First results from the DarkSide-50 dark matter experiment at Laboratori Nazionali del Gran Sasso
| العنوان: | First results from the DarkSide-50 dark matter experiment at Laboratori Nazionali del Gran Sasso |
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| المؤلفون: | S. Kidner, R. Tartaglia, A. L. Renshaw, E. V. Hungerford, Yanchu Wang, P. Cavalcante, A. Candela, C. Zhu, M. Cariello, S. Westerdale, A. Sotnikov, Samuele Sangiorgio, E. Shields, N. Rossi, F. Gabriele, E. Pantic, L. Crippa, D. Sablone, An. Ianni, V. N. Muratova, G. Testera, M. D. Skorokhvatov, L. Grandi, G. Forster, A. Devoto, A. E. Chavarria, K. Pelczar, K. Fomenko, Cristiano Galbiati, M. Wada, C. Love, G. Di Pietro, Min-Xin Guan, R. B. Vogelaar, Laura Cadonati, L. Papp, Y. Guardincerri, Gioacchino Ranucci, E. Edkins, P. Musico, K. Herner, M. E. Monzani, S. D. Rountree, P. J. Mosteiro, B. Baldin, Hui Wang, R. Parsells, G. Bonfini, A. Pocar, Thomas Alexander, Y. Q. Ma, Fausto Ortica, B. Rossi, K. Randle, P. Saggese, L. Marini, M. Bossa, N. Canci, Paolo Lombardi, B. R. Hackett, A. Empl, R. Saldanha, K. Arisaka, Henning O. Back, Stuart Derek Walker, M. Montuschi, M. Orsini, E. Meroni, Jilei Xu, A. Zec, O. Smirnov, D. Franco, G. Fiorillo, A. Monte, M. Okounkova, G. Zuzel, Alan Watson, J. Yoo, C. L. Kendziora, F. Di Eusanio, A. Razeto, L. Pagani, M. D'Incecco, J. Tatarowicz, D. Korablev, M. De Deo, A. V. Derbin, Nicomede Pelliccia, I. N. Machulin, B. Reinhold, Anselmo Meregaglia, H. Qian, S. Davini, E. Segreto, A. Wright, C. J. Martoff, A. Mandarano, Marcin Wójcik, S. Luitz, Marco Pallavicini, D. D'Angelo, K. J. Keeter, Frank Calaprice, F. Budano, X. Xiang, Sandra Zavatarelli, P. X. Li, V. V. Kobychev, W. Sands, Aldo Romani, B. Loer, M. Gromov, A. Tonazzo, S. Pordes, P. Agnes, Al. Ianni, G. Koh, J. Maricic, A. Nelson, G. Korga, Stefano Maria Mari, R. Milincic, Cécile Jollet, D. A. Semenov, A. Kurlej, S. Parmeggiano, K. Biery, A. Fan, D. A. Pugachev, S. Perasso, A. G. Cocco, A. K. Alton, B. J. Mount, Chung-Yao Yang, Augusto Brigatti, D. Montanari, E. V. Unzhakov, J. Brodsky, H. Cao, S. Odrowski, Peter Daniel Meyers, Y. Suvorov, Livia Ludhova, A. M. Goretti, A. S. Chepurnov, C. Stanford |
| المساهمون: | Agnes, P, Alexander, T., Alton, A., Arisaka, K., Back, H. O., Baldin, B., Biery, K., Bonfini, G., Bossa, M., Brigatti, A., Brodsky, J., Budano, F., Cadonati, L., Calaprice, F., Canci, N., Candela, A., Cao, H., Cariello, M., Cavalcante, P., Chavarria, A., Chepurnov, A., Cocco, A. G., Crippa, L., D'Angelo, D., D'Incecco, M., Davini, S., De Deo, M., Derbin, A., Devoto, A., Di Eusanio, F., Di Pietro, G., Edkins, E., Empl, A., Fan, A., Fiorillo, Giuliana, Fomenko, K., Forster, G., Franco, D., Gabriele, F., Galbiati, C., Goretti, A., Grandi, L., Gromov, M., Guan, M. Y., Guardincerri, Y., Hackett, B., Herner, K., Hungerford, E. V., Ianni, A. l., Ianni, A. n., Jollet, C., Keeter, K., Kendziora, C., Kidner, S., Kobychev, V., Koh, G., Korablev, D., Korga, G., Kurlej, A., Li, P. X., Loer, B., Lombardi, P., Love, C., Ludhova, L., Luitz, S., Ma, Y. Q., Machulin, I., Mandarano, A., Mari, S., Maricic, J., Marini, L., Martoff, C. J., Meregaglia, A., Meroni, E., Meyers, P. D., Milincic, R., Montanari, D., Monte, A., Montuschi, M., Monzani, M. E., Mosteiro, P., Mount, B., Muratova, V., Musico, P., Nelson, A., Odrowski, S., Okounkova, M., Orsini, M., Ortica, F., Pagani, L., Pallavicini, M., Pantic, E., Papp, L., Parmeggiano, S., Parsells, R., Pelczar, K., Pelliccia, N., Perasso, S., Pocar, A., Pordes, S., Pugachev, D., Qian, H., Randle, K., Ranucci, G., Razeto, A., Reinhold, B., Renshaw, A., Romani, A., Rossi, B., Rossi, N., Rountree, S. D., Sablone, D., Saggese, P., Saldanha, R., Sands, W., Sangiorgio, S., Segreto, E., Semenov, D., Shields, E., Skorokhvatov, M., Smirnov, O., Sotnikov, A., Stanford, C., Suvorov, Y., Tartaglia, R., Tatarowicz, J., Testera, G., Tonazzo, A., Unzhakov, E., Vogelaar, R. B., Wada, M., Walker, Susan Elizabeth, Wang, H., Wang, Y., Watson, A., Westerdale, S., Wojcik, M., Wright, A., Xiang, X., Xu, J., Yang, C. G., Yoo, J., Zavatarelli, S., Zec, A., Zhu, C., Zuzel, G., P. Agnes, Mari, Stefano Maria, The Darkside, Collaboration |
| المصدر: | Physics Letters B, Vol 743, Iss, Pp 456-466 (2015) Physics Letters ResearcherID |
| بيانات النشر: | Elsevier BV, 2015. |
| سنة النشر: | 2015 |
| مصطلحات موضوعية: | Nuclear and High Energy Physics, Particle physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Liquid scintillator, Physics - Instrumentation and Detectors, WIMP, Physics::Instrumentation and Detectors, low-background detectors, Dark matter, Noble liquid detectors, FOS: Physical sciences, liquid scintillators, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, WIMP Argon Programme, 01 natural sciences, dark matter, High Energy Physics - Experiment, Nuclear physics, High Energy Physics - Experiment (hep-ex), Low-background detectors, 0103 physical sciences, Nuclear Experiment, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, ICARUS, Time projection chamber, 010308 nuclear & particles physics, Liquid scintillators, Dark matter WIMP Noble liquid detectors Low-background detectors Liquid scintillators, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), Low-background detector, noble liquid detectors, lcsh:QC1-999, DAMA/NaI, Weakly interacting massive particles, High Energy Physics::Experiment, Noble liquid detector, Astrophysics - Instrumentation and Methods for Astrophysics, lcsh:Physics, Astrophysics - Cosmology and Nongalactic Astrophysics |
| الوصف: | We report the first results of DarkSide-50, a direct search for dark matter operating in the underground Laboratori Nazionali del Gran Sasso (LNGS) and searching for the rare nuclear recoils possibly induced by weakly interacting massive particles (WIMPs). The dark matter detector is a Liquid Argon Time Projection Chamber with a (46.4+-0.7) kg active mass, operated inside a 30 t organic liquid scintillator neutron veto, which is in turn installed at the center of a 1 kt water Cherenkov veto for the residual flux of cosmic rays. We report here the null results of a dark matter search for a (1422+-67) kg d exposure with an atmospheric argon fill. This is the most sensitive dark matter search performed with an argon target, corresponding to a 90% CL upper limit on the WIMP-nucleon spin-independent cross section of 6.1x10^-44 cm^2 for a WIMP mass of 100 GeV/c^2. 26 pages, 7 figures; updated figures and references, notably Fig. 7 has updated CDMSII curve; fixed typos; clarified some language and figures; updated references |
| تدمد: | 0370-2693 |
| الوصول الحر: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6bc95457db1b7a7a778d32a926d85c9cTest https://doi.org/10.1016/j.physletb.2015.03.012Test |
| حقوق: | OPEN |
| رقم الانضمام: | edsair.doi.dedup.....6bc95457db1b7a7a778d32a926d85c9c |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 03702693 |
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