Sensitivity Projections for a Dual-Phase Argon TPC Optimized for Light Dark Matter Searches Through the Ionization Channel

P. Agnes,I Ahmad,S. Albergo,I. F. M. Albuquerque,T. Alexander,A. K. Alton,P. Amaudruz,M. Atzori Corona,D. J. Auty,M. Ave,I. Ch. Avetisov,R. I. Avetisov,O. Azzolini,H. O. Back,Z. Balmforth,V. Barbarian,A. Barrado Olmedo,P. Barrillon,A. Basco,G. Batignani, E. Berzin,A. Bondar,W. M. Bonivento,E. Borisova,B. Bottino,M. G. Boulay,G. Buccino,S. Bussino,J. Busto,A. Buzulutskov,M. Cadeddu,M. Cadoni,A. Caminata,N. Canci,A. Capra,S. Caprioli,M. Caravati,M. Cardenas-Montes,N. Cargioli,M. Carlini,P. Castello,V. Cataudella,P. Cavalcante,S. Cavuoti,S. Cebrian,J. M. Cela Ruiz,S. Chashin,A. Chepurnov,E. Chyhyrynets,C. Cicalo,L. Cifarelli,D. Cintas,V. Cocco,E. Conde Vilda,L. Consiglio,S. Copello,G. Covone, S. Cross,M. Czubak,M. D'Aniello,S. D'Auria,M. D. Da Rocha Rolo,O. Dadoun,M. Daniel,S. Davini,A. De Candia,S. De Cecco,A. De Falco,G. De Filippis,D. De Gruttola,S. De Pasquale,G. De Rosa,G. Dellacasa,A. V. Derbin,A. Devoto,F. Di Capua,L. Di Noto,P. Di Stefano, C. Dionisi,G. Dolganov,F. Dordei,L. Doria,T. Erjavec, M. Fernandez Diaz,G. Fiorillo,A. Franceschi,P. Franchini,D. Franco,E. Frolov,N. Funicello,F. Gabriele,D. Gahan,C. Galbiati,G. Gallina,G. Gallus,M. Garbini,P. Garcia Abia,A. Gendotti,C. Ghiano,R. A. Giampaolo,C. Giganti,M. A. Giorgi,G. K. Giovanetti,V. Goicoechea Casanueva,A. Gola, D. Gorman,R. Graciani Diaz,G. Grauso,G. Grilli Di Cortona,A. Grobov,M. Gromov,M. Guan,M. Guerzoni,M. Gulino,C. Guo,B. R. Hackett, J. B. Hall,A. L. Hallin,A. Hamer, H. Helton,M. Haranczyk,T. Hessel,S. Hill,S. Horikawa,F. Hubaut,T. Hugues,E. V. Hungerford,An. Ianni,V. Ippolito, C. Jillings,P. Kachru,A. A. Kemp,C. L. Kendziora,G. Keppel,A. V. Khomyakov,M. Kimura,I. Kochanek,K. Kondo, G. Korga,S. Koulosousas,A. Kubankin,M. Kuss,M. Kuzniak,M. La Commara,M. Lai,E. Le Guirriec,E. Leason,X. Li,L. Lidey,J. Lipp,M. Lissia,G. Longo,L. Luzzi,O. Macfadyen,I. N. Machulin,I. Manthos,L. Mapelli,A. Margotti,S. M. Mari,C. Mariani,J. Maricic,A. Marini,M. Martinez,C. J. Martoff,A. Masoni,K. Mavrokoridis,A. Mazzi,A. B. McDonald,A. Messina, R. Milincic,A. Moggi,A. Moharana,J. Monroe,M. Morrocchi,E. N. Mozhevitina,T. Mroz,V. N. Muratova,C. Muscas,P. Musico,R. Nania,T. Napolitano,M. Nessi,G. Nieradka,K. Nikolopoulos,I. Nikulin,J. Nowak, K. Olchansky,A. Oleinik,V. Oleynikov,P. Organtini,A. Ortiz de Solorzano,L. Pagani,M. Pallavicini, L. Pandola,E. Pantic,E. Paoloni,G. Paternoster,P. A. Pegoraro,K. Pelczar,C. Pellegrino,F. Perotti,V. Pesudo,S. Piacentini,F. Pietropaolo,N. Pino,C. Pira,A. Pocar,D. M. Poehlmann,S. Pordes,P. Pralavorio,D. Price,F. Raffaelli,F. Ragusa,Y. Ramachers,A. Ramirez,M. Razeti,A. Razeto,A. L. Renshaw,M. Rescigno,F. Resnati,F. Retiere,L. P. Rignanese,C. Ripoli,A. Rivetti,A. Roberts,C. Roberts,J. Rode,G. Rogers,L. Romero,M. Rossi,A. Rubbia, S. Sadashivajois, T. R. Saffold,O. Samoylov,E. Sandford,S. Sanfilippo,D. Santone,R. Santorelli,C. Savarese,E. Scapparone,G. Scioli,D. A. Semenov,A. Shchagin,A. Sheshukov,M. Simeone,P. Skensved, M. D. Skorokhvatov,O. Smirnov,T. Smirnova,B. Smith,A. Sokolov,M. Spangenberg,R. Stefanizzi,A. Steri,S. Stracka,V. Strickland,M. Stringer,S. Sulis,A. Sung,Y. Suvorov,A. M. Szelc,C. Turkoglu,R. Tartaglia,A. Taylor,J. Taylor,S. Tedesco,G. Testera,K. Thieme,T. N. Thorpe,A. Tonazzo,S. Torres-Lara,A. Tricomi,E. V. Unzhakov,T. Vallivilayil John,M. Van Uffelen,T. Viant,S. Viel,A. Vishneva,R. B. Vogelaar,J. Vossebeld,M. Wada,M. B. Walczak,Y. Wang,S. Westerdale,R. J. Wheadon,L. Williams,I. Wingerter-Seez,R. Wojaczynski,Ma. M. Wojcik,Ma. Wojcik,T. Wright,Y. Xie,C. Yang,A. Zabihi,P. Zakhary,A. Zani,A. Zichichi,G. Zuzel,M. P. Zykova

Physical review D/Physical review D(2023)

引用 2|浏览166
暂无评分
摘要
Dark matter lighter than 10 GeV/c^2 encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a low-threshold electron-counting measurement. Sensitivity to light dark matter is explored for various potential energy thresholds and background rates. These studies show that DarkSide-LowMass can achieve sensitivity to light dark matter down to the solar neutrino floor for GeV-scale masses and significant sensitivity down to 10 MeV/c^2 considering the Migdal effect or interactions with electrons. Requirements for optimizing the detector's sensitivity are explored, as are potential sensitivity gains from modeling and mitigating spurious electron backgrounds that may dominate the signal at the lowest energies.
更多
查看译文
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要