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Glitches in four gamma-ray pulsars and inferences on the neutron star structure
Gugercinoglu, E.1,2; Ge, M. Y.3; Yuan, J. P.4,5; Zhou, S. Q.6
2022-02-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume511Issue:1Pages:425-439
Contribution Rank4
AbstractWe present timing solutions from the Fermi-LAT observations of gamma-ray pulsars PSR J0835 - 4510 (Vela), PSR J1023-5746, PSR J2111+4606, and PSR J2229+6114. Data ranges for each pulsar extend over a decade. From data analysis, we have identified a total of 20 glitches, 11 of which are new discoveries. Among them, 15 glitches are large ones with Delta nu/nu greater than or similar to 10(-6). PSR J1023-5746 is the most active pulsar with glitch activity parameter being A(g) = 14.5 x 10(-7) yr(-1) in the considered data span and should be a target for frequently glitching Vela-like pulsars in future observations. We have done fits within the framework of the vortex creep model for 16 glitches with Delta nu/nu greater than or similar to 10(-7). By theoretical analysis of these glitches, we are able to obtain important information on the structure of neutron star, including moments of inertia of the superfluid regions participated in glitches and coupling time-scales between various stellar components. The theoretical prediction for the time to the next glitch from the parameters of the previous one is found to be in qualitative agreement with the observed inter-glitch time-scales for the considered sample. Recoupling time-scales of the crustal superfluid are within the range of theoretical expectations and scale inversely with the spin-down rate of a pulsar. We also determined a braking index n = 2.63(30) for PSR J2229+6114 after glitch-induced contributions have been removed.
Keywordstars: neutron pulsars: general pulsars: individual: PSR J0835-4510 (Vela) pulsars: individual: PSR J1023-5746 pulsars: individual: PSR J2111+4606 pulsars: individual: PSR J2229+6114
DOI10.1093/mnras/stac026
Indexed BySCI
Language英语
WOS KeywordEQUATION-OF-STATE ; VORTEX CREEP ; SPIN-UP ; BRAKING INDEX ; RADIO PULSARS ; VELA PULSAR ; HIGH-ENERGY ; INTERNAL TEMPERATURE ; SUPERFLUID CORE ; MAGNETIC-FIELD
Funding ProjectScientific and Technological Research Council of Turkey (TuBTAK)[117F330] ; National Natural Science Foundation of China[U1838201] ; National Natural Science Foundation of China[U1838202] ; National Natural Science Foundation of China[U1838104] ; National Natural Science Foundation of China[U1938103] ; National Natural Science Foundation of China[U1938109] ; National Natural Science Foundation of China[11873080]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000770033900025
PublisherOXFORD UNIV PRESS
Funding OrganizationScientific and Technological Research Council of Turkey (TuBTAK) ; National Natural Science Foundation of China
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Cited Times:18[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4597
Collection射电天文研究室_脉冲星研究团组
Corresponding AuthorGugercinoglu, E.; Ge, M. Y.
Affiliation1.Hekim Tahsin St 7, TR-34467 Istanbul, Turkey
2.Sabanci Univ, Fac Engn & Nat Sci, TR-34956 Istanbul, Turkey
3.Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
5.Chinese Acad Sci, Ctr Astron Megasci, Beijing 100012, Peoples R China
6.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China
Recommended Citation
GB/T 7714
Gugercinoglu, E.,Ge, M. Y.,Yuan, J. P.,et al. Glitches in four gamma-ray pulsars and inferences on the neutron star structure[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2022,511(1):425-439.
APA Gugercinoglu, E.,Ge, M. Y.,Yuan, J. P.,&Zhou, S. Q..(2022).Glitches in four gamma-ray pulsars and inferences on the neutron star structure.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,511(1),425-439.
MLA Gugercinoglu, E.,et al."Glitches in four gamma-ray pulsars and inferences on the neutron star structure".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 511.1(2022):425-439.
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