中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints

文献类型:期刊论文

作者Ding, YC; Li, N; Wei, CC; Wu, YL; Zhou, YF
刊名JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
出版日期2019
期号6页码:4
ISSN号1475-7516
关键词PROPAGATION PROTON COLLISIONS PARTICLES DEUTERON ENERGIES
DOI10.1088/1475-7516/2019/06/004
英文摘要Cosmic-ray (CR) antihelium is an important observable for dark matter (DM) indirect Searches due to extremely low secondary backgrounds towards low energies. In a given DM model, the predicted CR antihelium flux is expected to be strongly correlated with that of CR antiprotons. In this work, we use the AMS-02 (p) over bar /p data to constrain the DM annihilation cross section, and the ALICE data on the (3)(He) over bar and (T) over bar productions to determine the parameters in the coalescence model for anti-nucleus formation. The hadronic cross sections are estimated using Monte-Carlo event generators including EPOS-LHC and DPMJET. Based on these constraints, we make predictions for the maximal antihelium flux for typical DM annihilation final states, and perform a detailed analysis on the uncertainties due to the DM density profiles and CR propagation models. We find that the results are highly insensitive to both of them, but still significantly depend on the hadronization models in event generators. The prospects of detecting antihelium for the AMS-02 experiment is discussed. We show that with very optimistic assumptions, CR (3)(He) over bar is within the reach of the AMS-02 experiment. The (3)(He) over bar events which can be detected by AMS-02 are likely to have kinetic energy T greater than or similar to 30 GeV, which is consistent with the preliminary AMS-02 search results. The events which can be observed by AMS-02 are likely to arise dominantly from secondary backgrounds rather than DM interactions.
学科主题Astronomy & Astrophysics ; Physics
语种英语
源URL[http://ir.itp.ac.cn/handle/311006/23414]  
专题理论物理研究所_理论物理所1978-2010年知识产出
作者单位1.Univ Chinese Acad Sci, Yuquan Rd 19A, Beijing 100049, Peoples R China
2.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Zhongguancun East Rd 55, Beijing 100190, Peoples R China
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GB/T 7714
Ding, YC,Li, N,Wei, CC,et al. Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints[J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS,2019(6):4.
APA Ding, YC,Li, N,Wei, CC,Wu, YL,&Zhou, YF.(2019).Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints.JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS(6),4.
MLA Ding, YC,et al."Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints".JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS .6(2019):4.

入库方式: OAI收割

来源:理论物理研究所

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