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dc.contributor.authorZhang, C. M. [UNESP]
dc.date.accessioned2014-05-27T11:19:53Z
dc.date.available2014-05-27T11:19:53Z
dc.date.issued2000-02-01
dc.identifierhttp://dx.doi.org/10.1142/S0218271800000025
dc.identifier.citationInternational Journal of Modern Physics D, v. 9, n. 1, p. 1-12, 2000.
dc.identifier.issn0218-2718
dc.identifier.urihttp://hdl.handle.net/11449/66098
dc.description.abstractConsidering the ferromagnetic screening for the decay of the X-ray neutron star magnetic field in the binary accretion phase, the phase transition of ferromagnetic materials in the crust of neutron star induces the ferromagnetic screening saturation of the accreted crust, which results in the minimum surface magnetic field of the accreting neutron star, about 108 G, if the accreted matter has completely replaced the crust mass of the neutron star. The magnetic field evolution versus accreted mass is given as Bs ∝ ΔM-0.9, and the obtained magnetic field versus spin period relation is consistent with the distribution of the binary X-ray sources and recycled pulsars. The further thermal effect on the magnetic evolution is also studied.en
dc.format.extent1-12
dc.language.isoeng
dc.relation.ispartofInternational Journal of Modern Physics D
dc.sourceScopus
dc.titleThe saturated magnetic field of the neutron starsen
dc.typeArtigo
dcterms.licensehttp://www.worldscientific.com/page/authors/author-rights
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.description.affiliationIFT UNESP, Rua Pamplona 145, 01405-900, Sao Paulo
dc.description.affiliationUnespIFT UNESP, Rua Pamplona 145, 01405-900, Sao Paulo
dc.identifier.doi10.1142/S0218271800000025
dc.identifier.wosWOS:000086862600001
dc.rights.accessRightsAcesso restrito
dc.identifier.scopus2-s2.0-0034401775
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt
dc.relation.ispartofjcr2.171
dc.relation.ispartofsjr1,079
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