Zobrazeno 1 - 10
of 55
pro vyhledávání: '"K. M. Belotsky"'
Publikováno v:
Physics of Atomic Nuclei. 85:92-96
Autor:
Pino Di Sciascio, M. Khlopov, Alexander S. Sakharov, Qingyu Gan, Paolo Panci, Michael Kachekriess, Vladimir Korchagin, Roman Pasechnick, Filippo Sala, Vladimir Kuksa, Andrei Neronov, K. M. Belotsky, Nicolao Fornengo, Arman Esmaili, N. Volchanskiy, Alexander Korochkin, Andrea Addazi, Vitaly Beylin, Pasquale D. Serpico, Dimitri Semikoz, Marco Cirelli, Antonino Marciano
Publikováno v:
37th International Cosmic Ray Conference
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.574, ⟨10.22323/1.395.0574⟩
Proceedings of Science
37th International Cosmic Ray Conference (ICRC 2021)
37th International Cosmic Ray Conference (ICRC 2021), Jul 2021, Berlin, Germany. pp.574, ⟨10.22323/1.395.0574⟩
37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.574, ⟨10.22323/1.395.0574⟩
Proceedings of Science
37th International Cosmic Ray Conference (ICRC 2021)
37th International Cosmic Ray Conference (ICRC 2021), Jul 2021, Berlin, Germany. pp.574, ⟨10.22323/1.395.0574⟩
International audience; We discuss the implications of next future LHAASO data on searches of Heavy Dark Matter decays.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b5e4ee07a616b8217c349178ee4619fc
https://hal.archives-ouvertes.fr/hal-03359029/file/document-1.pdf
https://hal.archives-ouvertes.fr/hal-03359029/file/document-1.pdf
Publikováno v:
Symmetry, Vol 12, Iss 1442, p 1442 (2020)
Symmetry
Volume 12
Issue 9
Symmetry
Volume 12
Issue 9
The effect of neutrino cooling of possible primary regions filled by hot matter is discussed. Such regions could be obtained from the primordial density inhomogeneities and survive up to the modern epoch. The inhomogeneities could be caused by a symm
Autor:
K. M. Belotsky, N. O. Nazarova
Publikováno v:
Physics of Atomic Nuclei. 80:1177-1180
The model of dark matter featuring a component in the form of free particles and antiparticles (a, ā ) possessing self-interaction of the Coulomb type is considered. Darkmattermay form small-scale clumps where the annihilation of particles a and ā
Autor:
R. I. Budaev, Yu V. Bogomolov, S. A. Rodenko, A. F. Mosichkin, A. M. Shitova, K. M. Belotsky, A. M. Galper, A. G. Mayorov, V. V. Alekseev, A. A. Okrugin, V. V. Malakhov, M. A. Mayorova, Alexander Kuznetsov, A. D. Lukyanov, A. A. Kirillov, O. A. Dunaeva
Publikováno v:
Physics of Particles and Nuclei. 48:687-690
The paper provides a review of the results of precision measurements of the fluxes of different charged components of galactic cosmic rays (positrons and antiprotons, protons and helium nuclei) in modern experiments with magnetic spectrometers PAMELA
Autor:
A. M. Shitova, O. A. Dunaeva, K. M. Belotsky, Yu V. Bogomolov, S. A. Rodenko, A. D. Lukyanov, V. V. Malakhov, A. F. Mosichkin, A. G. Mayorov, A. A. Kirillov, R. I. Budaev, M. A. Mayorova, A. A. Okrugin, Alexander Kuznetsov, V. V. Alekseev
Publikováno v:
Physics of Atomic Nuclei. 80:713-717
The possibility of explaining the positron anomaly on the basis of models involving the darkmatter annihilation or decay is being widely discussed at the present time. However, such models are severely constrained by data on cosmic gamma radiation. T
Here we briefly review possible indirect effects of dark matter (DM) of the Universe. It includes effects in cosmic rays (CR): first of all, the positron excess at $\sim$ 500 GeV and possible electron-positron excess at 1-1.5 TeV. We tell that the ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b848c4f9912dc8568676478faedb662
http://arxiv.org/abs/1909.04735
http://arxiv.org/abs/1909.04735
Autor:
E. A. Esipova, Alexander Kirillov, Maxim Yu. Khlopov, Valeriy V. Nikulin, I. V. Svadkovsky, Yury Eroshenko, K. M. Belotsky, Sergey G. Rubin, Leonid A. Khromykh, Vyacheslav Dokuchaev
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 79, Iss 3, Pp 1-20 (2019)
European Physical Journal
European Physical Journal
The Primordial Black Holes (PBHs) are gradually involved into consideration as the phenomenon having reliable basis. We discuss here the possibility of their agglomeration into clusters that may have several prominent observable features. The cluster
The direct measurements of the cosmic electron-positron spectrum around 1 TeV made by DAMPE have induced many theoretical speculations about possible excesses in the data above the standard astrophysical predictions that might have the dark matter (D
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b55235015274672400b4ea7ca024c317
Publikováno v:
Physics of Atomic Nuclei. 80:718-720
It is shown that the formation of primordialmassive black holes may be accompanied by a local heating of matter. The proposed heating mechanism is based on the interaction of the Higgs field with a scalar field that is responsible for the formation o