CONSTRAINING THE DISTRIBUTION OF DARK MATTER IN THE INNER GALAXY WITH AN INDIRECT DETECTION SIGNAL: THE CASE OF A TENTATIVE 130 GeV gamma-RAY LINE | |
Yang, Rui-Zhi1,2; Feng, Lei1; Li, Xiang1,2; Fan, Yi-Zhong1![]() | |
刊名 | ASTROPHYSICAL JOURNAL
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2013-06-20 | |
卷号 | 770期号:2页码:0 |
关键词 | dark matter galaxies: structure gamma rays: general |
ISSN号 | 0004-637X |
通讯作者 | Yang, RZ (reprint author), Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Jiangsu, Peoples R China. Email: yzfan@pmo.ac.cn |
英文摘要 | Dark matter distribution in the very inner region of our Galaxy is still debated. In N-body simulations, a cuspy dark matter halo density profile is favored. Several dissipative baryonic processes, however, are found to be able to significantly flatten dark matter distribution, and a cored dark matter halo density profile is possible. Baryons dominate the gravitational potential in the inner Galaxy, hence a direct constraint on the abundance of dark matter particles is rather challenging. Recently, a few groups have identified a tentative 130 GeV line signal in the Galactic center, which could be interpreted as the signal of dark matter annihilation. Using current 130 GeV line data and adopting the generalized Navarro-Frenk-White profile of the dark matter halo-local dark matter density rho(0) = 0.4 GeV cm(-3) and r(s) = 20 kpc-we obtain a 95% confidence level lower (upper) limit on the inner slope of dark matter density distribution, alpha = 1.06 (the cross section of dark matter annihilation into gamma-rays |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | HALOS ; CONDENSATION ; CONTRACTION ; FEEDBACK ; CUSPS ; CORES ; MILKY |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000320111200045 |
公开日期 | 2014-01-08 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/9887] ![]() |
专题 | 紫金山天文台_宇宙伽马暴、中子星及相关物理研究团组 |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210008, Jiangsu, Peoples R China 2.Chinese Acad Sci, Grad Univ, Beijing 100012, Peoples R China |
推荐引用方式 GB/T 7714 | Yang, Rui-Zhi,Feng, Lei,Li, Xiang,et al. CONSTRAINING THE DISTRIBUTION OF DARK MATTER IN THE INNER GALAXY WITH AN INDIRECT DETECTION SIGNAL: THE CASE OF A TENTATIVE 130 GeV gamma-RAY LINE[J]. ASTROPHYSICAL JOURNAL,2013,770(2):0. |
APA | Yang, Rui-Zhi,Feng, Lei,Li, Xiang,&Fan, Yi-Zhong.(2013).CONSTRAINING THE DISTRIBUTION OF DARK MATTER IN THE INNER GALAXY WITH AN INDIRECT DETECTION SIGNAL: THE CASE OF A TENTATIVE 130 GeV gamma-RAY LINE.ASTROPHYSICAL JOURNAL,770(2),0. |
MLA | Yang, Rui-Zhi,et al."CONSTRAINING THE DISTRIBUTION OF DARK MATTER IN THE INNER GALAXY WITH AN INDIRECT DETECTION SIGNAL: THE CASE OF A TENTATIVE 130 GeV gamma-RAY LINE".ASTROPHYSICAL JOURNAL 770.2(2013):0. |
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