银河系中心伽马射线过剩作为暗物质的印记

IF 0.6 4区 物理与天体物理 Q4 PHYSICS, MULTIDISCIPLINARY
V. V. Burdyuzha
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引用次数: 0

摘要

费米天文台观测到,磁单极子(2.4 GeV)的原子湮灭及其在莱曼系列(1.8、2.1和2.25 GeV)中的跃迁可能导致银河系中心的伽马射线过剩。GeV能量的单极子可以在磁星的磁球中形成并被吹出。在星系尺度上,来自磁单极子(g+g -)的原子是暗物质的一部分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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来源期刊
Bulletin of the Lebedev Physics Institute
Bulletin of the Lebedev Physics Institute PHYSICS, MULTIDISCIPLINARY-
CiteScore
0.70
自引率
25.00%
发文量
41
审稿时长
6-12 weeks
期刊介绍: Bulletin of the Lebedev Physics Institute is an international peer reviewed journal that publishes results of new original experimental and theoretical studies on all topics of physics: theoretical physics; atomic and molecular physics; nuclear physics; optics; lasers; condensed matter; physics of solids; biophysics, and others.
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