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Электронный каталог: Abusleme, A. - JUNO Sensitivity to the Annihilation of MeV Dark Matter in the Galactic Halo
Abusleme, A. - JUNO Sensitivity to the Annihilation of MeV Dark Matter in the Galactic Halo
Статья
Автор: Abusleme, A.
Journal of Cosmology and Astroparticle Physics [Electronic resource]: JUNO Sensitivity to the Annihilation of MeV Dark Matter in the Galactic Halo
б.г.
ISBN отсутствует
Автор: Abusleme, A.
Journal of Cosmology and Astroparticle Physics [Electronic resource]: JUNO Sensitivity to the Annihilation of MeV Dark Matter in the Galactic Halo
б.г.
ISBN отсутствует
Статья
Abusleme, A.
JUNO Sensitivity to the Annihilation of MeV Dark Matter in the Galactic Halo / A.Abusleme, N.Anfimov, T.Antoshkina, N.Balashov, A.Bolshakova, I.Butorov, A.Chetverikov, A.Chukanov, S.Dmitrievsky, D.Dolzhikov, D.Fedoseev, M.Gonchar, Yu.Gornushkin, V.Gromov, A.Gavrikov, D.Korablev, A.Krasnoperov, N.Kutovskiy, D.V.Naumov, E.Naumova, I.Nemchenok, A.Olshevskiy, A.Rybnikov, A.Sadovsky, A.Selyunin, V.Sharov, A.Shaydurova, V.Shutov, O.Smirnov, S.Sokolov, A.Sotnikov, K.Treskov, V.Zavadskyi, [a.o.] // Journal of Cosmology and Astroparticle Physics [Electronic resource]. – 2023. – Vol. 2023, No. 9. – P. 001. – URL: https://doi.org/10.1088/1475-7516/2023/09/001.
We discuss JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo via detecting inverse beta decay reactions of electron anti-neutrinos resulting from the annihilation. We study possible backgrounds to the signature, including the reactor neutrinos, diffuse supernova neutrino background, charged- and neutral-current interactions of atmospheric neutrinos, backgrounds from muon-induced fast neutrons and cosmogenic isotopes. A fiducial volume cut, as well as the pulse shape discrimination and the muon veto are applied to suppress the above backgrounds. It is shown that JUNO sensitivity to the thermally averaged dark matter annihilation rate in 10 years of exposure would be significantly better than the present-day best limit set by Super-Kamiokande and would be comparable to that expected by Hyper-Kamiokande.
ОИЯИ = ОИЯИ (JINR)2023
Спец.(статьи,препринты) = С 344.1х - Методы регистрации нейтрино
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны
Abusleme, A.
JUNO Sensitivity to the Annihilation of MeV Dark Matter in the Galactic Halo / A.Abusleme, N.Anfimov, T.Antoshkina, N.Balashov, A.Bolshakova, I.Butorov, A.Chetverikov, A.Chukanov, S.Dmitrievsky, D.Dolzhikov, D.Fedoseev, M.Gonchar, Yu.Gornushkin, V.Gromov, A.Gavrikov, D.Korablev, A.Krasnoperov, N.Kutovskiy, D.V.Naumov, E.Naumova, I.Nemchenok, A.Olshevskiy, A.Rybnikov, A.Sadovsky, A.Selyunin, V.Sharov, A.Shaydurova, V.Shutov, O.Smirnov, S.Sokolov, A.Sotnikov, K.Treskov, V.Zavadskyi, [a.o.] // Journal of Cosmology and Astroparticle Physics [Electronic resource]. – 2023. – Vol. 2023, No. 9. – P. 001. – URL: https://doi.org/10.1088/1475-7516/2023/09/001.
We discuss JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo via detecting inverse beta decay reactions of electron anti-neutrinos resulting from the annihilation. We study possible backgrounds to the signature, including the reactor neutrinos, diffuse supernova neutrino background, charged- and neutral-current interactions of atmospheric neutrinos, backgrounds from muon-induced fast neutrons and cosmogenic isotopes. A fiducial volume cut, as well as the pulse shape discrimination and the muon veto are applied to suppress the above backgrounds. It is shown that JUNO sensitivity to the thermally averaged dark matter annihilation rate in 10 years of exposure would be significantly better than the present-day best limit set by Super-Kamiokande and would be comparable to that expected by Hyper-Kamiokande.
ОИЯИ = ОИЯИ (JINR)2023
Спец.(статьи,препринты) = С 344.1х - Методы регистрации нейтрино
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны