Axially Symmetric Bulk Viscous String Cosmological Models in GR and Brans-Dicke Theory of Gravitation | Zendy

V. U. M. Rao | Zendy; D. Neelima | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

Axially Symmetric Bulk Viscous String Cosmological Models in GR and Brans-Dicke Theory of Gravitation

Author(s) -

V. U. M. Rao,

D. Neelima

Publication year - 2013

Publication title -

isrn astronomy and astrophysics

Language(s) - English

Resource type - Journals

eISSN - 2090-4746

pISSN - 2090-4738

DOI - 10.1155/2013/543483

Subject(s) - axial symmetry , physics , general relativity , string (physics) , gravitation , brans–dicke theory , classical mechanics , scalar field , volume viscosity , mathematical physics , universe , anisotropy , cosmological model , theoretical physics , string theory , cosmology , viscosity , quantum mechanics

Axially symmetric string cosmological models with bulk viscosity in Brans-Dicke (1961) and general relativity (GR) have been studied. The field equations have been solved by using the anisotropy feature of the universe in the axially symmetric space-time. Some important features of the models, thus obtained, have been discussed. We noticed that the presence of scalar field does not affect the geometry of the space-time but changes the matter distribution, and as a special case, it is always possible to obtain axially symmetric string cosmological model with bulk viscosity in general relativity.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research