Search for Dark Matter-Nucleon Interactions Via Migdal Effect with DarkSide-50

The DarkSide-5 Collaboration,P. Agnes,I. F. M. Albuquerque,T. Alexander,A. K. Alton,M. Ave,H. O. Back,G. Batignani,K. Biery,V. Bocci,W. M. Bonivento,B. Bottino,S. Bussino,M. Cadeddu,M. Cadoni,F. Calaprice,A. Caminata,M. D. Campos,N. Canci,M. Caravati,M. Cariello,M. Carlini, M. Carpinelli,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,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. 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,E. Picciau,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,W. Sands,S. Sanfilippo,E. Sanford,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

arxiv(2022)

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摘要
Dark matter elastic scattering off nuclei can result in the excitation and ionization of the recoiling atom through the so-called Migdal effect. The energy deposition from the ionization electron adds to the energy deposited by the recoiling nuclear system and allows for the detection of interactions of sub-GeV/c^2 mass dark matter. We present new constraints for sub-GeV/c^2 dark matter using the dual-phase liquid argon time projection chamber of the DarkSide-50 experiment with an exposure of (12306 ± 184) kg d. The analysis is based on the ionization signal alone and significantly enhances the sensitivity of DarkSide-50, enabling sensitivity to dark matter with masses down to 40 MeV/c^2. Furthermore, it sets the most stringent upper limit on the spin independent dark matter nucleon cross section for masses below 3.6 GeV/c^2.
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