par Chau, Thien Nhan 
;Abbasi, Rasha;Aguilar Sanchez, Juan Antonio ;Maris, Ioana Codrina ;Renzi, Giovanni ;Schlüter, Felix ;Toscano, Simona ; [et al.]
Référence (26 July 2023 through 3 August 2023: Nagoya), 38th International Cosmic Ray Conference, ICRC 2023, Pos proceedings of science (444), 1394
Publication Publié, 2024-03-01
;Abbasi, Rasha;Aguilar Sanchez, Juan Antonio ;Maris, Ioana Codrina ;Renzi, Giovanni ;Schlüter, Felix ;Toscano, Simona ; [et al.]Référence (26 July 2023 through 3 August 2023: Nagoya), 38th International Cosmic Ray Conference, ICRC 2023, Pos proceedings of science (444), 1394
Publication Publié, 2024-03-01
Publication dans des actes
| Résumé : | It is assumed that dark matter can annihilate or decay into Standard Model particles which then can produce a neutrino flux detectable at IceCube. Such a signal can be emitted from the Galactic Center thanks to the high density of dark matter abundance being gravitationally captured. This analysis aims at searching for neutrino signals from dark matter annihilation and decay in the Galactic Center using ∼9 years of IceCube-DeepCore data with an optimized selection for low energy. In this contribution, we present the sensitivities on the thermally averaged dark matter self-annihilation cross-section for dark matter masses ranging from 5 GeV up to 8 TeV. |
