Axially symmetric non-static domain walls in scalar-tensor theories of gravitation

Details Axially symmetric non-static domain walls in scalar-tensor theories of gravitation Axially symmetric non-static domain walls in scalar-tensor theories of gravitation

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.312..165a&link_type=abstract

Astrophysics and Space Science, Volume 312, Issue 3-4, pp. 165-169

Astronomy and Astrophysics

Astrophysics

8

Scientific paper

An axially symmetric non-static space-time is considered in the presence of thick domain walls in the scalar-tensor theories formulated by Brans and Dicke (Phys. Rev. 124:925, 1961) and Saez and Ballester (Phys. Lett. A 113:467, 1985). Exact cosmological models, in both the theories, are presented with the help of special law of variation proposed by Berman (Nuovo Cim. B 74:182, 1983), for Hubble’s parameter. Some physical and kinematical properties of the models are discussed.

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