DEFORMABILITY

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Dependence of the tidal deformability of neutron stars on the nuclear equation of state被引量：2
《Chinese Physics C》2023年第1期160-167,共8页谢文杰 陈建玲 马紫微 郭俊华 祝龙 
Supported by the Shanxi Provincial Foundation for Returned Overseas Scholars(20220037);the Natural Science Foundation of Shanxi Province(20210302123085);the discipline construction project of Yuncheng university;the National Natural Science Foundation of China(12075327)。
Within the Bayesian framework,using an explicitly isospin-dependent parametric equation of state(EOS)for the core of neutron stars(NSs),we studied how the NS EOS behaves when we confront it with the tidal deformabilit...
关键词：symmetry energy equation of state tidal deformability Bayesian inference approach neutron stars 
Chiral phase transition and equation of state in chiral imbalance
《Chinese Physics C》2021年第8期145-152,共8页Qing-Wu Wang Chao Shi Hong-Shi Zong 
Supported by the National Natural Science Foundation of China(11475085,11535005,11690030,11873030,11905104);the Fostering Program in Disciplines Possessing Novel Features for Natural Science(2020SCUNL209)。
The chiral phase transition and equation of state are studied within a novel self-consistent mean-field approximation of the two-flavor Nambu-Jona-Lasinio model.In this newly developed model,modifications to the chemi...
关键词：chiral imbalance critical end point tidal deformability 
Neutron star cooling and GW170817 constraint within quark-meson coupling models
《Chinese Physics C》2021年第2期531-547,共17页Odilon Lourenço César H.Lenzi Mariana Dutra Tobias Frederico M.Bhuyan Rodrigo Negreiros César V.Flores Guilherme Grams Débora P.Menezes 
This work is a part of the projet INCT-FNA Proe.(464898/2014-5),was partially supprted by CNPq(Brazil)(301155.2017-8)(D.P.M.),310242/2017-7,406958/2018-1(O.L),308486/2015-3(T.F.),43369/2018-3(M.D.),by Capes-PNPD program(C.V.F),and by Fundacio de Amparo a Pesquisa do Estado de Sio Paulo(FAPESP)under the thematic projescts 2013/26258-4(OL,TF)and 2017/05660-0(OL,M.D.T.E.).R.N.also acknowledges that this project was parly funded by FAPERJ,under grant E-26/203.2992017.M.B.acknowledge the support from FAPESP Project No.2017/05660-0,and FOSTECT Project No.FOSTECT.2019B.04.PDS acknow ledges support from the UK STFC under projeet number ST/P005314/1。
In the present work,we used five different versions of the quark-meson coupling(QMC)model to compute astrophysical quantities related to the GW170817 event and the neutron star cooling process.Two of the models are ba...
关键词：equation of state compact star cooling in stars quark-meson coupling models tidal deformability neutron star merger 
Key factor for determining relation between radius and tidal deformability of neutron stars: Slope of symmetry energy
《Chinese Physics C》2020年第6期103-108,共6页Nai-Bo Zhang Bin Qi Shou-Yu Wang 
This work is partly Supported by the Shandong Natural Science Foundation(JQ201701);the Natural Science Foundation of China(11622540,11675094,11705102,11775133);the China Postdoctoral Science Foundation(2019M652358);the Young Scholars Program of Shandong University,Weihai(2015WHWLJH01);the Fundamental Research Funds of Shandong University(2019ZRJC001)。
The constraints on tidal deformability Λ of neutron stars were first extracted from GW170817 by LIGO and Virgo Collaborations.However,the relationship between the radius R and tidal deformability Λ is still under de...
关键词：neutron stars symmetry energy tidal deformability RADIUS 
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