Locally Rotationally Symmetric Bianchi Type-II Magnetized String Cosmological Model with Bulk Viscous Fluid in General Relativity

作     者：Atul Tyagi Keerti Sharma 

作者机构：Department of Mathematics and StatisticsUniversity College of ScienceMLS UniversityUdaipur 313001(Raj.)India Department of MathematicsMedi-caps Institute of Technology and ManagementIndore(MP)India 

出 版 物：《Chinese Physics Letters》 (中国物理快报（英文版）)

年 卷 期：2011年第28卷第8期

页      面：364-367页

核心收录：

学科分类：07[理学] 070401[理学-天体物理] 0805[工学-材料科学与工程（可授工学、理学学位）] 0704[理学-天文学] 

主　　题：Bianchi string Cosmo 

摘      要：The locally rotationally symmetric Bianchi type-II magnetized string cosmological model with bulk viscous fluid is *** magnetic field is due to an electric current produced along the x−*** the magnetic field is in the y–z plane and F23 is the only non−vanishing component of electromagnetic field tensor *** obtain the deterministic model in terms of cosmic time t,we have assumed the conditionξθ=const,whereξis the coefficient of bulk viscosity andθis the expansion in the model.