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Search for dark matter annual modulation with DarkSide-50

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arxiv 2307.07249 v2 pith:EYBPIKA2 submitted 2023-07-14 hep-ex astro-ph.CO

The DarkSide-50 Collaboration: P. Agnes , I.F.M. Albuquerque , T. Alexander , A.K. Alton , M. Ave , H.O. Back , G. Batignani , K. Biery
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V. Bocci W.M. Bonivento B. Bottino S. Bussino M. Cadeddu M. Cadoni F. Calaprice A. Caminata M.D. Campos N. Canci M. Caravati N. Cargioli M. Cariello M. Carlini V. Cataudella P. Cavalcante S. Cavuoti S. Chashin A. Chepurnov C. Cicalò G. Covone D. D'Angelo S. Davini A. De Candia S. De Cecco G. De Filippis G. De Rosa A.V. Derbin A. Devoto M. D'Incecco C. Dionisi F. Dordei M. Downing D. D'Urso M. Fairbairn G. Fiorillo D. Franco F. Gabriele C. Galbiati C. Ghiano C. Giganti G.K. Giovanetti A.M. Goretti G. Grilli di Cortona A. Grobov M. Gromov M. Guan M. Gulino B.R. Hackett K. Herner T. Hessel B. Hosseini F. Hubaut T. Hugues E.V. Hungerford An. Ianni V. Ippolito K. Keeter C.L. Kendziora M. Kimura I. Kochanek D. Korablev G. Korga A. Kubankin M. Kuss M. Kuźniak M. La Commara M. Lai X. Li M. Lissia G. Longo O. Lychagina I.N. Machulin L.P. Mapelli S.M. Mari J. Maricic A. Messina R. Milincic J. Monroe M. Morrocchi X. Mougeot V.N. Muratova P. Musico A.O. Nozdrina A. Oleinik F. Ortica L. Pagani M. Pallavicini L. Pandola E. Pantic E. Paoloni K. Pelczar N. Pelliccia S. Piacentini A. Pocar D.M. Poehlmann S. Pordes S.S. Poudel P. Pralavorio D.D. Price F. Ragusa M. Razeti A. Razeto A.L. Renshaw M. Rescigno J. Rode A. Romani D. Sablone O. Samoylov E. Sandford W. Sands S. Sanfilippo C. Savarese B. Schlitzer D.A. Semenov A. Shchagin A. Sheshukov M.D. Skorokhvatov O. Smirnov A. Sotnikov S. Stracka Y. Suvorov R. Tartaglia G. Testera A. Tonazzo E.V. Unzhakov A. Vishneva R.B. Vogelaar M. Wada H. Wang Y. Wang S. Westerdale M.M. Wojcik X. Xiao C. Yang G. Zuzel
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classification hep-exastro-ph.CO
keywords darkmattermodulationannualdarkside-50searchsignatureabove
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abstract

Dark matter induced event rate in an Earth-based detector 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 $40~{\rm eV_{ee}}$, the lowest threshold ever achieved in such a search.

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Cited by 1 Pith paper

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  1. Uncertainties in tellurium-based dark matter searches stemming from nuclear structure uncertainties

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Nuclear shell-model uncertainties cause over 100% uncertainties on some tellurium-based dark matter coupling limits, comparable to xenon, while leaving the annual modulation phase unchanged.

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