Stationary spherically symmetric one-kink model in Saez-Ballester theory of gravitation

In this paper we consider stationary Spherically symmetric kink space–time in the scalar–tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986 ) in the presence of perfect fluid distribution. It is shown that spherically symmetric kink space-time does not accommoda...

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Bibliographic Details
Published in:Astrophysics and space science 2015-03, Vol.356 (1), p.137-139
Main Authors: Kiran, M., Reddy, D. R. K., Rao, V. U. M., Bhaskara Rao, M. P. V. V.
Format: Article
Language:English
Subjects:
Analogue
Astrobiology
Astronomy
Astrophysics
Astrophysics and Astroparticles
Asymptotic properties
Computational fluid dynamics
Cosmology
Flats
Fluid flow
Fluids
Gravitation
Gravity
Observations and Techniques
Original Article
Physics
Physics and Astronomy
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Symmetry
Theory
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Summary:In this paper we consider stationary Spherically symmetric kink space–time in the scalar–tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986 ) in the presence of perfect fluid distribution. It is shown that spherically symmetric kink space-time does not accommodate perfect fluid distribution in this theory. Hence a vacuum model is obtained which is asymptotically flat. This model corresponds to a one kink metric in this theory. This can be considered as an analogue of usual spherically symmetric Schwarzschild case in this theory.
ISSN:0004-640X
1572-946X
DOI:10.1007/s10509-014-2186-2