Galactic Center Gamma-Ray Excess As Imprint of Dark Matter

Probably, annihilation of atoms from magnetic monopoles (2.4 GeV) and their transitions in the Lyman series (1.8, 2.1, and 2.25 GeV) could result in a gamma-ray excess in our galactic center, which was observed by the Fermi observatory. Monopoles of GeV energies can form in the magnetospheres of magnetars and be blown out of them. At the galactic scale, atoms from magnetic monopoles (g+g‒) are part of dark matter.

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Publication Details

Journal
Bulletin of the Lebedev Physics Institute
Published
2024-12-01
DOI
https://doi.org/10.3103/s1068335624602000
Primary Topic
Atomic and Subatomic Physics Research
Type
article
Field-Weighted Citation Impact
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article

Galactic Center Gamma-Ray Excess As Imprint of Dark Matter

V. V. Burdyuzha
Bulletin of the Lebedev Physics Institute
Atomic and Subatomic Physics Research
article

Galactic Center Gamma-Ray Excess As Imprint of Dark Matter

V. V. Burdyuzha
article en

Abstract

Probably, annihilation of atoms from magnetic monopoles (2.4 GeV) and their transitions in the Lyman series (1.8, 2.1, and 2.25 GeV) could result in a gamma-ray excess in our galactic center, which was observed by the Fermi observatory. Monopoles of GeV energies can form in the magnetospheres of magnetars and be blown out of them. At the galactic scale, atoms from magnetic monopoles (g+g‒) are part of dark matter.

Bulletin of the Lebedev Physics InstituteVol. 51(12)
P.N. Lebedev Physical Institute of the Russian Academy of Sciences (RU), Astro Space Center (RU)
Openalex Percentile: Top 77%
Atomic and Subatomic Physics Research
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