Higher dimensional inhomogeneous cosmological models in Lyra geometry

Details Higher dimensional inhomogeneous cosmological models in Lyra geometry Higher dimensional inhomogeneous cosmological models in Lyra geometry

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.288..483r&link_type=abstract

Astrophysics and Space Science, v. 288, Issue 4, p. 483-491 (2003).

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

We have presented in homogeneous cosmological models within the framework of Lyra geometry. We have considered an inhomogeneous spherically symmetric higher dimensional model in presence of a mass less scalar field whose potential has a flat part. The scalar field is considered to be inhomogeneous. Also an inhomogeneous cosmological model is derived in a Kaluza-Klein type of space time. The matter field is taken as an inhomogeneous distribution of fluid. It is observed that there is no singularity at finite past in our model and the desirable feature of dimensional reduction is also possible for the extra space.

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