GRW-space-time and certain type of energy-momentum tensor

被引:3
|
作者
Baishya, Kanak Kanti [1 ]
机构
[1] Kurseong Coll, Dept Math, Dowhill Rd, Darjeeling 734203, W Bengal, India
关键词
Perfect fluid; (CS)(4)-space-time; Einstein's field equation; Energy-momentum tensor; Semisymmetric;
D O I
10.1016/j.geomphys.2020.103855
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
In [9] author proved that 4-dimensional Lorentzian concircular structure [in brief (CS)(4)] space-time coincides with generalized Robertson Walker [in brief GRW] spacetime. Consequently, to study perfect fluid (CS)(4)-spacetime obeying Einstein equation under various curvature restrictions on energy-momentum tensor like semi-symmetric, Ricci semi-symmetric etc. are equivalent to study that of perfect fluid GRW-spacetime obeying Einstein equation. The paper attempts to point out the curvature conditions for which the nature of the fluid in GRW-spacetime obeying Einstein equation is sometimes phantom barrier and some other time remains quintessence barrier (De and Ljubica, 2015). (C) 2020 Elsevier B.V. All rights reserved.
引用
收藏
页数:5
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