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成果类型:
期刊论文
作者:
Li, Jie;Yang, Bo;Wang, Yu;Lin, Wenbin
通讯作者:
Lin, WB
作者机构:
[Li, Jie] Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.
[Lin, Wenbin; Yang, Bo; Lin, WB] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
[Wang, Yu] Univ Rome, Dip Fis, ICRA, Ple Aldo Moro 5, I-00185 Rome, Italy.
[Lin, Wenbin] Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Peoples R China.
通讯机构:
[Lin, WB ] U
Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
语种:
英文
关键词:
Quark stars;Massive gravity;MIT bag model;Tolman-Oppenheimer-Volkoff equation
期刊:
Physics of the Dark Universe
ISSN:
2212-6864
年:
2023
卷:
42
页码:
101308
基金类别:
CRediT authorship contribution statement Jie Li: Model, Simulation, Investigation, Analysis, Writing – original draft. Bo Yang: Investigation, Analysis, Discussion, Writing – original draft. Yu Wang: Discussion, Writing – review & editing. Wenbin Lin: Conceptualization, acquisition, Resources, Supervision, Writing – review & editing.
机构署名:
本校为第一且通讯机构
院系归属:
核科学技术学院
数理学院
摘要:
We investigate the structure of quark stars in de Rham-Gabadadze-Tolley like massive gravity with an anisotropic matter source. The MIT bag model as the equation of state for compact stars is used to numerically solve the modified Tolman-Oppenheimer-Volkoff equation. We analyze the effects of bag constant, anisotropy parameter and massive gravity parameters on the structure of quark stars. The results show that the mass and radius of the quark star depend on these parameters significantly, and the maximum mass can satisfy the observational data for the massive pulsar PSR J0348+0432. Furthermor...

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