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A strange star scenario for the formation of isolated millisecond pulsars
Jiang, Long1,2,3; Wang, Na1; Chen, Wen-Cong2,3; Li, Xiang-Dong3; Liu, Wei-Min2; Gao, Zhi-Fu1
2020-01-09
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume633Pages:A45
Contribution Rank1
AbstractAccording to the recycling model, neutron stars in low-mass X-ray binaries were spun up to millisecond pulsars (MSPs), which indicates that all MSPs in the Galactic plane ought to be harbored in binaries. However, about 20% Galactic field MSPs are found to be solitary. To interpret this problem, we assume that the accreting neutron star in binaries may collapse and become a strange star when it reaches some critical mass limit. Mass loss and a weak kick induced by asymmetric collapse during the phase transition (PT) from neutron star to strange star can result in isolated MSPs. In this work, we use a population-synthesis code to examine the PT model. The simulated results show that a kick velocity of similar to 60 km s(-1) can produce similar to 6x10(3) isolated MSPs and birth rate of similar to 6.6x10(-7) yr(-1) in the Galaxy, which is approximately in agreement with predictions from observations. For the purpose of comparisons with future observation, we also give the mass distributions of radio and X-ray binary MSPs, along with the delay time distribution.
Keywordstars: evolution stars: neutron pulsars: general
DOI10.1051/0004-6361/201935132
Indexed BySCI
Language英语
WOS KeywordACCRETION-INDUCED COLLAPSE ; EQUATION-OF-STATE ; MAGNETIC NEUTRON-STARS ; X-RAY BINARIES ; LOW-MASS ; POPULATION SYNTHESIS ; QUARK DECONFINEMENT ; EVOLUTION ; ORIGIN ; RADIO
Funding ProjectCAS Light of West China Program[2018-XBQNXZ-B-022] ; National Natural Science Foundation of China[11573016] ; National Natural Science Foundation of China[11733009] ; National Natural Science Foundation of China[11773015] ; National Natural Science Foundation of China[11803018] ; National Natural Science Foundation of China[U1731103] ; National Natural Science Foundation of China[11463004] ; National Natural Science Foundation of China[11605110] ; National Key Research and Development Program of China[2016YFA0400803] ; National Key Research and Development Program of China[2016YFA0400804] ; Scientific Research Fund of Hunan Provincial Education Department[16B250] ; Scientific Research Fund of Hunan Provincial Education Department[16C1531] ; Program for Innovative Research Team (in Science and Technology) at the University of Henan Province
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000506362500001
PublisherEDP SCIENCES S A
Funding OrganizationCAS Light of West China Program ; National Natural Science Foundation of China ; National Key Research and Development Program of China ; Scientific Research Fund of Hunan Provincial Education Department ; Program for Innovative Research Team (in Science and Technology) at the University of Henan Province
Citation statistics
Cited Times:8[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/3313
Collection射电天文研究室_脉冲星研究团组
Corresponding AuthorWang, Na
Affiliation1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
2.Shangqiu Normal Univ, Sch Phys & Elect Informat, Shangqiu 476000, Henan, Peoples R China
3.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210046, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Jiang, Long,Wang, Na,Chen, Wen-Cong,et al. A strange star scenario for the formation of isolated millisecond pulsars[J]. ASTRONOMY & ASTROPHYSICS,2020,633:A45.
APA Jiang, Long,Wang, Na,Chen, Wen-Cong,Li, Xiang-Dong,Liu, Wei-Min,&Gao, Zhi-Fu.(2020).A strange star scenario for the formation of isolated millisecond pulsars.ASTRONOMY & ASTROPHYSICS,633,A45.
MLA Jiang, Long,et al."A strange star scenario for the formation of isolated millisecond pulsars".ASTRONOMY & ASTROPHYSICS 633(2020):A45.
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