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=c2 mass dark matter. We present new constraints for sub-GeV=c2 dark matter using the dual-phase liquid argon time projection chamber of the DarkSide-50 experiment with an exposure of ð12 306 184Þ 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=c2 . Furthermore, it sets the most stringent upper limit on the spin independent dark matter nucleon cross section for masses below 3.6 GeV=c2.
Agnes, P., Albuquerque, I. . ., Alexander, T., Alton, A. ., Ave, M., Back, H. ., et al. (2023). Search for Dark-Matter–Nucleon Interactions via Migdal Effect with DarkSide-50. PHYSICAL REVIEW LETTERS, 130(10), 101001 [10.1103/PhysRevLett.130.101001].
Search for Dark-Matter–Nucleon Interactions via Migdal Effect with DarkSide-50
Bussino, S.Membro del Collaboration Group
;Mari, S. M.Membro del Collaboration Group
;Sanfilippo, S.Membro del Collaboration Group
;
2023-01-01
Abstract
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=c2 mass dark matter. We present new constraints for sub-GeV=c2 dark matter using the dual-phase liquid argon time projection chamber of the DarkSide-50 experiment with an exposure of ð12 306 184Þ 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=c2 . Furthermore, it sets the most stringent upper limit on the spin independent dark matter nucleon cross section for masses below 3.6 GeV=c2.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.