A PLANE-SYMMETRICAL INHOMOGENEOUS COSMOLOGICAL MODEL OF PERFECT FLUID DISTRIBUTION WITH ELECTROMAGNETIC-FIELD

被引：19
|
作者：
BALI, R
TYAGI, A
机构：
[1] Department of Mathematics, University of Rajasthan, Jaipur
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1990年 / 173卷 / 02期
关键词：
D O I：
10.1007/BF00643932
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field, is obtained. F12 is the non-vanishing component of the electromagnetic field tensor. To get a determinate solution, we assume the free gravitational field is Petrov type-II non-degenerate. In general, the model represents an expanding, shearing, non-rotating universe in which the flow vector is geodetic. The behaviour of the electromagnetic field tensor together with some geometrical and physical aspect of the model are also discussed. © 1990 Kluwer Academic Publishers.
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页码：233 / 240
页数：8
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