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The simulation of the magnetic field and spin period evolution of accreting neutron stars
Pan YY(潘元月); Song LM(宋黎明); Pan, YY; Song, LM; Zhang, CM; Guo, YQ
2015
发表期刊ASTRONOMISCHE NACHRICHTEN
卷号336期号:4页码:370-377
通讯作者潘元月
文章类型Article
摘要By means of the Monte Carlo method, we simulate the evolutionary distribution of accreting neutron stars (NSs) in the magnetic field versus spin period (B-P) diagram where the accretion induced magnetic-field decay model is exploited. The simulated results show that by mass accretion the B-P distribution of the accreting NS would evolve along the equilibrium period line to a region with low field and short period. The B-P distributions of the simulated accreting NSs are consistent with those of the observed millisecond pulsars (MSPs) after accretion of approximate to 0.1-0.2 M. We also test the effects of the initial magnetic field and the spin period on the evolved B-P distribution of the accreting NSs. It is shown that the evolved distributions of the simulated samples are independent of the selection of the initial condition when the NS magnetic field decays to a value less than approximate to 10(10) G. ((c) 2015 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)
关键词pulsars: general stars: binaries stars: evolution X-rays: binaries
学科领域Astronomy & Astrophysics
DOI10.1002/asna.201412168
收录类别SCI ; CA
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000355980200005
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被引频次:3[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/228464
专题粒子天体物理中心
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Pan YY,Song LM,Pan, YY,et al. The simulation of the magnetic field and spin period evolution of accreting neutron stars[J]. ASTRONOMISCHE NACHRICHTEN,2015,336(4):370-377.
APA 潘元月,宋黎明,Pan, YY,Song, LM,Zhang, CM,&Guo, YQ.(2015).The simulation of the magnetic field and spin period evolution of accreting neutron stars.ASTRONOMISCHE NACHRICHTEN,336(4),370-377.
MLA 潘元月,et al."The simulation of the magnetic field and spin period evolution of accreting neutron stars".ASTRONOMISCHE NACHRICHTEN 336.4(2015):370-377.
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