Constraints on dark matter with future MeV gamma-ray telescopes

IF 5 2区 物理与天体物理 Q1 Physics and Astronomy
Kayla E. O’Donnell, Tracy R. Slatyer
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引用次数: 0

Abstract

A number of new balloon or space-based γ-ray observatories have been proposed to close a “MeV gap” in sensitivity to γ rays in the MeV–GeV energy band. One aspect of the science case for these instruments is their ability to constrain or discover decaying or annihilating dark matter. In this work, we forecast the sensitivity of these instruments for dark matter annihilation or decay for a range of possible Standard Model final states and compare to existing bounds. Published by the American Physical Society 2025
未来MeV伽玛射线望远镜对暗物质的限制
已经提出了一些新的气球或空间γ射线观测站,以弥补对MeV-GeV能段γ射线灵敏度的 "MeV差距"。这些仪器的科学依据之一是它们能够约束或发现衰变或湮灭的暗物质。在这项工作中,我们预测了这些仪器对一系列可能的标准模型终态的暗物质湮灭或衰变的灵敏度,并与现有的边界进行了比较。 美国物理学会出版 2025
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physical Review D
Physical Review D 物理-天文与天体物理
CiteScore
9.20
自引率
36.00%
发文量
0
审稿时长
2 months
期刊介绍: Physical Review D (PRD) is a leading journal in elementary particle physics, field theory, gravitation, and cosmology and is one of the top-cited journals in high-energy physics. PRD covers experimental and theoretical results in all aspects of particle physics, field theory, gravitation and cosmology, including: Particle physics experiments, Electroweak interactions, Strong interactions, Lattice field theories, lattice QCD, Beyond the standard model physics, Phenomenological aspects of field theory, general methods, Gravity, cosmology, cosmic rays, Astrophysics and astroparticle physics, General relativity, Formal aspects of field theory, field theory in curved space, String theory, quantum gravity, gauge/gravity duality.
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