Bayesian Analysis of the Hardening in AMS-02 Nuclei Spectra

doi:10.3847/1538-4357/ab0420

CORC > 理论物理研究所 > 中国科学院理论物理研究所 > 理论物理所科研产出 > 理论物理所1978-2010年知识产出

	Bayesian Analysis of the Hardening in AMS-02 Nuclei Spectra
	Niu, Jia-Shu ; Li, TianJun ; Xue, HuiFang
刊名	ASTROPHYSICAL JOURNAL
	2019
卷号	873 期号:1 页码:77
关键词	COSMIC-RAY PROPAGATION RADIAL-DISTRIBUTION CARBON ANTIPROTONS GALAXY CO
ISSN号	0004-637X
DOI	10.3847/1538-4357/ab0420
英文摘要	Based on the precise nuclei data released by AMS-02, we study the spectra hardening of both the primary (proton, helium, carbon, oxygen, and the primary component of nitrogen) and the secondary (anti-proton, lithium, beryllium, boron, and the secondary component of nitrogen) cosmic-ray (CR) nuclei. With the diffusion-reacceleration model, we consider two schemes to reproduce the hardening in the spectra: (i) a high-rigidity break in primary source injection; and (ii) a high-rigidity break in diffusion coefficient. The global fitting results show that both schemes could reproduce the spectra hardening in the current status. More precise multi-TV data (especially the data of secondary CR species) is needed if one wants to distinguish these two schemes. In our global fitting, each of the nuclei species is allocated an independent solar-modulation potential and a rescale factor (which accounts for the isotopic abundance for primary nuclei species and uncertainties of production cross section or inhomogeneity of CR sources and propagation for secondary nuclei species). The fitting values of these two parameter classes show us some hints on some new directions in CR physics. All the fitted rescale factors of primary nuclei species have values that are systematically smaller than 1.0, while that of secondary nuclei species are systematically larger than 1.0. Moreover, both the rescale factor and solar-modulation potential of beryllium have values that are obviously different from other species. This might indicate that beryllium has the specificity not only on its propagation in the heliosphere, but also on its production cross section. All these new results should be seriously studied in the future.
学科主题	Astronomy & Astrophysics
语种	英语
内容类型	期刊论文
源URL	[http://ir.itp.ac.cn/handle/311006/23473]
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.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China 2.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 3.Shanxi Univ, Inst Theoret Phys, State Key Lab Quantum Opt & Quantum Opt Devices, Taiyuan 030006, Peoples R China 4.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, Jia-Shu,Li, TianJun,Xue, HuiFang. Bayesian Analysis of the Hardening in AMS-02 Nuclei Spectra[J]. ASTROPHYSICAL JOURNAL,2019,873(1):77.
APA	Niu, Jia-Shu,Li, TianJun,&Xue, HuiFang.(2019).Bayesian Analysis of the Hardening in AMS-02 Nuclei Spectra.ASTROPHYSICAL JOURNAL,873(1),77.
MLA	Niu, Jia-Shu,et al."Bayesian Analysis of the Hardening in AMS-02 Nuclei Spectra".ASTROPHYSICAL JOURNAL 873.1(2019):77.