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The magnetar crustal magneto-thermal evolution
Wang, Hui1; Li, Zhi Bing2; Yang, Xiao Feng3,4,5; Song, Dong Ling6
2024-01-25
Source PublicationASTRONOMISCHE NACHRICHTEN
ISSN0004-6337
Volume345Issue:2-3Pages:e240011
Contribution Rank3
AbstractMagnetars are a type of pulsars powered by magnetic field energy. Part of the X-ray luminosities of magnetars in quiescence have a thermal origin and can be fitted by a blackbody spectrum with the surface temperature, much higher than the typical values for rotation-powered pulsars. The persistent thermal emissions and bursts of magnetars indicate the presence of some internal heat sources in their outer crusts. In this work, we have formulated the energy balance equation and applied it to investigate the thermal evolution in the magnetar crust, taking into account the heating mechanisms of Ohmic decay and electron capture processes. This model can explain the changes in the X-ray luminosity of the magnetars.
Keywordmagnetars magneto-thermal evolution Ohmic dissipation
DOI10.1002/asna.20240011
Indexed BySCI
Language英语
WOS Keyword2.25/8.60 GHZ OBSERVATIONS ; NEUTRON-STARS ; X-RAY ; INTERSTELLAR SCINTILLATION ; SINGLE-PULSE ; REPEATERS ; FIELDS ; DECAY
Funding ProjectNational SKA Program of China ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi[2021L480] ; Research Initiation Grant for doctor of Yuncheng University[YQ-2021027] ; Special Scientific Research Project of Excellent Doctors in Shanxi[QZX-2022003] ; [2022SKA0110203]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:001148642700001
PublisherWILEY-V C H VERLAG GMBH
Funding OrganizationNational SKA Program of China ; Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi ; Research Initiation Grant for doctor of Yuncheng University ; Special Scientific Research Project of Excellent Doctors in Shanxi
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5762
Collection射电天文研究室_理论天体物理研究团组
Corresponding AuthorYang, Xiao Feng
Affiliation1.Yuncheng Univ, Dept Phys & Elect Engn, Yuncheng, Peoples R China
2.Hunan Univ Sci & Engn, Coll Sci, Yongzhou, Hunan, Peoples R China
3.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
4.Univ Roma La Sapienza, ICRA, Rome, Italy
5.Univ Roma Sapienza, Dipartimento Fis, Rome, Italy
6.Informat Engn Univ, Basic Dept, Phys Teaching & Res Off, Zhengzhou, Henan, Peoples R China
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Wang, Hui,Li, Zhi Bing,Yang, Xiao Feng,et al. The magnetar crustal magneto-thermal evolution[J]. ASTRONOMISCHE NACHRICHTEN,2024,345(2-3):e240011.
APA Wang, Hui,Li, Zhi Bing,Yang, Xiao Feng,&Song, Dong Ling.(2024).The magnetar crustal magneto-thermal evolution.ASTRONOMISCHE NACHRICHTEN,345(2-3),e240011.
MLA Wang, Hui,et al."The magnetar crustal magneto-thermal evolution".ASTRONOMISCHE NACHRICHTEN 345.2-3(2024):e240011.
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