Spherically symmetric anisotropic and inhomogeneous cosmological models |
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Authors: | J Krishna Rao |
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Institution: | (1) Department of Mathematics, Bhavnagar University, 364002 Bhavnagar, India |
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Abstract: | Spherically symmetric cosmological models filled with dust (pressure-free fluid) content are analyzed. It has been pointed
out that these models are anisotropic (of non-vanishing shear) and inhomogeneous (∂p/ρr ≠ 0), the characteristics related
directly to the presence of the free gravitational field. It is demonstrated that when the free gravitational field vanishes
these models degenerate to the corresponding Friedmann-Robertson-Walker (FRW) models. It is further shown that the energy
density of the free gravitational field can be introduced into observational cosmology as a new parameter since it enters
into the expansion and deceleration equations, as well as conservation law for total energy, implying that the present Hubble
velocity can be reached in a shorter time from the big bang. Finally, the effect of shear on the redshift is also discussed.
This paper is dedicated to my teacher Professor V V Narlikar on the occasion of his 81st birthday. |
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Keywords: | Cosmology gravitational radiation energy density of the free gravitational field |
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