-type and -type four dimensional plane wave solutions of Einstein's

Page 1

Research Inventy: International Journal Of Engineering And Science Vol.5, Issue 2 (February 2015), PP 30-38 Issn (e): 2278-4721, Issn (p):2319-6483, www.researchinventy.com [

1 2

( y  z )  t ] -type

and

[t 2 ( y  z )] -type

four dimensional plane wave

solutions of Einstein’s field equations in general relativity B. G. Ambatkar , J K Jumale* Head Department of mathematics, R.S. Bidkar Arts, Comm. and Science College, Hinganghat, * R.S. Bidkar Arts, Comm. and Science College, Hinganghat, Distt. Wardha*, jyotsnajumale21@gmail.com

ABSTRACT: In the present paper, we have studied [

1 2

( y  z )  t ] - type and [t 2 ( y  z )] -type plane

wave solutions of Einstein’s field equations in general theory of relativity in the case where the zero mass scalar field coupled with gravitational field and zero mass scalar field coupled with gravitational & electromagnetic field and established the existence of these two types of plane wave solutions in V 4 . Furthermore we have considered the case of massive scalar field and shown that the non-existence of these two types of plane wave solutions in GR theory. Keywords : Einstein’s field equations in general relativity in case where the zero mass scalar field coupled with gravitational field and zero mass scalar field coupled with gravitational & electromagnetic field, four dimensional space-time, etc.

I. INTRODUCTION

H.Takeno (1961) has obtained the non-flat plane wave solutions g ij of the field equations Rij  0 and established the existence of ( z  t ) -type and (t z ) -type plane waves in purely gravitational case in fourdimensional empty region of space-time. On the lines of Takeno (1961), Kadhao and Thengane (2002) have also obtained the plane wave solutions g ij of the field equations Rij  0 in purely gravitational case by reformulating Takeno's (1961) definition of plane wave as follows: Definition A plane wave g ij is a non-flat solution of field equations

Rij  0 ,

[i, j  1,2,3,4,5]

(1.1)

in an empty region of space-time such that

g ij  g ij (Z ) ,

Z  Z (xi ) ,

where x  u, x, y, z , t i

(1.2)

in some suitable co-ordinate system such that

Z ,i 

g ij Z ,i Z , j  0, Z  Z ( y, z, t ),

Z

x i

Z , 2  0,

,

(1.3)

Z ,4  0 .

Z , 3  0,

(1.4) In this

definition, the signature convention adopted is

g rr  0, r  1,2,3

g rr g sr

g rs  0, g ss

g11

g12

g13

g 21

g 22

g 31

g 32

g 23 <0, g 33

g 44  0

[not summed for r,s =1,2,3] and accordingly g  det( g ij )  0

30

(1.5)

(1.6)


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