LRS Bianchi type-II dark energy model in a scalar-tensor theory of gravitation

Details LRS Bianchi type-II dark energy model in a scalar-tensor theory of gravitation LRS Bianchi type-II dark energy model in a scalar-tensor theory of gravitation

Apr 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ap%26ss.338..333n&link_type=abstract

Astrophysics and Space Science, Volume 338, Issue 2, pp.333-336

Astronomy and Astrophysics

Astrophysics

2

Scalar-Tensor Theory, Lrs Bianchi Type-Ii Universe, Dark Energy, Variable Eos Parameter

Scientific paper

A locally rotationally symmetric Bianchi type-II (LRS B-II) space-time with variable equation of state (EoS) parameter and constant deceleration parameter have been investigated in the scalar-tensor theory proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986). The scalar-tensor field equations have been solved by applying variation law for generalized Hubble's parameter given by Bermann (Nuovo Cimento 74:182, 1983). The physical and kinematical properties of the model are also discussed.

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