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Rotating Massive Strangeon Stars and X-Ray Plateau of Short GRBs

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成果类型:
期刊论文
作者:
Yang, Xi-Yan;Lai, Xiao-Yu;Tan, Wei-Wei;Xu, Ren-Xin
通讯作者:
Lai, XY
作者机构:
[Yang, Xi-Yan] Yangtze Univ, Sch Phys & Optoelect Engn, Jingzhou 434023, Peoples R China.
[Lai, Xiao-Yu; Tan, Wei-Wei; Yang, Xi-Yan] Hubei Univ Educ, Res Ctr Astron, Wuhan 430205, Peoples R China.
[Tan, Wei-Wei] Cent China Normal Univ, Key Lab Quark & Lepton Phys, Minist Educ, Wuhan 430079, Peoples R China.
[Xu, Ren-Xin] Peking Univ, Sch Phys, Beijing 100871, Peoples R China.
[Xu, Ren-Xin] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China.
通讯机构:
[Lai, XY ] H
Hubei Univ Educ, Res Ctr Astron, Wuhan 430205, Peoples R China.
语种:
英文
关键词:
dense matter;(stars:) pulsars: general;(stars:) gamma-ray burst: general
期刊:
天文和天体物理学研究:英文版
ISSN:
1674-4527
年:
2024
卷:
24
期:
3
页码:
035005
基金类别:
supported by the National SKA Program of China(Nos.2020SKA0120300,2020SKA0120100) the Outstanding Young and Middle-aged Science and Technology Innovation Teams from Hubei colleges and universities(No.T2021026) the Young Top-notch Talent Cultivation Program of Hubei Province,and the Key Laboratory Opening Fund(MOE)of China(grant No.QLPL2021P01)。
机构署名:
本校为其他机构
院系归属:
物理科学与技术学院
摘要:
Strangeon stars, which are proposed to describe the nature of pulsar-like compact stars, have passed various observational tests. The maximum mass of a non-rotating strangeon star could be high, which implies that the remnants of binary strangeon star mergers could even be long-lived massive strangeon stars. We study rigidly rotating strangeon stars in the slowly rotating approximation, using the Lennard-Jones model for the equation of state. Rotation can significantly increase the maximum mass of strangeon stars with unchanged baryon numbers, enlarging the mass-range of long-lived strangeon s...
摘要(中文):
Strangeon stars,which are proposed to describe the nature of pulsar-like compact stars,have passed various obs...展开更多 Strangeon stars,which are proposed to describe the nature of pulsar-like compact stars,have passed various observational tests.The maximum mass of a non-rotating strangeon star could be high,which implies that the remnants of binary strangeon star mergers could even be long-lived massive strangeon stars.We study rigidly rotating strangeon stars in the slowly rotating approximation,using the Lennard-Jones model for the equati...

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