Artículo

Search for Daily Modulation of MeV Dark Matter Signals with DAMIC-M

Arnquist, I. ; Avalos, Nicolás Ezequiel ; Baxter, D. ; Bertou, Xavier Pierre Louis Icon; Castelló Mor, N. ; Chavarria, A. E. ; Cuevas Zepeda, J. ; Dastgheibi Fard, A. ; De Dominicis, C. ; Deligny, O. ; Estrada, E. ; Gadola, N. ; Gaïor, R. ; Hossbach, T. ; Iddir, L. ; Kavanagh, B. J. ; Kilminster, B. ; Lantero Barreda, A. ; Lawson, I. ; Lee, S. ; Letessier Selvon, A. ; Loaiza, P. ; Lopez Virto, A. ; McGuire, K. J. ; Mitra, P. ; Traina, Ángeles Melina ; Vilar, R. ; Warot, G. ; Yajur, R. ; Zopounidis, J. P.

Otros responsables

Fecha

03/2024

Editorial

American Physical Society

Revista

Physical Review Letters

Título del libro

Nombre del evento

Fecha del evento

Institución organizadora

ISSN

0031-9007

eISSN

ISBN

Idioma

Inglés

Tipo del evento

Resumen

Dark matter (DM) particles with sufficiently large cross sections may scatter as they travel through Earth’s bulk. The corresponding changes in the DM flux give rise to a characteristic daily modulation signal in detectors sensitive to DM-electron interactions. Here, we report results obtained from the first underground operation of the DAMIC-M prototype detector searching for such a signal from DM with MeV-scale mass. A model-independent analysis finds no modulation in the rate of 1 e− events with sidereal period, where a DM signal would appear. We then use these data to place exclusion limits on DM in the mass range [0.53; 2.7]Š MeV/c2 interacting with electrons via a dark photon mediator. Taking advantage of the time-dependent signal we improve by ∼2 orders of magnitude on our previous limit obtained from the total rate of 1 e− events, using the same dataset. This daily modulation search represents the current strongest limit on DM-electron scattering via ultralight mediators for DM masses around 1 MeV/c2.

Aprobación

Revisión

Complementado por

Referenciado por

Licencia Creative Commons

Excepto donde se indique lo contrario, la licencia de este ítem se describe como by-nc-sa