Axially symmetric cosmological models in a scalar tensor theory based on Lyra manifold

Details Axially symmetric cosmological models in a scalar tensor theory based on Lyra manifold Axially symmetric cosmological models in a scalar tensor theory based on Lyra manifold

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ap%26ss.319..161r&link_type=abstract

Astrophysics and Space Science, Volume 319, Issue 2-4, pp. 161-167

Astronomy and Astrophysics

Astrophysics

2

Axially Symmetric, Lyra Manifold, String Source, Perfect Fluid, Dust Distribution, Thick Domain Walls

Scientific paper

Axially symmetric cosmological models are obtained in a scalar tensor
theory proposed by Sen (Z. Phys. 149:311, 1957) based on Lyra manifold
with time dependent β in the presence of string source, perfect
fluid distribution, dust distribution and thick domain walls. Some
physical and geometrical properties of these models are discussed.

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