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Constraining a relativistic mean field model using neutron star mass–radius measurements I: nucleonic models

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成果类型:
期刊论文
作者:
Chun Huang*;Geert Raaijmakers;Anna L Watts;Laura Tolos;Constança Providência
通讯作者:
Chun Huang
作者机构:
[Constança Providência] CFisUC, Department of Physics, University of Coimbra , P-3004-516 Coimbra , Portugal
[Geert Raaijmakers] GRAPPA, University of Amsterdam , Science Park 904, 1098 XH Amsterdam , the Netherlands
[Anna L Watts] Anton Pannekoek Institute for Astronomy, University of Amsterdam , Science Park 904, 1090 GE Amsterdam , the Netherlands
Institute of Space Sciences (ICE , CSIC), Campus UAB, Carrer de Can Magrans E-08193, Barcelona , Spain
Institut d’Estudis Espacials de Catalunya (IEEC) , E-08034, Barcelona , Spain
通讯机构:
[Chun Huang] P
Physics Department, Central China Normal University , Luoyu Road, 430030 Wuhan , China<&wdkj&>Anton Pannekoek Institute for Astronomy, University of Amsterdam , Science Park 904, 1090 GE Amsterdam , the Netherlands<&wdkj&>Physics Department, Washington University , One Brookings Drive, St. Louis, MO 63130 , USA
语种:
英文
关键词:
dense matter;equation of state;stars: neutron;X-rays: general
期刊:
Monthly Notices of the Royal Astronomical Society
ISSN:
0035-8711
年:
2024
卷:
529
期:
4
页码:
4650-4665
机构署名:
本校为通讯机构
院系归属:
物理科学与技术学院
摘要:
Measurements of neutron star mass and radius or tidal deformability deliver unique insight into the equation of state (EOS) of cold dense matter. EOS inference is very often done using generalized parametric or non-parametric models, which deliver no information on composition. In this paper, we consider a microscopic nuclear EOS model based on a field theoretical approach. We show that current measurements from NICER and gravitational wave observations constrain primarily the symmetric nuclear matter EOS. We then explore what could be delivered by measurements of mass and radius at the level ...

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