Neutron star cooling and GW170817 constraint within quark-meson coupling models

作     者：Odilon Lourenço César H.Lenzi Mariana Dutra Tobias Frederico M.Bhuyan Rodrigo Negreiros César V.Flores Guilherme Grams Débora P.Menezes Odilon Lourengo;César H.Lenzi;Mariana Dutra;Tobias Frederico;M.Bhuyan;Rodrigo Negreiros;César V.Flores;Guilherme Grams;Débora P.Menezes

作者机构：Departamento de FísicaInstituto Tecnológico de AeronáuticaDCTA12228-900São Josédos CamposSPBrazil Department of PhysicsFaculty of ScienceUniversity of MalayaKuala Lumpur 50603Malaysia Atomic Molecular and Optical Research GroupAdvanced Institute of Materials ScienceTon Duc Thang UniversityHo Chi Minh CityVietnam Faculty of Applied SciencesTon Duc Thang UniversityHo Chi Minh CityVietnam Instituto de FísicaUniversidade Federal Fluminense 20420NiteróiRJBrazil Centro de Ciências ExatasNaturais e TecnológicasUEMASULRua Godofredo Viana 1300Centro CEP:65901-480ImperatrizMaranhãoBrazil Departamento de FísicaUniversidade Federal de Santa CatarinaFlorianópolisSCCP 476CEP 88.040-900Brazil Univ.LyonUniv.Claude Bernard Lyon 1CNRS/IN2P3IP2I LyonUMR 5822F-69622VilleurbanneFrance 

出 版 物：《Chinese Physics C》 (中国物理C（英文版）)

年 卷 期：2021年第45卷第2期

页      面：531-547页

核心收录：

学科分类：0709[理学-地质学] 07[理学] 0708[理学-地球物理学] 0804[工学-仪器科学与技术] 070401[理学-天体物理] 0827[工学-核科学与技术] 0703[理学-化学] 0704[理学-天文学] 0702[理学-物理学] 

基　　金：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 

主　　题：equation of state compact star cooling in stars quark-meson coupling models tidal deformability neutron star merger 

摘      要：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 *** of the models are based on the original bag potential structure and three versions consider a harmonic oscillator potential to confine *** bag-like models also incorporate the pasta phase used to describe the inner crust of neutron *** a simple method studied in the present work,we show that the pasta phase does not play a significant ***,the QMC model that satisfies the GW170817 constraints with the lowest slope of the symmetry energy exhibits a cooling profile compatible with observational data.