Search

Your search keyword '"C Weinheimer"' showing total 6 results
Start Over Author "C Weinheimer" Publication Year Range This year
6 results on '"C Weinheimer"'

1. The XENONnT dark matter experiment

Author

XENON Collaboration, E. Aprile, J. Aalbers, K. Abe, S. Ahmed Maouloud, L. Althueser, B. Andrieu, E. Angelino, J. R. Angevaare, V. C. Antochi, D. Antón Martin, F. Arneodo, M. Balata, L. Baudis, A. L. Baxter, M. Bazyk, L. Bellagamba, R. Biondi, A. Bismark, E. J. Brookes, A. Brown, S. Bruenner, G. Bruno, R. Budnik, T. K. Bui, C. Cai, J. M. R. Cardoso, F. Cassese, A. Chiarini, D. Cichon, A. P. Cimental Chavez, A. P. Colijn, J. Conrad, R. Corrieri, J. J. Cuenca-García, J. P. Cussonneau, O. Dadoun, V. D’Andrea, M. P. Decowski, B. De Fazio, P. Di Gangi, S. Diglio, J. M. Disdier, D. Douillet, K. Eitel, A. Elykov, S. Farrell, A. D. Ferella, C. Ferrari, H. Fischer, M. Flierman, S. Form, D. Front, W. Fulgione, C. Fuselli, P. Gaemers, R. Gaior, A. Gallo Rosso, M. Galloway, F. Gao, R. Gardner, N. Garroum, R. Glade-Beucke, L. Grandi, J. Grigat, H. Guan, M. Guerzoni, M. Guida, R. Hammann, A. Higuera, C. Hils, L. Hoetzsch, N. F. Hood, J. Howlett, C. Huhmann, M. Iacovacci, G. Iaquaniello, L. Iven, Y. Itow, J. Jakob, F. Joerg, A. Joy, M. Kara, P. Kavrigin, S. Kazama, M. Kobayashi, G. Koltman, A. Kopec, F. Kuger, H. Landsman, R. F. Lang, L. Levinson, I. Li, S. Li, S. Liang, S. Lindemann, M. Lindner, K. Liu, J. Loizeau, F. Lombardi, J. Long, J. A. M. Lopes, Y. Ma, C. Macolino, J. Mahlstedt, A. Mancuso, L. Manenti, F. Marignetti, T. Marrodán Undagoitia, P. Martella, K. Martens, J. Masbou, D. Masson, E. Masson, S. Mastroianni, E. Mele, M. Messina, R. Michinelli, K. Miuchi, A. Molinario, S. Moriyama, K. Morå, Y. Mosbacher, M. Murra, J. Müller, K. Ni, S. Nisi, U. Oberlack, D. Orlandi, R. Othegraven, B. Paetsch, J. Palacio, S. Parlati, P. Paschos, Q. Pellegrini, R. Peres, C. Peters, J. Pienaar, M. Pierre, G. Plante, T. R. Pollmann, J. Qi, J. Qin, D. Ramírez García, M. Rynge, J. Shi, R. Singh, L. Sanchez, J. M. F. dos Santos, I. Sarnoff, G. Sartorelli, J. Schreiner, D. Schulte, P. Schulte, H. Schulze Eißing, M. Schumann, L. Scotto Lavina, M. Selvi, F. Semeria, P. Shagin, S. Shi, E. Shockley, M. Silva, H. Simgen, J. Stephen, M. Stern, B. K. Stillwell, A. Takeda, P.-L. Tan, D. Tatananni, A. Terliuk, D. Thers, F. Toschi, G. Trinchero, C. Tunnell, F. Tönnies, K. Valerius, G. Volta, C. Weinheimer, M. Weiss, D. Wenz, J. Westermann, C. Wittweg, T. Wolf, V. H. S. Wu, Y. Xing, D. Xu, Z. Xu, M. Yamashita, L. Yang, J. Ye, L. Yuan, G. Zavattini, M. Zhong, and T. Zhu

Subjects
Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract The multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter with two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in the program, planned to be an upgrade of its predecessor XENON1T. It features an active target of 5.9 tonnes of cryogenic liquid xenon (8.5 tonnes total mass in cryostat). The experiment is expected to extend the sensitivity to WIMP dark matter by more than an order of magnitude compared to XENON1T, thanks to the larger active mass and the significantly reduced background, improved by novel systems such as a radon removal plant and a neutron veto. This article describes the XENONnT experiment and its sub-systems in detail and reports on the detector performance during the first science run.

Published
2024
Full Text
View/download PDF

2. Improved treatment of the T $$_2$$ 2 molecular final-states uncertainties for the KATRIN neutrino-mass measurement

Author

S. Schneidewind, J. Schürmann, A. Lokhov, C. Weinheimer, and A. Saenz

Subjects
Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract The KArlsruhe TRItium Neutrino experiment (KATRIN) aims to determine the effective mass of the electron antineutrino via a high-precision measurement of the tritium $$\upbeta $$ β -decay spectrum in its end-point region. The target neutrino-mass sensitivity of $${0.2}~\text {eV}/\text {c}^2$$ 0.2 eV / c 2 at 90% CL can only be achieved in the case of high statistics and good control of the systematic uncertainties. One key systematic effect originates from the calculation of the molecular final states of T $$_2$$ 2 $$\upbeta $$ β decay. In the first neutrino-mass analyses of KATRIN the contribution of the uncertainty of the molecular final-states distribution (FSD) was estimated via a conservative phenomenological approach to be $$2 \times 10^{-2}~\text {eV}^{2}/\text {c}^{4}.$$ 2 × 10 - 2 eV 2 / c 4 . In this work a new procedure is presented for estimating the FSD-related uncertainties by considering the details of the final-states calculation, i.e. the uncertainties of constants, parameters, and functions used in the calculation as well as its convergence itself as a function of the basis-set size used in expanding the molecular wave functions. The calculated uncertainties are directly propagated into the experimental observable, the squared neutrino mass $$m_\nu ^2,$$ m ν 2 , and thus have to be determined individually for each experimental configuration. For the experimental conditions of the first KATRIN measurement campaign the new procedure is presented in detail, allowing for the application of this procedure to other experiments. This specific calculation leads to a constraint of the FSD-related uncertainty of $$1.3 \times 10^{-3}~\text {eV}^{2}/\text {c}^{4},$$ 1.3 × 10 - 3 eV 2 / c 4 , well below the design limit of $$7.5 \times 10^{-3}~\text {eV}^{2}/\text {c}^{4}$$ 7.5 × 10 - 3 eV 2 / c 4 for any individual systematic contribution.

Published
2024
Full Text
View/download PDF

3. Cosmogenic background simulations for neutrinoless double beta decay with the DARWIN observatory at various underground sites

Author

DARWIN Collaboration, M. Adrover, L. Althueser, B. Andrieu, E. Angelino, J. R. Angevaare, B. Antunovic, E. Aprile, M. Babicz, D. Bajpai, E. Barberio, L. Baudis, M. Bazyk, N. Bell, L. Bellagamba, R. Biondi, Y. Biondi, A. Bismark, C. Boehm, A. Breskin, E. J. Brookes, A. Brown, G. Bruno, R. Budnik, C. Capelli, J. M. R. Cardoso, A. Chauvin, A. P. Cimental Chavez, A. P. Colijn, J. Conrad, J. J. Cuenca-García, V. D’Andrea, M. P. Decowski, A. Deisting, P. Di Gangi, S. Diglio, M. Doerenkamp, G. Drexlin, K. Eitel, A. Elykov, R. Engel, S. Farrell, A. D. Ferella, C. Ferrari, H. Fischer, M. Flierman, W. Fulgione, P. Gaemers, R. Gaior, M. Galloway, N. Garroum, S. Ghosh, F. Girard, R. Glade-Beucke, F. Glück, L. Grandi, J. Grigat, R. Größle, H. Guan, M. Guida, R. Hammann, V. Hannen, S. Hansmann-Menzemer, N. Hargittai, T. Hasegawa, C. Hils, A. Higuera, K. Hiraoka, L. Hoetzsch, M. Iacovacci, Y. Itow, J. Jakob, F. Jörg, M. Kara, P. Kavrigin, S. Kazama, M. Keller, B. Kilminster, M. Kleifges, M. Kobayashi, A. Kopec, B. von Krosigk, F. Kuger, H. Landsman, R. F. Lang, I. Li, S. Li, S. Liang, S. Lindemann, M. Lindner, F. Lombardi, J. Loizeau, T. Luce, Y. Ma, C. Macolino, J. Mahlstedt, A. Mancuso, T. Marrodán Undagoitia, J. A. M. Lopes, F. Marignetti, K. Martens, J. Masbou, S. Mastroianni, S. Milutinovic, K. Miuchi, R. Miyata, A. Molinario, C. M. B. Monteiro, K. Morå, E. Morteau, Y. Mosbacher, J. Müller, M. Murra, J. L. Newstead, K. Ni, U. G. Oberlack, I. Ostrovskiy, B. Paetsch, M. Pandurovic, Q. Pellegrini, R. Peres, J. Pienaar, M. Pierre, M. Piotter, G. Plante, T. R. Pollmann, L. Principe, J. Qi, J. Qin, M. Rajado Silva, D. Ramírez García, A. Razeto, S. Sakamoto, L. Sanchez, P. Sanchez-Lucas, J. M. F. dos Santos, G. Sartorelli, A. Scaffidi, P. Schulte, H.-C. Schultz-Coulon, H. Schulze Eißing, M. Schumann, L. Scotto Lavina, M. Selvi, F. Semeria, P. Shagin, S. Sharma, W. Shen, M. Silva, H. Simgen, R. Singh, M. Solmaz, O. Stanley, M. Steidl, P.-L. Tan, A. Terliuk, D. Thers, T. Thümmler, F. Tönnies, F. Toschi, G. Trinchero, R. Trotta, C. Tunnell, P. Urquijo, K. Valerius, S. Vecchi, S. Vetter, G. Volta, D. Vorkapic, W. Wang, K. M. Weerman, C. Weinheimer, M. Weiss, D. Wenz, C. Wittweg, J. Wolf, T. Wolf, V. H. S. Wu, M. Wurm, Y. Xing, M. Yamashita, J. Ye, G. Zavattini, and K. Zuber

Subjects
Astrophysics, QB460-466, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract Xenon dual-phase time projections chambers (TPCs) have proven to be a successful technology in studying physical phenomena that require low-background conditions. With $$40\,\textrm{t}$$ 40 t of liquid xenon (LXe) in the TPC baseline design, DARWIN will have a high sensitivity for the detection of particle dark matter, neutrinoless double beta decay ( $$0\upnu \upbeta \upbeta $$ 0 ν β β ), and axion-like particles (ALPs). Although cosmic muons are a source of background that cannot be entirely eliminated, they may be greatly diminished by placing the detector deep underground. In this study, we used Monte Carlo simulations to model the cosmogenic background expected for the DARWIN observatory at four underground laboratories: Laboratori Nazionali del Gran Sasso (LNGS), Sanford Underground Research Facility (SURF), Laboratoire Souterrain de Modane (LSM) and SNOLAB. We present here the results of simulations performed to determine the production rate of $${}^{137}$$ 137 Xe, the most crucial isotope in the search for $$0\upnu \upbeta \upbeta $$ 0 ν β β of $${}^{136}$$ 136 Xe. Additionally, we explore the contribution that other muon-induced spallation products, such as other unstable xenon isotopes and tritium, may have on the cosmogenic background.

Published
2024
Full Text
View/download PDF

4. First Indication of Solar ^{8}B Neutrinos via Coherent Elastic Neutrino-Nucleus Scattering with XENONnT.

Author

Aprile E, Aalbers J, Abe K, Ahmed Maouloud S, Althueser L, Andrieu B, Angelino E, Antón Martin D, Arneodo F, Baudis L, Bazyk M, Bellagamba L, Biondi R, Bismark A, Boese K, Brown A, Bruno G, Budnik R, Cai C, Capelli C, Cardoso JMR, Cimental Chávez AP, Colijn AP, Conrad J, Cuenca-García JJ, D'Andrea V, Daniel Garcia LC, Decowski MP, Deisting A, Di Donato C, Di Gangi P, Diglio S, Eitel K, Elykov A, Ferella AD, Ferrari C, Fischer H, Flehmke T, Flierman M, Fulgione W, Fuselli C, Gaemers P, Gaior R, Galloway M, Gao F, Ghosh S, Giacomobono R, Glade-Beucke R, Grandi L, Grigat J, Guan H, Guida M, Gyorgy P, Hammann R, Higuera A, Hils C, Hoetzsch L, Hood NF, Iacovacci M, Itow Y, Jakob J, Joerg F, Kaminaga Y, Kara M, Kavrigin P, Kazama S, Kobayashi M, Koke D, Kopec A, Kuger F, Landsman H, Lang RF, Levinson L, Li I, Li S, Liang S, Lin YT, Lindemann S, Lindner M, Liu K, Liu M, Loizeau J, Lombardi F, Long J, Lopes JAM, Luce T, Ma Y, Macolino C, Mahlstedt J, Mancuso A, Manenti L, Marignetti F, Marrodán Undagoitia T, Martens K, Masbou J, Masson E, Mastroianni S, Melchiorre A, Merz J, Messina M, Michael A, Miuchi K, Molinario A, Moriyama S, Morå K, Mosbacher Y, Murra M, Müller J, Ni K, Oberlack U, Paetsch B, Pan Y, Pellegrini Q, Peres R, Peters C, Pienaar J, Pierre M, Plante G, Pollmann TR, Principe L, Qi J, Qin J, Ramírez García D, Rajado M, Singh R, Sanchez L, Dos Santos JMF, Sarnoff I, Sartorelli G, Schreiner J, Schulte P, Schulze Eißing H, Schumann M, Scotto Lavina L, Selvi M, Semeria F, Shagin P, Shi S, Shi J, Silva M, Simgen H, Takeda A, Tan PL, Thers D, Toschi F, Trinchero G, Tunnell CD, Tönnies F, Valerius K, Vecchi S, Vetter S, Villazon Solar FI, Volta G, Weinheimer C, Weiss M, Wenz D, Wittweg C, Wu VHS, Xing Y, Xu D, Xu Z, Yamashita M, Yang L, Ye J, Yuan L, Zavattini G, and Zhong M

Abstract

We present the first measurement of nuclear recoils from solar ^{8}B neutrinos via coherent elastic neutrino-nucleus scattering with the XENONnT dark matter experiment. The central detector of XENONnT is a low-background, two-phase time projection chamber with a 5.9 t sensitive liquid xenon target. A blind analysis with an exposure of 3.51  t×yr resulted in 37 observed events above 0.5 keV, with (26.4_{-1.3}^{+1.4}) events expected from backgrounds. The background-only hypothesis is rejected with a statistical significance of 2.73σ. The measured ^{8}B solar neutrino flux of (4.7_{-2.3}^{+3.6})×10^{6}  cm^{-2} s^{-1} is consistent with results from the Sudbury Neutrino Observatory. The measured neutrino flux-weighted CEνNS cross section on Xe of (1.1_{-0.5}^{+0.8})×10^{-39}  cm^{2} is consistent with the Standard Model prediction. This is the first direct measurement of nuclear recoils from solar neutrinos with a dark matter detector.

Published
2024
Full Text
View/download PDF

5. In chronic kidney disease altered cardiac metabolism precedes cardiac hypertrophy.

Author

Williams MJ, Halabi CM, Patel HM, Joseph Z, McCommis K, Weinheimer C, Kovacs A, Lima F, Finck B, Malluche H, and Hruska KA

Subjects
Animals, Disease Models, Animal, Activins metabolism, Activins genetics, Mitochondria, Heart metabolism, Mitochondria, Heart pathology, Mice, Male, Oxidative Phosphorylation, Nephritis, Hereditary metabolism, Nephritis, Hereditary pathology, Nephritis, Hereditary genetics, Fibroblast Growth Factors metabolism, Fibroblast Growth Factors genetics, Parathyroid Hormone metabolism, Fibroblast Growth Factor-23 metabolism, Renal Insufficiency, Chronic metabolism, Renal Insufficiency, Chronic pathology, Cardiomegaly metabolism, Cardiomegaly pathology, Myocardium metabolism, Myocardium pathology
Abstract

Conduit arterial disease in chronic kidney disease (CKD) is an important cause of cardiac complications. Cardiac function in CKD has not been studied in the absence of arterial disease. In an Alport syndrome model bred not to have conduit arterial disease, mice at 225 days of life (dol) had CKD equivalent to humans with CKD stage 4-5. Parathyroid hormone (PTH) and FGF23 levels were one log order elevated, circulating sclerostin was elevated, and renal activin A was strongly induced. Aortic Ca levels were not increased, and vascular smooth muscle cell (VSMC) transdifferentiation was absent. The CKD mice were not hypertensive, and cardiac hypertrophy was absent. Freshly excised cardiac tissue respirometry (Oroboros) showed that ADP-stimulated O 2 flux was diminished from 52 to 22 pmol/mg ( P = 0.022). RNA-Seq of cardiac tissue from CKD mice revealed significantly decreased levels of cardiac mitochondrial oxidative phosphorylation genes. To examine the effect of activin A signaling, some Alport mice were treated with a monoclonal Ab to activin A or an isotype-matched IgG beginning at 75 days of life until euthanasia. Treatment with the activin A antibody (Ab) did not affect cardiac oxidative phosphorylation. However, the activin A antibody was active in the skeleton, disrupting the effect of CKD to stimulate osteoclast number, eroded surfaces, and the stimulation of osteoclast-driven remodeling. The data reported here show that cardiac mitochondrial respiration is impaired in CKD in the absence of conduit arterial disease. This is the first report of the direct effect of CKD on cardiac respiration. NEW & NOTEWORTHY Heart disease is an important morbidity of chronic kidney disease (CKD). Hypertension, vascular stiffness, and vascular calcification all contribute to cardiac pathophysiology. However, cardiac function in CKD devoid of vascular disease has not been studied. Here, in an animal model of human CKD without conduit arterial disease, we analyze cardiac respiration and discover that CKD directly impairs cardiac mitochondrial function by decreasing oxidative phosphorylation. Protection of cardiac oxidative phosphorylation may be a therapeutic target in CKD.

Published
2024
Full Text
View/download PDF

6. The XENONnT dark matter experiment.

Author

Aprile E, Aalbers J, Abe K, Ahmed Maouloud S, Althueser L, Andrieu B, Angelino E, Angevaare JR, Antochi VC, Antón Martin D, Arneodo F, Balata M, Baudis L, Baxter AL, Bazyk M, Bellagamba L, Biondi R, Bismark A, Brookes EJ, Brown A, Bruenner S, Bruno G, Budnik R, Bui TK, Cai C, Cardoso JMR, Cassese F, Chiarini A, Cichon D, Cimental Chavez AP, Colijn AP, Conrad J, Corrieri R, Cuenca-García JJ, Cussonneau JP, Dadoun O, D'Andrea V, Decowski MP, De Fazio B, Gangi PD, Diglio S, Disdier JM, Douillet D, Eitel K, Elykov A, Farrell S, Ferella AD, Ferrari C, Fischer H, Flierman M, Form S, Front D, Fulgione W, Fuselli C, Gaemers P, Gaior R, Rosso AG, Galloway M, Gao F, Gardner R, Garroum N, Glade-Beucke R, Grandi L, Grigat J, Guan H, Guerzoni M, Guida M, Hammann R, Higuera A, Hils C, Hoetzsch L, Hood NF, Howlett J, Huhmann C, Iacovacci M, Iaquaniello G, Iven L, Itow Y, Jakob J, Joerg F, Joy A, Kara M, Kavrigin P, Kazama S, Kobayashi M, Koltman G, Kopec A, Kuger F, Landsman H, Lang RF, Levinson L, Li I, Li S, Liang S, Lindemann S, Lindner M, Liu K, Loizeau J, Lombardi F, Long J, Lopes JAM, Ma Y, Macolino C, Mahlstedt J, Mancuso A, Manenti L, Marignetti F, Marrodán Undagoitia T, Martella P, Martens K, Masbou J, Masson D, Masson E, Mastroianni S, Mele E, Messina M, Michinelli R, Miuchi K, Molinario A, Moriyama S, Morå K, Mosbacher Y, Murra M, Müller J, Ni K, Nisi S, Oberlack U, Orlandi D, Othegraven R, Paetsch B, Palacio J, Parlati S, Paschos P, Pellegrini Q, Peres R, Peters C, Pienaar J, Pierre M, Plante G, Pollmann TR, Qi J, Qin J, García DR, Rynge M, Shi J, Singh R, Sanchez L, Santos JMFD, Sarnoff I, Sartorelli G, Schreiner J, Schulte D, Schulte P, Schulze Eißing H, Schumann M, Scotto Lavina L, Selvi M, Semeria F, Shagin P, Shi S, Shockley E, Silva M, Simgen H, Stephen J, Stern M, Stillwell BK, Takeda A, Tan PL, Tatananni D, Terliuk A, Thers D, Toschi F, Trinchero G, Tunnell C, Tönnies F, Valerius K, Volta G, Weinheimer C, Weiss M, Wenz D, Westermann J, Wittweg C, Wolf T, Wu VHS, Xing Y, Xu D, Xu Z, Yamashita M, Yang L, Ye J, Yuan L, Zavattini G, Zhong M, and Zhu T

Abstract

The multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter with two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in the program, planned to be an upgrade of its predecessor XENON1T. It features an active target of 5.9 tonnes of cryogenic liquid xenon (8.5 tonnes total mass in cryostat). The experiment is expected to extend the sensitivity to WIMP dark matter by more than an order of magnitude compared to XENON1T, thanks to the larger active mass and the significantly reduced background, improved by novel systems such as a radon removal plant and a neutron veto. This article describes the XENONnT experiment and its sub-systems in detail and reports on the detector performance during the first science run., (© The Author(s) 2024.)

Published
2024
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results