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constraints on the dark matter annihilation scenario of Fermi 130 GeV gamma-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observations (vol 11, pg 48, 2013)
Huang, Xiaoyuan1; Yuan, Qiang2,3; Yin, Peng-Fei2; Bi, Xiao-Jun2; Chen, Xuelei1
2013-05-01
Source PublicationJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
ISSN1475-7516
Volume0Issue:5Pages:0267
Corresponding AuthorHuang, XY (reprint author), Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China. Email: huangxiaoyuan@gmail.com ; yuanq@ihep.ac.cn ; yinpf@ihep.ac.cn ; bixj@ihep.ac.cn ; xuelei@cosmology.bao.ac.cn
AbstractIt was recently reported that there may exist monochromatic $\gamma$-ray emission at $\sim 130$ GeV from the Galactic center in the Fermi Large Area Telescope data, which might be related with dark matter (DM) annihilation. In this work we carry out a comprehensive check of consistency of the results with the DM annihilation scenario, using the 3.7 yrs Fermi observation of the inner Galaxy, Galactic halo, clusters of galaxies and dwarf galaxies. The results found are as follows. 1) Very strong constraints on the DM annihilation into continuous $\gamma$-rays from the Galactic center are set, which are as stringent as the "natural" scale assuming thermal freeze-out of DM. Such limit sets strong constraint on the DM models to explain the line emission. 2) No line emission from the Galactic halo is found in the Fermi data, and the constraints on line emission is marginally consistent with the DM annihilation interpretation of the $\sim 130$ GeV line emission from the inner Galaxy. 3) No line emission from galaxy clusters and dwarf galaxies is detected, although possible concentration of photons from clusters in 120-140 GeV is revealed. The constraints from clusters and dwarf galaxies are weak and consistent with the DM annihilation scenario to explain the $\sim 130$ GeV line emission.
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1088/1475-7516/2013/05/E02
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics ; Physics
WOS SubjectAstronomy & Astrophysics ; Physics, Particles & Fields
WOS IDWOS:000320161400002
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/9836
Collection分子云与恒星形成研究团组
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Jiangsu, Peoples R China
Recommended Citation
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Huang, Xiaoyuan,Yuan, Qiang,Yin, Peng-Fei,et al. constraints on the dark matter annihilation scenario of Fermi 130 GeV gamma-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observations (vol 11, pg 48, 2013)[J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS,2013,0(5):0267.
APA Huang, Xiaoyuan,Yuan, Qiang,Yin, Peng-Fei,Bi, Xiao-Jun,&Chen, Xuelei.(2013).constraints on the dark matter annihilation scenario of Fermi 130 GeV gamma-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observations (vol 11, pg 48, 2013).JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS,0(5),0267.
MLA Huang, Xiaoyuan,et al."constraints on the dark matter annihilation scenario of Fermi 130 GeV gamma-ray line emission by continuous gamma-rays, Milky Way halo, galaxy clusters and dwarf galaxies observations (vol 11, pg 48, 2013)".JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS 0.5(2013):0267.
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