In this situation as well validity of the above expression for all null vectors [l.sub.a], along with two times contracted Bianchi identity and covariant conservation of matter
energy momentum tensor, amounts to furnishing the ten components of Einstein's equations.
The known exact solutions may be classified into (at least) four classes [2], namely, the algebraic classification of conformal curvature, physical characterization of the
energy momentum tensor, existence, and structure of preferred vector fields and group of motions.
The
energy momentum tensor of the electromagnetic field [T.sup.[mu]v] not generally symmetric.
for all vector fields X, Y where S is the Ricci tensor of the type (0, 2), r is the scalar curvature, k is the gravitational constant and T is the
energy momentum tensor of type (0, 2).
So, for example, if one begins with a vacuum seed solution, then it is known that the Einstein tensor is zero and so only the conformal part must now be considered in conjunction with a perfect fluid
energy momentum tensor. Such solutions are referred to as conformally Ricci-flat spacetimes.
In the general theory of relativity,
energy momentum tensor plays an important role and the condition on
energy momentum tensor for a perfect fluid space time changes the nature of space time (5).
here [T.sub.ij] being the ordinary
energy momentum tensor associated to isotropic matter and radiation.
the new improved
energy momentum tensor is defined as
where k is the Einstein's gravitational constant, T is the
energy momentum tensor of type (0,2) given by
Although there are physical arguments for equating the Einstein tensor to the
energy momentum tensor ([G.sub.[micro]v] = K[T.sub.[micro]v]), and thus into analogues for Newton's Law of Gravity, we note simply in this paper that Eq.
One way is to modify the dynamical field equations by taking negative pressure in the form of
energy momentum tensor [T.sub.[mu][nu]].
Therefore, the nonzero components of the
energy momentum tensor from (11) using (13) are