KMS of Xinjiang Astronomical Observatory, CAS
| The Impacts of Neutron Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison | |
Zhen, Guoqing1; Lu, Guoliang1,2 ; Liu, Helei1; Dohi, Akira3,4; Nishimura, Nobuya5,6; Zhu, Chunhua1; Song, Liyu1; Wang, Weiyang7,8; Xu, Renxin7,8
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| 2023-06-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 950Issue:2Pages:110 |
| Contribution Rank | 2 |
| Abstract | Type I X-ray bursts are rapidly brightening phenomena triggered by thermonuclear burning on the accreting layers of a neutron star (NS). The light curves represent the physical properties of NSs and the nuclear reactions on the proton-rich nuclei. The numerical treatments of the accreting NS and physics of the NS interior are not established, which shows uncertainty in modeling for observed X-ray light curves. In this study, we investigate theoretical X-ray burst models compared with burst light curves with GS 1826-24 observations. We focus on the impacts of the NS mass and radius and base heating on the NS surface using the MESA code. We find a monotonic correlation between the NS mass and the parameters of the light curve. The higher the mass, the longer the recurrence time and the greater the peak luminosity. While the larger the radius, the longer the recurrence time, the peak luminosity remains nearly constant. In the case of increasing base heating, both the recurrence time and peak luminosity decrease. We also examine the above results with a different numerical code, HERES, based on general relativity and consider the central NS. We find that the burst rate, energy, and strength are almost the same in two X-ray burst codes by adjusting the base heat parameter in MESA (the relative errors less than or similar to 5%), while the duration and rise times are significantly different between (the relative error is possibly similar to 50%). The peak luminosity and the e-folding time change irregularly between two codes for different accretion rates. |
| DOI | 10.3847/1538-4357/accd5f |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | EQUATION-OF-STATE ; THERMAL EVOLUTION ; NUCLEAR PROCESSES ; MODELS ; NUCLEOSYNTHESIS ; MODULES ; CRUST ; O-15(ALPHA,GAMMA)NE-19 ; DISCOVERY ; FLASHES |
| Funding Project | National Natural Science Foundation of China[12263006] ; National Natural Science Foundation of China[U2031204] ; National Natural Science Foundation of China[12163005] ; Natural Science Foundation of Xinjiang Province[2020D01C063] ; Natural Science Foundation of Xinjiang Province[2021D01C075] ; China Manned Space Project[CMS-CSST-2021-A10] ; JSPS Research Fellowship for Young Scientists[22J10448] ; JSPS KAKENHI[19H00693] ; JSPS KAKENHI[20H05648] ; JSPS KAKENHI[21H01087] ; RIKEN Intensive Research Project |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001007552800001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | National Natural Science Foundation of China ; Natural Science Foundation of Xinjiang Province ; China Manned Space Project ; JSPS Research Fellowship for Young Scientists ; JSPS KAKENHI ; RIKEN Intensive Research Project |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/5262 |
| Collection | 中国科学院新疆天文台 射电天文研究室_理论天体物理研究团组 |
| Corresponding Author | Liu, Helei; Dohi, Akira |
| Affiliation | 1.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Peoples R China 2.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Peoples R China 3.Hiroshima Univ, Grad Sch Adv Sci & Engn, Dept Phys, Higashihiroshima, Hiroshima 7398526, Japan 4.RIKEN, Interdisciplinary Theoret & Math Sci Program iTHE, Wako, Saitama 3510198, Japan 5.RIKEN, Astrophys Big Bang Lab, Cluster Pioneering Res, Wako, Saitama 3510198, Japan 6.RIKEN, RIKEN Nishina Ctr Accelerator Based Sci, Wako, Saitama 3510198, Japan 7.Peking Univ, Dept Astron, Beijing 100871, Peoples R China 8.Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China |
| Recommended Citation GB/T 7714 | Zhen, Guoqing,Lu, Guoliang,Liu, Helei,et al. The Impacts of Neutron Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison[J]. ASTROPHYSICAL JOURNAL,2023,950(2):110. |
| APA | Zhen, Guoqing.,Lu, Guoliang.,Liu, Helei.,Dohi, Akira.,Nishimura, Nobuya.,...&Xu, Renxin.(2023).The Impacts of Neutron Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison.ASTROPHYSICAL JOURNAL,950(2),110. |
| MLA | Zhen, Guoqing,et al."The Impacts of Neutron Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison".ASTROPHYSICAL JOURNAL 950.2(2023):110. |
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| Zhen-2023-The Impact（1289KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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