Neutron Star Magnetic Field as for Nonzero Photon Mass

作     者：WANGQing-Wu LǖXiao-Fu 

作者机构：DepartmentofPhysicsSichuanUniversityChengdu610064China DepartmentofPhysicsSichuanUniversityChengdu610064China／／CCAST（WorldLaboratory）P.O.Box8730Beijing100080China／／InstituteofTheoreticalPhysicsAcademiaSinicaP.O.Box2735Beijing100080China 

出 版 物：《Communications in Theoretical Physics》 (理论物理通讯（英文版）)

年 卷 期：2005年第43卷第4期

页      面：704-708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] 

基　　金：the Key Research Plan of Theoretical Physics and Cross Science 

主　　题：effective photon mass Fermi momentum beta-equilibrium 

摘      要：We investigate the neutron star magnetic field by the relative mean-field theory, where the photon effective mass depending on baryon density of charged particles is nonzero. This field is produced by star itself, which is the function of baryon density. The result fits the observations.