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Equation of state and surface thermal emission of magnetized white dwarfs
Gao, Zhi Fu1,2; Wang, Hui3; Zhao, Xin Jun2,6; Yang, Xiao Feng1,4,5
2023-01
Source PublicationASTRONOMISCHE NACHRICHTEN
ISSN0004-6337
Volume344Issue:1-2Pages:e220112
Contribution Rank1
AbstractThe observation and theoretical study of massive magnetized white dwarfs is one of the most important topics in the field of astronomy. This paper aims to obtain a coupled magneto-thermal evolution model of magnetized white dwarfs (B-WDs). As a fiducial model, we choose a non-magnetized WD with a baryonic mass M-0 = 1.37 M-? (M-? is the solar mass) for comparison with the magnetized cases. Firstly, we give an overview of the WD cooling, then study the equation of the state of a B-WD. We find that the WD mass increases with magnetic field strength B, while its radius decreases with B, and the minimum of B required to reach the Chandrasecka limit is about 3.2 x 10(14) G. Finally, by introducing the magnetic-to-thermal conversion coefficient xi, and taking the temperature effect on the stellar radius into consideration, we calculate the luminosities of thermal photons L-ph and surface effective temperature, T-eff due to Ohmic dissipation for B-WDs. According to our calculations, magnetic field decay can definitely maintain a long-term thermal evolution for massive B-WDs. This study will be useful for the study of internal thermal evolution and internal stability of B-WDs in the future.
Keywordequation of state magnetized white dwarf magneto-thermal evolution Ohmic dissipation
DOI10.1002/asna.20220112
Indexed BySCI
Language英语
WOS KeywordFIELD ; EVOLUTION ; STARS
Funding ProjectChinese National Science Foundation[12041304] ; CAS Pioneer Hundred Talents Program
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000903870100001
PublisherWILEY-V C H VERLAG GMBH
Funding OrganizationChinese National Science Foundation ; CAS Pioneer Hundred Talents Program
Conference Name10th International Workshop on Astronomy and Relativistic Astrophysics: from Quarks to Cosmos
Conference PlaceHotel Soleil La Antigua, Antigua Guatemala, Guatemala
Conference Date5-9 September 2022
Citation statistics
Cited Times:8[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/5000
Collection射电天文研究室_脉冲星研究团组
射电天文研究室_星系宇宙学研究团组
Corresponding AuthorZhao, Xin Jun
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Xinjiang, Peoples R China
2.Yili Normal Univ, Coll Phys Sci & Technol, Xinjiang Lab Phase Transit & Microstruct Condensed, Yining, Xinjiang, Peoples R China
3.Yuncheng Univ, Dept Phys & Elect Engn, Yuncheng, Peoples R China
4.Univ Roma La Sapienza, ICRA & Dipartimento Fis, Rome, Italy
5.Int Ctr Relativist Astrophys Network, Piazza Repubbl 10, Pescara, Italy
6.Yili Normal Univ, Coll Phys Sci & Technol, Xinjiang Labortory Phase Transit & Microstruct Con, Yining 835000, Xinjiang, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Gao, Zhi Fu,Wang, Hui,Zhao, Xin Jun,et al. Equation of state and surface thermal emission of magnetized white dwarfs[J]. ASTRONOMISCHE NACHRICHTEN,2023,344(1-2):e220112.
APA Gao, Zhi Fu,Wang, Hui,Zhao, Xin Jun,&Yang, Xiao Feng.(2023).Equation of state and surface thermal emission of magnetized white dwarfs.ASTRONOMISCHE NACHRICHTEN,344(1-2),e220112.
MLA Gao, Zhi Fu,et al."Equation of state and surface thermal emission of magnetized white dwarfs".ASTRONOMISCHE NACHRICHTEN 344.1-2(2023):e220112.
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