additional, Nahnhauer, R., additional, Nam, J. W., additional, Nießen, P., additional, Nygren, D. R., additional, Odrowski, S., additional, Olivas, A., additional, Olivo, M., additional, Ono, M., additional, Panknin, S., additional, Patton, S., additional, Pérez de los Heros, C., additional, Petrovic, J., additional, Piegsa, A., additional, Pieloth, D., additional, Pohl, A. C., additional, Porrata, R., additional, Potthoff, N., additional, Price, P. B., additional, Prikockis, M., additional, Przybylski, G. T., additional, Rawlins, K., additional, Redl, P., additional, Resconi, E., additional, Rhode, W., additional, Ribordy, M., additional, Rizzo, A., additional, Rodrigues, J. P., additional, Roth, P., additional, Rothmaier, F., additional, Rott, C., additional, Roucelle, C., additional, Rutledge, D., additional, Ryckbosch, D., additional, Sander, H.-G., additional, Sarkar, S., additional, Satalecka, K., additional, Schlenstedt, S., additional, Schmidt, T., additional, Schneider, D., additional, Schukraft, A., additional, Schulz, O., additional, Schunck, M., additional, Seckel, D., additional, Semburg, B., additional, Seo, S. H., additional, Sestayo, Y., additional, Seunarine, S., additional, Silvestri, A., additional, Slipak, A., additional, Spiczak, G. M., additional, Spiering, C., additional, Stamatikos, M., additional, Stanev, T., additional, Stephens, G., additional, Stezelberger, T., additional, Stokstad, R. G., additional, Stoufer, M. C., additional, Stoyanov, S., additional, Strahler, E. A., additional, Straszheim, T., additional, Sulanke, K.-H., additional, Sullivan, G. W., additional, Swillens, Q., additional, Taboada, I., additional, Tarasova, O., additional, Tepe, A., additional, Ter-Antonyan, S., additional, Terranova, C., additional, Tilav, S., additional, Tluczykont, M., additional, Toale, P. A., additional, Tosi, D., additional, Turčan, D., additional, van Eijndhoven, N., additional, Vandenbroucke, J., additional, Van Overloop, A., additional, Voigt, B., additional, Walck, C., additional, Waldenmaier, T., additional, Walter, M., additional, Wendt, C., additional, Westerhoff, S., additional, Whitehorn, N., additional, Wiebusch, C. H., additional, Wiedemann, A., additional, Wikström, G., additional, Williams, D. R., additional, Wischnewski, R., additional, Wissing, H., additional, Woschnagg, K., additional, Xu, X. W., additional, Yodh, G., additional, and Yoshida, S., additional

Published
2009
Full Text
View/download PDF

14. Tritium Beta Spectrum Measurement and Neutrino Mass Limit from Cyclotron Radiation Emission Spectroscopy.

Author

Ashtari Esfahani A, Böser S, Buzinsky N, Carmona-Benitez MC, Claessens C, de Viveiros L, Doe PJ, Fertl M, Formaggio JA, Gaison JK, Gladstone L, Grando M, Guigue M, Hartse J, Heeger KM, Huyan X, Johnston J, Jones AM, Kazkaz K, LaRoque BH, Li M, Lindman A, Machado E, Marsteller A, Matthé C, Mohiuddin R, Monreal B, Mueller R, Nikkel JA, Novitski E, Oblath NS, Peña JI, Pettus W, Reimann R, Robertson RGH, Rosa De Jesús D, Rybka G, Saldaña L, Schram M, Slocum PL, Stachurska J, Sun YH, Surukuchi PT, Tedeschi JR, Telles AB, Thomas F, Thomas M, Thorne LA, Thümmler T, Tvrznikova L, Van De Pontseele W, VanDevender BA, Weintroub J, Weiss TE, Wendler T, Young A, Zayas E, and Ziegler A

Abstract

The absolute scale of the neutrino mass plays a critical role in physics at every scale, from the subatomic to the cosmological. Measurements of the tritium end-point spectrum have provided the most precise direct limit on the neutrino mass scale. In this Letter, we present advances by Project 8 to the cyclotron radiation emission spectroscopy (CRES) technique culminating in the first frequency-based neutrino mass limit. With only a cm^{3}-scale physical detection volume, a limit of m&#95;{β}<155  eV/c^{2} (152  eV/c^{2}) is extracted from the background-free measurement of the continuous tritium beta spectrum in a Bayesian (frequentist) analysis. Using ^{83m}Kr calibration data, a resolution of 1.66±0.19  eV (FWHM) is measured, the detector response model is validated, and the efficiency is characterized over the multi-keV tritium analysis window. These measurements establish the potential of CRES for a high-sensitivity next-generation direct neutrino mass experiment featuring low background and high resolution.

Published
2023
Full Text
View/download PDF

15. Measurement of the atmospheric νe flux in IceCube.

Author

Aartsen MG, Abbasi R, Abdou Y, Ackermann M, Adams J, Aguilar JA, Ahlers M, Altmann D, Auffenberg J, Bai X, Baker M, Barwick SW, Baum V, Bay R, Beattie K, Beatty JJ, Bechet S, Becker Tjus J, Becker KH, Bell M, Benabderrahmane ML, BenZvi S, Berdermann J, Berghaus P, Berley D, Bernardini E, Bernhard A, Bertrand D, Besson DZ, Bindig D, Bissok M, Blaufuss E, Blumenthal J, Boersma DJ, Bohaichuk S, Bohm C, Bose D, Böser S, Botner O, Brayeur L, Brown AM, Bruijn R, Brunner J, Buitink S, Carson M, Casey J, Casier M, Chirkin D, Christy B, Clark K, Clevermann F, Cohen S, Cowen DF, Cruz Silva AH, Danninger M, Daughhetee J, Davis JC, De Clercq C, De Ridder S, Desiati P, de Vries-Uiterweerd G, de With M, DeYoung T, Díaz-Vélez JC, Dreyer J, Dunkman M, Eagan R, Eberhardt B, Eisch J, Ellsworth RW, Engdegård O, Euler S, Evenson PA, Fadiran O, Fazely AR, Fedynitch A, Feintzeig J, Feusels T, Filimonov K, Finley C, Fischer-Wasels T, Flis S, Franckowiak A, Franke R, Frantzen K, Fuchs T, Gaisser TK, Gallagher J, Gerhardt L, Gladstone L, Glüsenkamp T, Goldschmidt A, Golup G, Goodman JA, Góra D, Grant D, Groß A, Gurtner M, Ha C, Haj Ismail A, Hallgren A, Halzen F, Hanson K, Heereman D, Heimann P, Heinen D, Helbing K, Hellauer R, Hickford S, Hill GC, Hoffman KD, Hoffmann R, Homeier A, Hoshina K, Huelsnitz W, Hulth PO, Hultqvist K, Hussain S, Ishihara A, Jacobi E, Jacobsen J, Japaridze GS, Jero K, Jlelati O, Kaminsky B, Kappes A, Karg T, Karle A, Kelley JL, Kiryluk J, Kislat F, Kläs J, Klein SR, Köhne JH, Kohnen G, Kolanoski H, Köpke L, Kopper C, Kopper S, Koskinen DJ, Kowalski M, Krasberg M, Kroll G, Kunnen J, Kurahashi N, Kuwabara T, Labare M, Landsman H, Larson MJ, Lesiak-Bzdak M, Leute J, Lünemann J, Madsen J, Maruyama R, Mase K, Matis HS, McNally F, Meagher K, Merck M, Mészáros P, Meures T, Miarecki S, Middell E, Milke N, Miller J, Mohrmann L, Montaruli T, Morse R, Nahnhauer R, Naumann U, Niederhausen H, Nowicki SC, Nygren DR, Obertacke A, Odrowski S, Olivas A, Olivo M, O'Murchadha A, Panknin S, Paul L, Pepper JA, Pérez de los Heros C, Pfendner C, Pieloth D, Pirk N, Posselt J, Price PB, Przybylski GT, Rädel L, Rawlins K, Redl P, Resconi E, Rhode W, Ribordy M, Richman M, Riedel B, Rodrigues JP, Rott C, Ruhe T, Ruzybayev B, Ryckbosch D, Saba SM, Salameh T, Sander HG, Santander M, Sarkar S, Schatto K, Scheel M, Scheriau F, Schmidt T, Schmitz M, Schoenen S, Schöneberg S, Schönherr L, Schönwald A, Schukraft A, Schulte L, Schulz O, Seckel D, Seo SH, Sestayo Y, Seunarine S, Sheremata C, Smith MW, Soiron M, Soldin D, Spiczak GM, Spiering C, Stamatikos M, Stanev T, Stasik A, Stezelberger T, Stokstad RG, Stößl A, Strahler EA, Ström R, Sullivan GW, Taavola H, Taboada I, Tamburro A, Ter-Antonyan S, Tilav S, Toale PA, Toscano S, Usner M, van der Drift D, van Eijndhoven N, Van Overloop A, van Santen J, Vehring M, Voge M, Vraeghe M, Walck C, Waldenmaier T, Wallraff M, Wasserman R, Weaver Ch, Wellons M, Wendt C, Westerhoff S, Whitehorn N, Wiebe K, Wiebusch CH, Williams DR, Wissing H, Wolf M, Wood TR, Woschnagg K, Xu C, Xu DL, Xu XW, Yanez JP, Yodh G, Yoshida S, Zarzhitsky P, Ziemann J, Zierke S, Zilles A, and Zoll M

Abstract

We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of operation of IceCube's DeepCore low-energy extension. Techniques to identify neutrinos interacting within the DeepCore volume and veto muons originating outside the detector are demonstrated. A sample of 1029 events is observed in 281 days of data, of which 496±66(stat)±88(syst) are estimated to be cascade events, including both electron neutrino and neutral current events. The rest of the sample includes residual backgrounds due to atmospheric muons and charged current interactions of atmospheric muon neutrinos. The flux of the atmospheric electron neutrinos is consistent with models of atmospheric neutrinos in this energy range. This constitutes the first observation of electron neutrinos and neutral current interactions in a very large volume neutrino telescope optimized for the TeV energy range.

Published
2013
Full Text
View/download PDF

16. Search for dark matter annihilations in the sun with the 79-string IceCube detector.

Author

Aartsen MG, Abbasi R, Abdou Y, Ackermann M, Adams J, Aguilar JA, Ahlers M, Altmann D, Auffenberg J, Bai X, Baker M, Barwick SW, Baum V, Bay R, Beattie K, Beatty JJ, Bechet S, Becker Tjus J, Becker KH, Bell M, Benabderrahmane ML, BenZvi S, Berdermann J, Berghaus P, Berley D, Bernardini E, Bernhard A, Bertrand D, Besson DZ, Bindig D, Bissok M, Blaufuss E, Blumenthal J, Boersma DJ, Bohaichuk S, Bohm C, Bose D, Böser S, Botner O, Brayeur L, Brown AM, Bruijn R, Brunner J, Buitink S, Carson M, Casey J, Casier M, Chirkin D, Christy B, Clark K, Clevermann F, Cohen S, Cowen DF, Cruz Silva AH, Danninger M, Daughhetee J, Davis JC, De Clercq C, De Ridder S, Desiati P, de Vries-Uiterweerd G, de With M, DeYoung T, Díaz-Vélez JC, Dreyer J, Dunkman M, Eagan R, Eberhardt B, Eisch J, Ellsworth RW, Engdegård O, Euler S, Evenson PA, Fadiran O, Fazely AR, Fedynitch A, Feintzeig J, Feusels T, Filimonov K, Finley C, Fischer-Wasels T, Flis S, Franckowiak A, Franke R, Frantzen K, Fuchs T, Gaisser TK, Gallagher J, Gerhardt L, Gladstone L, Glüsenkamp T, Goldschmidt A, Golup G, Goodman JA, Góra D, Grant D, Groß A, Gurtner M, Ha C, Haj Ismail A, Hallgren A, Halzen F, Hanson K, Heereman D, Heimann P, Heinen D, Helbing K, Hellauer R, Hickford S, Hill GC, Hoffman KD, Hoffmann R, Homeier A, Hoshina K, Huelsnitz W, Hulth PO, Hultqvist K, Hussain S, Ishihara A, Jacobi E, Jacobsen J, Japaridze GS, Jero K, Jlelati O, Kaminsky B, Kappes A, Karg T, Karle A, Kelley JL, Kiryluk J, Kislat F, Kläs J, Klein SR, Köhne JH, Kohnen G, Kolanoski H, Köpke L, Kopper C, Kopper S, Koskinen DJ, Kowalski M, Krasberg M, Kroll G, Kunnen J, Kurahashi N, Kuwabara T, Labare M, Landsman H, Larson MJ, Lesiak-Bzdak M, Leute J, Lünemann J, Madsen J, Maruyama R, Mase K, Matis HS, McNally F, Meagher K, Merck M, Mészáros P, Meures T, Miarecki S, Middell E, Milke N, Miller J, Mohrmann L, Montaruli T, Morse R, Nahnhauer R, Naumann U, Niederhausen H, Nowicki SC, Nygren DR, Obertacke A, Odrowski S, Olivas A, Olivo M, O'Murchadha A, Paul L, Pepper JA, Pérez de los Heros C, Pfendner C, Pieloth D, Pirk N, Posselt J, Price PB, Przybylski GT, Rädel L, Rawlins K, Redl P, Resconi E, Rhode W, Ribordy M, Richman M, Riedel B, Rodrigues JP, Rott C, Ruhe T, Ruzybayev B, Ryckbosch D, Saba SM, Salameh T, Sander HG, Santander M, Sarkar S, Schatto K, Scheel M, Scheriau F, Schmidt T, Schmitz M, Schoenen S, Schöneberg S, Schönherr L, Schönwald A, Schukraft A, Schulte L, Schulz O, Seckel D, Seo SH, Sestayo Y, Seunarine S, Sheremata C, Smith MW, Soiron M, Soldin D, Spiczak GM, Spiering C, Stamatikos M, Stanev T, Stasik A, Stezelberger T, Stokstad RG, Stößl A, Strahler EA, Ström R, Sullivan GW, Taavola H, Taboada I, Tamburro A, Ter-Antonyan S, Tilav S, Toale PA, Toscano S, Usner M, van der Drift D, van Eijndhoven N, Van Overloop A, van Santen J, Vehring M, Voge M, Vraeghe M, Walck C, Waldenmaier T, Wallraff M, Wasserman R, Weaver Ch, Wellons M, Wendt C, Westerhoff S, Whitehorn N, Wiebe K, Wiebusch CH, Williams DR, Wissing H, Wolf M, Wood TR, Woschnagg K, Xu C, Xu DL, Xu XW, Yanez JP, Yodh G, Yoshida S, Zarzhitsky P, Ziemann J, Zierke S, Zilles A, and Zoll M

Abstract

We have performed a search for muon neutrinos from dark matter annihilation in the center of the Sun with the 79-string configuration of the IceCube neutrino telescope. For the first time, the DeepCore subarray is included in the analysis, lowering the energy threshold and extending the search to the austral summer. The 317 days of data collected between June 2010 and May 2011 are consistent with the expected background from atmospheric muons and neutrinos. Upper limits are set on the dark matter annihilation rate, with conversions to limits on spin-dependent and spin-independent scattering cross sections of weakly interacting massive particles (WIMPs) on protons, for WIMP masses in the range 20-5000  GeV/c2. These are the most stringent spin-dependent WIMP-proton cross section limits to date above 35  GeV/c2 for most WIMP models.

Published
2013
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results