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Radiation properties of the accretion disk around a black hole in Einstein-Maxwell-scalar theory

作     者:Mirzabek Alloqulov Sanjar Shaymatov Bobomurat Ahmedov Abdul Jawad 

作者机构:New Uzbekistan UniversityMovarounnahr street 1Tashkent 100000Uzbekistan Institute of Fundamental and Applied ResearchNational Research University TIIAMEKori Niyoziy 39Tashkent 100000Uzbekistan University of Tashkent for Applied SciencesStr.Gavhar 1Tashkent 100149Uzbekistan Institute for Theoretical Physics and CosmologyZhejiang University of TechnologyHangzhou 310023China Central Asian UniversityMilliy Bog Street 264Tashkent 111221Uzbekistan National University of UzbekistanTashkent 100174Uzbekistan Power Engineering FacultyTashkent State Technical UniversityTashkent 100095Uzbekistan Ulugh Beg Astronomical InstituteAstronomy St 33Tashkent 100052Uzbekistan Institute of Theoretical PhysicsNational University of UzbekistanTashkent 100174Uzbekistan Department of MathematicsCOMSATS University IslamabadLahore CampusLahore-54000Pakistan 

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

年 卷 期:2024年第48卷第2期

页      面:162-170页

核心收录:

学科分类:07[理学] 070401[理学-天体物理] 0704[理学-天文学] 0702[理学-物理学] 

基  金:Supported by the National Natural Science Foundation of China (11675143, 11975203) the National Key Research and Development Program of China(2020YFC2201503) 

主  题:Einstein-Maxwell-scalar theory black hole accretion disk 

摘      要:In this study,we explore the properties of a non-rotating black hole in the Einstein-Maxwell-scalar(EMS)theory and investigate the luminosity of the accretion disk surrounding *** determine all the orbital parameters of particles in the accretion disk,including the radius of the innermost stable circular orbit(ISCO)with angular velocity,angular momentum,and ***,we study the radiative efficiency for different values of black hole ***,we analyze the flux,differential luminosity,and temperature of the accretion disk.

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