PAMELA data and leptonically decaying dark matter
文献类型：期刊论文
| 作者 | Yin, PF ; Yuan Q(袁强); Zhang J(张娟); Bi XJ(毕效军); Zhang XM(张新民); Yuan, Q; Liu, J; Zhang, J; Bi, XJ; Zhu, SH
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| 刊名 | PHYSICAL REVIEW D
 |
| 出版日期 | 2009 |
| 卷号 | 79期号:2页码:23512 |
| 通讯作者 | [Yin, Peng-fei ; Liu, Jia ; Zhu, Shou-hua] Peking Univ, Inst Theoret Phys, Beijing 100871, Peoples R China ; [Yin, Peng-fei ; Liu, Jia ; Zhu, Shou-hua] Peking Univ, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China ; [Yuan, Qiang ; Zhang, Juan ; Bi, Xiao-jun] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China ; [Bi, Xiao-jun] Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China ; [Bi, Xiao-jun ; Zhu, Shou-hua] Chinese Acad Sci, Kavli Inst Theoret Phys China, Beijing 100190, Peoples R China ; [Zhang, Xinmin] Chinese Acad Sci, Inst High Energy Phys, Div Theoret, Beijing 100049, Peoples R China |
| 英文摘要 | Recently PAMELA released their first results on the positron and antiproton ratios. Stimulated by the new data, we studied the cosmic ray propagation models and calculated the secondary positron and antiproton spectra. The low energy positron ratio can be consistent with data in the convection propagation model. Above similar to 10 GeV PAMELA data shows a clear excess on the positron ratio. However, the secondary antiproton is roughly consistent with the data. The positron excess may be evidence of dark matter annihilation or decay. We compare the positron and antiproton spectra with the data by assuming that dark matter annihilates or decays into different final states. The PAMELA data actually excludes quark pairs being the main final states, and disfavors gauge boson final states. Only in the case of leptonic final states can the positron and antiproton spectra be explained simultaneously. We also compare the decaying and annihilating dark matter scenarios which can account for the PAMELA results and find that the decaying dark matter is preferred. Finally, we consider a decaying neutralino dark matter model in the frame of supersymmetry with R-parity violation. The PAMELA data is well fitted with a neutralino mass of 600 similar to 2000 GeV and a lifetime of similar to 10(26) seconds. We also demonstrate that a neutralino with mass around 2 TeV can fit PAMELA and ATIC data simultaneously. |
| 学科主题 | Astronomy & Astrophysics; Physics |
| 类目[WOS] | Astronomy & Astrophysics ; Physics, Particles & Fields |
| 研究领域[WOS] | Astronomy & Astrophysics ; Physics |
| 原文出处 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000262979800022 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/240495]  |
| 专题 | 高能物理研究所_粒子天体物理中心 高能物理研究所_实验物理中心 |
| 作者单位 | 中国科学院高能物理研究所 |
| 推荐引用方式 GB/T 7714 | Yin, PF,Yuan Q,Zhang J,et al. PAMELA data and leptonically decaying dark matter[J]. PHYSICAL REVIEW D,2009,79(2):23512. |
| APA | Yin, PF.,袁强.,张娟.,毕效军.,张新民.,...&Zhang, XM.(2009).PAMELA data and leptonically decaying dark matter.PHYSICAL REVIEW D,79(2),23512. |
| MLA | Yin, PF,et al."PAMELA data and leptonically decaying dark matter".PHYSICAL REVIEW D 79.2(2009):23512. |
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来源：高能物理研究所
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