Search for dark matter annual modulation with DarkSide-50

Dark matter may induce an event in an Earth-based detector, and its event rate is predicted to show an annual modulation as a result of the Earth’s orbital motion around the Sun. We searched for this modulation signature using the ionization signal of the DarkSide-50 liquid argon time projection chamber. No significant signature compatible with dark matter is observed in the electron recoil equivalent energy range above <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mn>40</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:msub><a:mi>eV</a:mi><a:mrow><a:mi>ee</a:mi></a:mrow></a:msub></a:mrow></a:math>, the lowest threshold ever achieved in such a search. Published by the American Physical Society 2024

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2024-11-21
DOI
https://doi.org/10.1103/physrevd.110.102006
Citations
4
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
2.64

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article

Search for dark matter annual modulation with DarkSide-50

C. Ghiano, M. Cadeddu, M. Morrocchi, M. Kuss et al.
4 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
2.64
article

Search for dark matter annual modulation with DarkSide-50

C. Ghiano, M. Cadeddu, M. Morrocchi, M. Kuss, G. Fiorillo, A. Sheshukov, K. Herner, M. Gulino, P. Cavalcante, K. Keeter, M. D. Campos, F. Ragusa, S. Piacentini, A. Oleinik, A. Romani, I. F. M. Albuquerque, A. K. Alton, S. De Cecco, V. Cataudella, V. N. Muratova, O. Lychagina, S. Chashin, G. De Filippis, V. Bocci, D. D’Angelo, M. Ave, S. Cavuoti, M. Caravati, X. Li, S. Sanfilippo, P. Agnes, I. Kochanek, W. Bonivento, A. Grobov, H. O. Back, M. La Commara, C. Galbiati, Giovanni Grilli di Cortona, O. Samoylov, V. Ippolito, A. Caminata, Xiang Xiao, A. Sotnikov, S. S. Poudel, A. Oleinik, C. Cicalò, C. Dionisi, A. V. Derbin, D. Franco, A. Pocar, A. Razeto, X. Mougeot, M. Pallavicini, B. Hosseini, F. Dordei, M. Wada, A. Devoto, A Kubankin, D. M. Poehlmann, S. Stracka, A. De Candia, N. Pelliccia, J. Maricic, G. Covone, D. D’Urso, Malcolm Fairbairn, R. Tartaglia, P. Pralavorio, A. Chepurnov, B. Bottino, Masato Kimura, D. Price, N. Cargioli, T. Alexander, F. Ortica, M. Lissia, M. Kuźniak, M. Cadoni, L. Pandola, T. Hessel, N. Canci, M. Downing, F. Gabriele, F. Calaprice, A. Messina, H. Wang, T. Hugues, G. Korga, G. Batignani, K. Pelczar, S. Westerdale, C. Savarese, E. Sandford, I. N. Machulin, M. Carlini, M. D. Skorokhvatov, E. Paoloni, M. Cariello, W. Sands, Y. Wang, E. Unzhakov, J. Rode, A. L. Renshaw, A. Sheshukov, O. Samoylov, S. Bussino, C. Kendziora, C. Giganti, M. Gromov, M. Razeti, M. Guan, M. D’Incecco, G. Zuzel, B. Schlitzer, A. Vishneva, Д. А. Семенов, S. M. Mari, Y. Suvorov, E. Hungerford, An. Ianni, G. Longo, G. De Rosa, S. Davini, L. Pagani, R. B. Vogelaar, G. Zuzel, A. Tonazzo, G. K. Giovanetti, G. Testera, L. Pandola, K. Biery, M. Lai, O. Smirnov, B. R. Hackett, D. Korablev, J. Monroe, S. M. Mari, V. N. Muratova, S. Pordes, M. Rescigno, T. Miletic, Fabrice Hubaut
article en
4 citations

Abstract

Dark matter may induce an event in an Earth-based detector, and its event rate is predicted to show an annual modulation as a result of the Earth’s orbital motion around the Sun. We searched for this modulation signature using the ionization signal of the DarkSide-50 liquid argon time projection chamber. No significant signature compatible with dark matter is observed in the electron recoil equivalent energy range above <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mn>40</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:msub><a:mi>eV</a:mi><a:mrow><a:mi>ee</a:mi></a:mrow></a:msub></a:mrow></a:math>, the lowest threshold ever achieved in such a search. Published by the American Physical Society 2024

Physical review. D/Physical review. D.Vol. 110(10)
Roma Tre University (IT), Belgorod National Research University (RU), Jagiellonian University (PL), Fermi National Accelerator Laboratory (US), Pacific Northwest National Laboratory (US), Augustana University (US), University of Sassari (IT), King's College - North Carolina (US), University of Cagliari (IT), Universidade de São Paulo (BR), King's College London (GB), Royal Holloway University of London (GB), University of Milan (IT), Lomonosov Moscow State University (RU), Princeton University (US), Université Paris Cité (FR), Aix-Marseille Université (FR), Università degli Studi di Enna Kore (IT), University of Hawaii–West Oahu (US), Commissariat à l'Énergie Atomique et aux Énergies Alternatives (FR), University of Perugia (IT), Université Paris-Saclay (FR), Kurchatov Institute (RU), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso (IT), University of California System (US), University of Manchester (GB), Joint Institute for Nuclear Research (RU), Sorbonne Université (FR), Laboratoire d'Intégration des Systèmes et des Technologies (FR), Centre de physique des particules de Marseille (FR), Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (IT), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Genova (IT), Fondazione Stella Maris (IT), Petersburg Nuclear Physics Institute (RU), Istituto Nazionale di Fisica Nucleare, Sezione di Milano (IT), Nicolaus Copernicus Astronomical Center (PL), Laboratoire National Henri Becquerel (FR), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati (IT), Moscow State University (TJ), Gran Sasso Science Institute (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Roma I (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Pisa (IT), Istituto Nazionale di Fisica Nucleare, Sezione di Perugia (IT), Laboratoire Médiations (FR), University of Houston (US), University of Naples Federico II (IT), Black Hills State University (US), University of Genoa (IT), Virginia Tech (US), Sapienza University of Rome (IT), National Research Nuclear University MEPhI (RU), Polish Academy of Sciences (PL)
National Science Foundation, U.S. Department of Energy, Istituto Nazionale di Fisica Nucleare Sezione di Padova, European Commission, Agence Nationale de la Recherche, Fundação de Amparo à Pesquisa do Estado de São Paulo, Fundacja na rzecz Nauki Polskiej, Ministry of Education and Science of the Russian Federation, Conselho Nacional de Desenvolvimento Científico e Tecnológico, Narodowe Centrum Nauki, Narodowym Centrum Nauki, Ministerstwo Edukacji i Nauki, Istituto Nazionale di Fisica Nucleare, Office of Science, Horizon 2020 Framework Programme, Science and Technology Facilities Council, European Regional Development Fund, Labex UnivEarthS, Institut National de Physique Nucléaire et de Physique des Particules, Nuclear Physics, Fermilab, European Metrology Programme for Innovation and Research
Openalex Percentile: Top 7%
Dark Matter and Cosmic Phenomena
2.64
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