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Antiprotons from dark matter annihilation through light mediators and a possible excess in AMS-02 (p)over-bar/p data
Huang, XJ; Wei, CC; Wu, YL; Zhang, WH; Zhou, YF; Huang, XJ (reprint author), Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, ZhongGuanCun East Rd 55, Beijing 100190, Peoples R China.
2017
发表期刊PHYSICAL REVIEW D
卷号95期号:6页码:63021
文章类型Article
摘要We showthat in the scenariowhere darkmatter (DM) particles annihilate through lightmediators, the energy spectra of the final state cosmic-ray particles depend strongly on themediatormass. For final state antiprotons, a spectrum with relatively narrow peak occurs when the mediator mass is comparable to the (p) over tildep production threshold. Of interest, the latestAMS-02 data on the (p) over tildep flux ratio hint at a bumplike excess over the expected background in the energy range similar to 100-450 GeV. We showthat such a lightmediator scenario is favored by the latest AMS-02 data over the scenarios of DM direct annihilation into the standard model particles and that of antiprotons produced from inside supernova remnants (SNRs), and is consistent with the upper limits derived from the Fermi-LAT data on the gamma rays towards the dwarf spheroidal galaxies. The (p) over tildep flux ratio with energy above 450 GeVis predicted to fall with energy quickly, which can be easily distinguished from the other two scenarios as they predict the ratio to be flattening or rising up to the multi-TeV region.
学科领域Astronomy & Astrophysics ; Physics
资助者National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000]
DOIhttp://dx.doi.org/10.1103/PhysRevD.95.063021
关键词[WOS]COSMIC-RAYS ; PROPAGATION
语种英语
资助者National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; National Science Foundation of China (NSFC) [11335012, 11475237] ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Key Research Program of Frontier Sciences, CAS ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000] ; Strategic Priority Research Program of CAS Grant [XDB23030000]
WOS类目Astronomy & Astrophysics ; Physics, Particles & Fields
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文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/22097
专题理论物理所SCI论文
通讯作者Huang, XJ (reprint author), Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, ZhongGuanCun East Rd 55, Beijing 100190, Peoples R China.
推荐引用方式
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Huang, XJ,Wei, CC,Wu, YL,et al. Antiprotons from dark matter annihilation through light mediators and a possible excess in AMS-02 (p)over-bar/p data[J]. PHYSICAL REVIEW D,2017,95(6):63021.
APA Huang, XJ,Wei, CC,Wu, YL,Zhang, WH,Zhou, YF,&Huang, XJ .(2017).Antiprotons from dark matter annihilation through light mediators and a possible excess in AMS-02 (p)over-bar/p data.PHYSICAL REVIEW D,95(6),63021.
MLA Huang, XJ,et al."Antiprotons from dark matter annihilation through light mediators and a possible excess in AMS-02 (p)over-bar/p data".PHYSICAL REVIEW D 95.6(2017):63021.
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