Cylindrically Symmetric Cosmological Models in Bimetric Theory
P. K. Sahoo, G. Mohanty
Abstract
P. K. Sahoo, G. Mohanty
Abstract
Spherically symmetric Kantowski-Sachs space-time is studied in Rosen’s (1973) bimetric theory of gravitation, considering the source of gravitation as perfect fluid and scalar meson field. It is shown that a macro cosmological model – represented by perfect fluid distribution – does not exist, and only a vacuum model can be constructed, whereas in case of a micro cosmological model represented by a scalar meson field exists, and the model is obtained as in the case of Mohanty & Sahoo (2002).
OpenAlex reports 1 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Spherically symmetric Kantowski-Sachs space-time is studied in Rosen’s (1973) bimetric theory of gravitation, considering the source of gravitation as perfect fluid and scalar meson field. It is shown that a macro cosmological model – represented by perfect fluid distribution – does not exist, and only a vacuum model can be constructed, whereas in case of a micro cosmological model represented by a scalar meson field exists, and the model is obtained as in the case of Mohanty & Sahoo (2002).
Key concepts: Physics, Gravitation, Perfect fluid, Scalar (mathematics), Cosmological model, Scalar field, Theoretical physics, Field (mathematics)