Galactic cosmic-ray model in the light of AMS-02 nuclei data
文献类型：期刊论文
| 作者 | Niu, JS; Li, TJ
|
| 刊名 | PHYSICAL REVIEW D
 |
| 出版日期 | 2018 |
| 卷号 | 97期号:2页码:23015 |
| 关键词 | INTERSTELLAR-MEDIUM SPECTRAL FEATURES BAYESIAN-ANALYSIS DIFFUSION-MODEL HELIUM SPECTRA PROPAGATION GALAXY PROTON TRANSPORT ORIGIN |
| ISSN号 | 2470-0010 |
| DOI | 10.1103/PhysRevD.97.023015 |
| 英文摘要 | Cosmic ray (CR) physics has entered a precision-driven era. With the latest AMS-02 nuclei data (boron-to-carbon ratio, proton flux, helium flux, and antiproton-to-proton ratio), we perform a global fitting and constrain the primary source and propagation parameters of cosmic rays in the Milky Way by considering 3 schemes with different data sets (with and without (p) over bar /p data) and different propagation models (diffusionreacceleration and diffusion-reacceleration-convection models). We find that the data set with (p) over bar /p data can remove the degeneracy between the propagation parameters effectively and it favors the model with a very small value of convection (or disfavors the model with convection). The separated injection spectrum parameters are used for proton and other nucleus species, which reveal the different breaks and slopes among them. Moreover, the helium abundance, antiproton production cross sections, and solar modulation are parametrized in our global fitting. Benefited from the self-consistence of the new data set, the fitting results show a little bias, and thus the disadvantages and limitations of the existed propagation models appear. Comparing to the best fit results for the local interstellar spectra (phi = 0) with the VOYAGER-1 data, we find that the primary sources or propagation mechanisms should be different between proton and helium (or other heavier nucleus species). Thus, how to explain these results properly is an interesting and challenging question. |
| 学科主题 | Astronomy & Astrophysics ; Physics |
| 语种 | 英语 |
| 源URL | [http://ir.itp.ac.cn/handle/311006/22977]  |
| 专题 | 理论物理研究所_理论物理所1978-2010年知识产出 计算平台成果 |
| 作者单位 | 1.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China 2.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China |
| 推荐引用方式 GB/T 7714 | Niu, JS,Li, TJ. Galactic cosmic-ray model in the light of AMS-02 nuclei data[J]. PHYSICAL REVIEW D,2018,97(2):23015. |
| APA | Niu, JS,&Li, TJ.(2018).Galactic cosmic-ray model in the light of AMS-02 nuclei data.PHYSICAL REVIEW D,97(2),23015. |
| MLA | Niu, JS,et al."Galactic cosmic-ray model in the light of AMS-02 nuclei data".PHYSICAL REVIEW D 97.2(2018):23015. |
入库方式： OAI收割
来源：理论物理研究所
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