Origins of sharp cosmic-ray electron structures and the DAMPE excess
文献类型：期刊论文
| 作者 | Huang, XJ; Zhou, YF ; Zhang, WH; Wu, YL
|
| 刊名 | PHYSICAL REVIEW D
 |
| 出版日期 | 2018 |
| 卷号 | 97期号:9页码:91701 |
| ISSN号 | 2470-0010 |
| 关键词 | DARK-MATTER ANNIHILATION FERMI-LAT CONSTRAINTS SATELLITES EMISSION SEESAW E(-) |
| DOI | 10.1103/PhysRevD.97.091701 |
| 英文摘要 | Nearby 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. |
| 学科主题 | Astronomy & Astrophysics ; Physics |
| 语种 | 英语 |
| 源URL | [http://ir.itp.ac.cn/handle/311006/22904]  |
| 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.Zhang, Wei-Hong 2.Wu, Yue-Liang 3.[Huang, Xian-Jun 4.Sichuan Univ Sci & Engn, Zigong 643000, Peoples R China 5.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 6.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China |
| 推荐引用方式 GB/T 7714 | Huang, XJ,Zhou, YF,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,Zhou, YF,Zhang, WH,&Wu, YL.(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. |
入库方式： OAI收割
来源：理论物理研究所
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