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Modified Baryogenesis and Ultra-High-Energy Cosmic Rays. / Arbuzova, E. V.

In: Physics of Particles and Nuclei, Vol. 56, No. 3, 27.06.2025, p. 632-638.

Research output: Contribution to journal › Article › peer-review

Harvard

Arbuzova, EV 2025, 'Modified Baryogenesis and Ultra-High-Energy Cosmic Rays', Physics of Particles and Nuclei, vol. 56, no. 3, pp. 632-638. https://doi.org/10.1134/S1063779624702034

APA

Arbuzova, E. V. (2025). Modified Baryogenesis and Ultra-High-Energy Cosmic Rays. Physics of Particles and Nuclei, 56(3), 632-638. https://doi.org/10.1134/S1063779624702034

Vancouver

Arbuzova EV. Modified Baryogenesis and Ultra-High-Energy Cosmic Rays. Physics of Particles and Nuclei. 2025 Jun 27;56(3):632-638. doi: 10.1134/S1063779624702034

Author

Arbuzova, E. V. / Modified Baryogenesis and Ultra-High-Energy Cosmic Rays. In: Physics of Particles and Nuclei. 2025 ; Vol. 56, No. 3. pp. 632-638.

BibTeX

@article{5ce22508b74f401c986c32f0edb7a10b,
title = "Modified Baryogenesis and Ultra-High-Energy Cosmic Rays",
abstract = "The scenario of gravitational baryogenesis modified through adding an R2 term into the model is explored. This modification allows eliminating the cosmological instability inherent to the canonical version of gravitational baryogenesis. In the updated model, the exponential growth of the curvature is transformed into high-frequency oscillations, which, in turn, results in forming super-heavy dark matter particles. Slow decay of these particles through virtual black holes can contribute to the flux of ultra-high-energy cosmic rays.",
author = "Arbuzova, {E. V.}",
note = "The work was supported by the Russian Science Foundation Grant no. 22-12-00103. Arbuzova, E. V. Modified Baryogenesis and Ultra-High-Energy Cosmic Rays / E. V. Arbuzova // Physics of Particles and Nuclei. – 2025. – Vol. 56, No. 3. – P. 632-638. – DOI 10.1134/S1063779624702034.",
year = "2025",
month = jun,
day = "27",
doi = "10.1134/S1063779624702034",
language = "English",
volume = "56",
pages = "632--638",
journal = "Physics of Particles and Nuclei",
issn = "1063-7796",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "3",

}

RIS

TY - JOUR

T1 - Modified Baryogenesis and Ultra-High-Energy Cosmic Rays

AU - Arbuzova, E. V.

N1 - The work was supported by the Russian Science Foundation Grant no. 22-12-00103. Arbuzova, E. V. Modified Baryogenesis and Ultra-High-Energy Cosmic Rays / E. V. Arbuzova // Physics of Particles and Nuclei. – 2025. – Vol. 56, No. 3. – P. 632-638. – DOI 10.1134/S1063779624702034.

PY - 2025/6/27

Y1 - 2025/6/27

N2 - The scenario of gravitational baryogenesis modified through adding an R2 term into the model is explored. This modification allows eliminating the cosmological instability inherent to the canonical version of gravitational baryogenesis. In the updated model, the exponential growth of the curvature is transformed into high-frequency oscillations, which, in turn, results in forming super-heavy dark matter particles. Slow decay of these particles through virtual black holes can contribute to the flux of ultra-high-energy cosmic rays.

AB - The scenario of gravitational baryogenesis modified through adding an R2 term into the model is explored. This modification allows eliminating the cosmological instability inherent to the canonical version of gravitational baryogenesis. In the updated model, the exponential growth of the curvature is transformed into high-frequency oscillations, which, in turn, results in forming super-heavy dark matter particles. Slow decay of these particles through virtual black holes can contribute to the flux of ultra-high-energy cosmic rays.

UR - https://www.mendeley.com/catalogue/86b01158-e5b8-354d-8a9c-37178455b102/

UR - https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=105009329898&origin=inward

UR - https://www.elibrary.ru/item.asp?id=82558450

U2 - 10.1134/S1063779624702034

DO - 10.1134/S1063779624702034

M3 - Article

VL - 56

SP - 632

EP - 638

JO - Physics of Particles and Nuclei

JF - Physics of Particles and Nuclei

SN - 1063-7796

IS - 3

ER -

ID: 68294913