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New special homogeneous Bianchi type I Massive string cosmological models with anisotropic dark energy

Abstract

A special law of variation for Hubble’s parameter is presented in a spatially homogeneous Bianchi type-I massive string cosmological models with space-time that yields a constant value of deceleration parameter. Using the law of variation for Hubble’s parameter, exact solutions of Einstein’s field equations are obtained for Bianchi-I space-time filled with perfect fluid in two different cases where the universe exhibits power-law and exponential expansion. It is found that the solutions are consistent with the recent observations of type Ia supernovae. A detailed study of physical and kinematical properties of the models is carried out.

Cosmology and Gravitation TheoriesGeophysics and Gravity MeasurementsBlack Holes and Theoretical PhysicsPhysicsDeceleration parameterDark energyHubble's lawMathematical physicsString (physics)Cosmological constantType (biology)Metric expansion of spacePower law
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New special homogeneous Bianchi type I Massive string cosmological models with anisotropic dark energy · Scinovex