The reviewed record of science sign in
Pith

arxiv: 1603.05043 · v2 · pith:IM3XXAUZ · submitted 2016-03-16 · math.GM

On a Kaehlerian space-time manifold

Reviewed by Pith T0 review T1 audit T2 compute T3 formal T4 kernel pith:IM3XXAUZrecord.jsonopen to challenge →

classification math.GM
keywords manifoldspace-timekaehlerfluidperfectsymmetricweaklyalpha
0
0 comments X
read the original abstract

In this paper, the theory of space-time in 4-dimensional Kaehler manifold has been studied. We have discussed the Einstein equation with cosmological constant in perfect fluid Kaehler space-time manifold and proved that the isotropic pressure, energy density and the energy momentum tensor vanish and such a space-time manifold is an Einstein manifold. We have shown also that a conformally flat perfect fluid Kaehler space-time manifold is infinitesimally spatially isotropic relative to the velocity vector field. In last two sections, we have studied weakly symmetric and weakly Ricci symmetric perfect fluid Kaehler space-time manifolds and it has been shown, either the manifold is of zero scalar curvature or the associated vector fields rho and alpha are related by g(rho,alpha) = 4. At last, we have proved that the weakly Ricci symmetric perfect fluid Kaehler space-time manifold of non-zero scalar curvature does not exist.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.