MeV gamma-ray constraints for light dark matter from semi-annihilation

Exploring the realm of Dark Matter research, Light DM, which has a mass in the range of 1 MeV to 1 GeV, is a fascinating topic both theoretically and experimentally. We assume that the light dark matter is composed of complex scalars and produced from semi-annihilation, which is close to the scale o...

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Main Authors: Jun Guo, Lei Wu, Bin Zhu
Format: Article
Language:English
Published: Elsevier 2023-05-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269323001879
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author Jun Guo
Lei Wu
Bin Zhu
author_facet Jun Guo
Lei Wu
Bin Zhu
author_sort Jun Guo
collection DOAJ
description Exploring the realm of Dark Matter research, Light DM, which has a mass in the range of 1 MeV to 1 GeV, is a fascinating topic both theoretically and experimentally. We assume that the light dark matter is composed of complex scalars and produced from semi-annihilation, which is close to the scale of the MeV Gamma-ray satellite, allowing us to explore the implications of this hypothesis. The experimental data we used to constrain the scenario is from five different sources: the COMPTEL, EGRET, INTEGRAL, Fermi Gamma-ray Space Telescope, and the e-ASTROGAM future reach. We use the analytical formula to measure the X-ray spectra allowing us to determine the annihilation cross-section bounds from 10−28cm3/s to 10−22cm3/s for different combinations of dark matter and mediator masses. We found that the MeV gamma-ray provides valuable insight into the structure of the semi-annihilation dark matter, where EGRET contributes to the stringent constraint to the semi-annihilation, and the e-ASTROGAM future reach could probe the whole parameter space of the model.
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spelling doaj.art-900632d2aa25449a8784dcc4c54149cc2023-04-20T04:35:33ZengElsevierPhysics Letters B0370-26932023-05-01840137853MeV gamma-ray constraints for light dark matter from semi-annihilationJun Guo0Lei Wu1Bin Zhu2College of Physics and Communication Electronics, Jiangxi Normal University, Nanchang 330022, China; Corresponding authors.Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing, 210023, China; Corresponding authors.Department of Physics, Yantai University, Yantai 264005, China; Corresponding authors.Exploring the realm of Dark Matter research, Light DM, which has a mass in the range of 1 MeV to 1 GeV, is a fascinating topic both theoretically and experimentally. We assume that the light dark matter is composed of complex scalars and produced from semi-annihilation, which is close to the scale of the MeV Gamma-ray satellite, allowing us to explore the implications of this hypothesis. The experimental data we used to constrain the scenario is from five different sources: the COMPTEL, EGRET, INTEGRAL, Fermi Gamma-ray Space Telescope, and the e-ASTROGAM future reach. We use the analytical formula to measure the X-ray spectra allowing us to determine the annihilation cross-section bounds from 10−28cm3/s to 10−22cm3/s for different combinations of dark matter and mediator masses. We found that the MeV gamma-ray provides valuable insight into the structure of the semi-annihilation dark matter, where EGRET contributes to the stringent constraint to the semi-annihilation, and the e-ASTROGAM future reach could probe the whole parameter space of the model.http://www.sciencedirect.com/science/article/pii/S0370269323001879
spellingShingle Jun Guo
Lei Wu
Bin Zhu
MeV gamma-ray constraints for light dark matter from semi-annihilation
Physics Letters B
title MeV gamma-ray constraints for light dark matter from semi-annihilation
title_full MeV gamma-ray constraints for light dark matter from semi-annihilation
title_fullStr MeV gamma-ray constraints for light dark matter from semi-annihilation
title_full_unstemmed MeV gamma-ray constraints for light dark matter from semi-annihilation
title_short MeV gamma-ray constraints for light dark matter from semi-annihilation
title_sort mev gamma ray constraints for light dark matter from semi annihilation
url http://www.sciencedirect.com/science/article/pii/S0370269323001879
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