Plane Symmetric Cosmological Model with Quark and Strange Quark Matter in f(R,T) Theory of Gravity
arXiv:1702.02349 · doi:10.1007/s12036-016-9420-y
Abstract
We studied plane symmetric cosmological model in the presence of quark and strange quark matter with the help of f(R,T) theory. To decipher solutions of Plane symmetric space-time, we used power law relation between scale factor and deceleration parameter. We considered the special law of variation of Hubble's parameter proposed by Berman (Nuovo Cimento B 74, 182, 1983) which yields constant deceleration parameter. We also discussed the physical behavior of the solutions by using some physical parameters.
arXiv commentAccepted for publication in Journal of Astrophysics and Astronomy, August 2016
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- Stability, dark energy parameterization and swampland aspect of Bianchi Type- cosmological models with f(R, T)-gravity
- Anti-Correlated lags in a Neutron star Z source GX 5-1: AstroSat's View
- Static plane symmetric solutions in gravity