We discuss a class of nonsingular spherically-symmetric cosmological models with radial heat flux and variable cosmological term Λ(t). Three different exact solutions of the Einstein’s field equations are obtained for both perfect fluid and fluid with bulk viscosity. It turns out that the cosmological term Λ(t) is a decreasing function of time, what is consistent with recent observations of type Ia supernovae. PACS numbers: 98.80.-k, 98.80.Es UDC 524.8
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A new class of cosmological models in f(R,T) modified theories of gravity proposed by Harko et al. (...
Bianchi type V perfect fluid cosmological models are investigated with cosmological term $\Lambda$ v...
Abstract—Exact solutions of Einstein’s field equations are obtained in a spatially homogeneous and a...
We present a class of nonsingular cosmological models with a variable cosmological term described by...
A plane-symmetric non-static cosmological model representing a bulk viscous fluid distribution has b...
A class of non-static inhomogeneous cosmological models are investigated with cosmological term Λ(t)...
Abstract—Exact solutions of Einstein’s field equations for a Bianchi type-I space-time filled with a...
WOS: A1994QB86900010We obtain some cosmological models that are exact solutions of Einstein field eq...
Abstract—Exact solutions of Einstein’s field equations are obtained in a spatially homogeneous and a...
In this note it is proposed a class of non-stationary de Sitter, rotating and non-rotating, solution...
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A new class of cosmological models in f(R,T) modified theories of gravity proposed by Harko et al. (...
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Abstract—Exact solutions of Einstein’s field equations are obtained in a spatially homogeneous and a...