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Huang, XJ; Wu, YL; Zhang, WH; Zhou, YF
Origins of sharp cosmic-ray electron structures and the DAMPE excess
Source PublicationPHYSICAL REVIEW D
Language英语
KeywordDARK-MATTER ANNIHILATION FERMI-LAT CONSTRAINTS SATELLITES EMISSION SEESAW E(-)
AbstractNearby sources may contribute to cosmic-ray electron (CRE) structures at high energies. Recently, the first DAMPE results on the CRE flux hinted at a narrow excess at energy similar to 1.4 TeV. We show that in general a spectral structure with a narrow width appears in two scenarios. The first is spectrum broadening for the continuous sources with a delta-function-like injection spectrum. In this scenario, a finite width can develop after propagation through the Galaxy, which can reveal the distance of the source. Well-motivated sources include minispikes and subhalos formed by dark matter (DM) particles x(s) which annihilate directly into e(+)e(-) pairs. The second is phase-space shrinking for burstlike sources with a power-law-like injection spectrum. The spectrum after propagation can shrink at a cooling-related cutoff energy and form a sharp spectral peak. The peak can be more prominent due to the energy-dependent diffusion. In this scenario, the width of the excess constrains both the power index and the distance of the source. Possible such sources are pulsar wind nebulae (PWNe) and supernova remnants (SNRs). We analysis the DAMPE excess and find that the continuous DM sources should be fairly close within similar to 0.3 kpc, and the annihilation cross sections are close to the thermal value. For the burstlike source, the narrow width of the excess suggests that the injection spectrum must be hard with power index significantly less than two, the distance is within similar to(3-4) kpc, and the age of the source is similar to 0.16 Myr. In both scenarios, large anisotropies in the CRE flux are predicted. We identify possible candidates of minispike and PWN sources in the current Fermi-LAT 3FGL and ATNF catalog, respectively. The diffuse gamma-rays from these sources can be well below the Galactic diffuse gamma-ray backgrounds and less constrained by the Fermi-LAT data, if they are located at the low Galactic latitude regions.
2018
ISSN2470-0010
Volume97Issue:9Pages:91701
Subject AreaAstronomy & Astrophysics ; Physics
MOST Discipline CatalogueAstronomy & Astrophysics ; Physics, Particles & Fields
DOI10.1103/PhysRevD.97.091701
Indexed BySCIE
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Cited Times:8[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.itp.ac.cn/handle/311006/22904
Collection理论物理所科研产出_SCI论文
Affiliation1.[Huang, Xian-Jun
2.Wu, Yue-Liang
3.Zhang, Wei-Hong
4.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
5.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
6.Sichuan Univ Sci & Engn, Zigong 643000, Peoples R China
Recommended Citation
GB/T 7714
Huang, XJ,Wu, YL,Zhang, WH,et al. Origins of sharp cosmic-ray electron structures and the DAMPE excess[J]. PHYSICAL REVIEW D,2018,97(9):91701.
APA Huang, XJ,Wu, YL,Zhang, WH,&Zhou, YF.(2018).Origins of sharp cosmic-ray electron structures and the DAMPE excess.PHYSICAL REVIEW D,97(9),91701.
MLA Huang, XJ,et al."Origins of sharp cosmic-ray electron structures and the DAMPE excess".PHYSICAL REVIEW D 97.9(2018):91701.
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