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Mutual influence of magnetic field decay and thermal evolution of rotational neutron stars
Zhou,Xia1; Kang, Miao2; Wang Na2
2013-02-21
Conference NameNeutron Stars and Pulsars: Challenges and Opportunities after 80 years
Source PublicationProceedings of the International Astronomical Union, Symposium S291
Pages586-588
Conference Date20–24 August, 2012
Correspondent Emailzhouxia@xao.ac.cn ; kangmiao07@gmail.com ; na.wang@xao.ac.cn
Conference PlaceBeijing, China
PublisherCambridge
AbstractThe effect of magnetic field decay on the chemical heating and thermal evolution of neutron stars is discussed. Our main goal is to study how chemical heating mechanisms and thermal evolution are changed by field decay and how magnetic field decay is modified by the thermal evolution. We show that the effect of chemical heating is suppressed by the star spin-down through decaying magnetic field at a later stage; magnetic field decay is delayed significantly relative to stars cooling without heating mechanisms; compared to typical chemical heating, the decay of the magnetic field can even cause the temperature to turn down at a later stage.
Funding OrganizationIAU ; IAU
KeywordStars: Evolution Stars: Magnetic Fields Stars: Neutron Stars: Rotation Radiation Mechanisms: Thermal
Subject Area致密天体、高能和基础物理
DOI10.1017/S1743921313000045
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Indexed By其他
Funding Project脉冲星研究团组
Language英语
ISBN978-1-107-03380-1
ISSN1743-9213
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Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/397
Collection射电天文研究室_脉冲星研究团组
射电天文研究室
其它
Corresponding AuthorZhou,Xia
Affiliation1.Xinjiang Astronomical Observatory, CAS, 150, Science 1-Street, Urumqi, 830011, China Key Laboratory of Radio Astronomy, CAS, Urumqi, 830011, China
2.College of Physics and Electronics, Henan University, Kaifeng, Henan 475004, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhou,Xia,Kang, Miao,Wang Na. Mutual influence of magnetic field decay and thermal evolution of rotational neutron stars[C]:Cambridge,2013:586-588.
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