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dc.contributor.authorALPAR, MEHMET ALİ
dc.contributor.authorGugercinoglu, Erbil
dc.date.accessioned2021-03-06T10:36:45Z
dc.date.available2021-03-06T10:36:45Z
dc.date.issued2014
dc.identifier.citationGugercinoglu E., ALPAR M. A. , "VORTEX CREEP AGAINST TOROIDAL FLUX LINES, CRUSTAL ENTRAINMENT, AND PULSAR GLITCHES", ASTROPHYSICAL JOURNAL LETTERS, cilt.788, 2014
dc.identifier.issn2041-8205
dc.identifier.otherav_eb250f3f-76dc-4864-9b5c-c9648b2dc12c
dc.identifier.othervv_1032021
dc.identifier.urihttp://hdl.handle.net/20.500.12627/154449
dc.identifier.urihttps://doi.org/10.1088/2041-8205/788/1/l11
dc.description.abstractA region of toroidally oriented quantized flux lines must exist in the proton superconductor in the core of the neutron star. This region will be a site of vortex pinning and creep. Entrainment of the neutron superfluid with the crustal lattice leads to a requirement of superfluid moment of inertia associated with vortex creep in excess of the available crustal moment of inertia. This will bring about constraints on the equation of state. The toroidal flux region provides the moment of inertia necessary to complement the crust superfluid with postglitch relaxation behavior fitting the observations.
dc.language.isoeng
dc.subjectUzay bilimi
dc.subjectTemel Bilimler
dc.subjectAstronomi ve Astrofizik
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleVORTEX CREEP AGAINST TOROIDAL FLUX LINES, CRUSTAL ENTRAINMENT, AND PULSAR GLITCHES
dc.typeMakale
dc.relation.journalASTROPHYSICAL JOURNAL LETTERS
dc.contributor.departmentSabancı Üniversitesi , ,
dc.identifier.volume788
dc.identifier.issue1
dc.contributor.firstauthorID215069


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