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Cosmic Rays from Heavy Particle Decays. / Arbuzova, E. V.; Dolgov, A. D.; Nikitenko, A. A.

в: Physics of Atomic Nuclei, Том 87, № 1, 02.2024, стр. 49-55.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Arbuzova, EV, Dolgov, AD & Nikitenko, AA 2024, 'Cosmic Rays from Heavy Particle Decays', Physics of Atomic Nuclei, Том. 87, № 1, стр. 49-55. https://doi.org/10.1134/S1063778824020066

APA

Vancouver

Arbuzova EV, Dolgov AD, Nikitenko AA. Cosmic Rays from Heavy Particle Decays. Physics of Atomic Nuclei. 2024 февр.;87(1):49-55. doi: 10.1134/S1063778824020066

Author

Arbuzova, E. V. ; Dolgov, A. D. ; Nikitenko, A. A. / Cosmic Rays from Heavy Particle Decays. в: Physics of Atomic Nuclei. 2024 ; Том 87, № 1. стр. 49-55.

BibTeX

@article{ad8b11a231d949e390dc8a0a0ffa8945,
title = "Cosmic Rays from Heavy Particle Decays",
abstract = "Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such processes are estimated. It is shown that with the proper fixation of the parameters the decays of these ultra-massive particles can give noticeable contribution to the flux of high energy cosmic rays in particular, near the Greisen–Zatsepin–Kuzmin limit. Such particles can also create neutrinos of very high energies observed in the existing huge underwater or ice-cube detectors.",
author = "Arbuzova, {E. V.} and Dolgov, {A. D.} and Nikitenko, {A. A.}",
note = "The work by E.V. Arbuzova and A.A. Nikitenko was supported by RSF grant no. 22-22-00294.",
year = "2024",
month = feb,
doi = "10.1134/S1063778824020066",
language = "English",
volume = "87",
pages = "49--55",
journal = "Physics of Atomic Nuclei",
issn = "1063-7788",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "1",

}

RIS

TY - JOUR

T1 - Cosmic Rays from Heavy Particle Decays

AU - Arbuzova, E. V.

AU - Dolgov, A. D.

AU - Nikitenko, A. A.

N1 - The work by E.V. Arbuzova and A.A. Nikitenko was supported by RSF grant no. 22-22-00294.

PY - 2024/2

Y1 - 2024/2

N2 - Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such processes are estimated. It is shown that with the proper fixation of the parameters the decays of these ultra-massive particles can give noticeable contribution to the flux of high energy cosmic rays in particular, near the Greisen–Zatsepin–Kuzmin limit. Such particles can also create neutrinos of very high energies observed in the existing huge underwater or ice-cube detectors.

AB - Multidimensional modification of gravity with a smaller mass scale of the gravitational interaction is considered. Stable by assumption dark matter particles could decay via interactions with virtual black holes. The decay rates of such processes are estimated. It is shown that with the proper fixation of the parameters the decays of these ultra-massive particles can give noticeable contribution to the flux of high energy cosmic rays in particular, near the Greisen–Zatsepin–Kuzmin limit. Such particles can also create neutrinos of very high energies observed in the existing huge underwater or ice-cube detectors.

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UR - https://www.mendeley.com/catalogue/1aad9256-941e-31f9-9158-9955111c826c/

U2 - 10.1134/S1063778824020066

DO - 10.1134/S1063778824020066

M3 - Article

VL - 87

SP - 49

EP - 55

JO - Physics of Atomic Nuclei

JF - Physics of Atomic Nuclei

SN - 1063-7788

IS - 1

ER -

ID: 61174263