Neutron star equation of state: Quark mean-field (QMF) modeling and applications

doi:10.1016/j.jheap.2020.07.001

	Neutron star equation of state: Quark mean-field (QMF) modeling and applications
	Li, A.2; Zhu, Z. -Y.2,3; Zhou, E. -P.4; Dong, J. -M.1; Hu, J. -N.5,6; Xia, C. -J.7,8
刊名	JOURNAL OF HIGH ENERGY ASTROPHYSICS
	2020-11-01
卷号	28 页码:19-46
ISSN号	2214-4048
DOI	10.1016/j.jheap.2020.07.001
通讯作者	Li, A.(liang@xmu.edu.cn)
英文摘要	Because of the development of many-body theories of nuclear matter, the long-standing, open problem of the equation of state (EOS) of dense matter may be understood in the near future through the confrontation of theoretical calculations with laboratory measurements of nuclear properties & reactions and increasingly accurate observations in astronomy. In this review, we focus on the following six aspects: 1) providing a survey of the quark mean-field (QMF) model, which consistently describes a nucleon and many-body nucleonic system from a quark potential; 2) applying QMF to both nuclear matter and neutron stars; 3) extending QMF formalism to the description of hypernuclei and hyperon matter, as well as hyperon stars; 4) exploring the hadron-quark phase transition and hybrid stars by combining the QMF model with the quark matter model characterized by the sound speed; 5) constraining interquark interactions through both the gravitational wave signals and electromagnetic signals of binary merger event GW170817; and 6) discussing further opportunities to study dense matter EOS from compact objects, such as neutron star cooling and pulsar glitches. (C) 2020 The Authors. Published by Elsevier B.V.
资助项目	National Natural Science Foundation of China[11873040] ; National Natural Science Foundation of China[11775276] ; National Natural Science Foundation of China[11705163] ; National Natural Science Foundation of China[11775119] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Natural Science Foundation of Tianjin ; China Scholarship Council[201906205013] ; Ningbo Natural Science Foundation[2019A610066]
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	ELSEVIER
WOS记录号	WOS:000598688300003
资助机构	National Natural Science Foundation of China ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Natural Science Foundation of Tianjin ; China Scholarship Council ; Ningbo Natural Science Foundation
内容类型	期刊论文
源URL	[http://119.78.100.186/handle/113462/138489]
专题	中国科学院近代物理研究所
通讯作者	Li, A.
作者单位	1.Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China 2.Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China 3.Inst Theoret Phys, D-60438 Frankfurt, Germany 4.Albert Einstein Inst, Max Planck Inst Gravitat Phys, Muhlenberg 1, D-14476 Potsdam, Germany 5.Nankai Univ, Sch Phys, Tianjin 300071, Peoples R China 6.RIKEN Nishina Ctr, Strangeness Nucl Phys Lab, Wako, Saitama 3510198, Japan 7.Zhejiang Univ, Sch Informat Sci & Engn, Ningbo Inst Technol, Ningbo 315100, Peoples R China 8.Japan Atom Energy Res Inst, Adv Sci Res Ctr, Tokai, Ibaraki 3191195, Japan
推荐引用方式 GB/T 7714	Li, A.,Zhu, Z. -Y.,Zhou, E. -P.,et al. Neutron star equation of state: Quark mean-field (QMF) modeling and applications[J]. JOURNAL OF HIGH ENERGY ASTROPHYSICS,2020,28:19-46.
APA	Li, A.,Zhu, Z. -Y.,Zhou, E. -P.,Dong, J. -M.,Hu, J. -N.,&Xia, C. -J..(2020).Neutron star equation of state: Quark mean-field (QMF) modeling and applications.JOURNAL OF HIGH ENERGY ASTROPHYSICS,28,19-46.
MLA	Li, A.,et al."Neutron star equation of state: Quark mean-field (QMF) modeling and applications".JOURNAL OF HIGH ENERGY ASTROPHYSICS 28(2020):19-46.