Accelerating And Decelerating Hypersurface-Homogeneous Cosmological Models In Barberas Second Self-Creation Theory

α
Dr. S.D.Katore
Dr. S.D.Katore
σ
R. S. Rane
R. S. Rane
ρ
K. S. Wankhade
K. S. Wankhade
Ѡ
S. A. Bhaskar
S. A. Bhaskar
α Sant Gadge Baba Amravati University

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Accelerating And Decelerating Hypersurface-Homogeneous Cosmological Models In Barberas Second Self-Creation Theory

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Abstract

We study the hypersurface-homogeneous cosmological model in presence of perfect fluid within the framework of Barber’s [1982, GRG, 14, 117] second self-creation theory of gravitation. We have shown that the field equations are solvable for any arbitrary cosmic scale function and then obtained exact solutions for two values of a specific parameter. While doing so, we have used the general equation of state ρ m p where m ( 1 0 ≤ ≤ m ) is a constant. We also discussed the physical aspects of the models of the universe.

References

21 Cites in Article
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Funding

No external funding was declared for this work.

Conflict of Interest

The authors declare no conflict of interest.

Ethical Approval

No ethics committee approval was required for this article type.

Data Availability

Not applicable for this article.

How to Cite This Article

Dr. S.D.Katore. 2012. \u201cAccelerating And Decelerating Hypersurface-Homogeneous Cosmological Models In Barberas Second Self-Creation Theory\u201d. Global Journal of Science Frontier Research - F: Mathematics & Decision GJSFR-F Volume 12 (GJSFR Volume 12 Issue F3): .

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Issue Cover
GJSFR Volume 12 Issue F3
Pg. 41- 49
Journal Specifications

Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

Version of record

v1.2

Issue date

April 10, 2012

Language
en
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We study the hypersurface-homogeneous cosmological model in presence of perfect fluid within the framework of Barber’s [1982, GRG, 14, 117] second self-creation theory of gravitation. We have shown that the field equations are solvable for any arbitrary cosmic scale function and then obtained exact solutions for two values of a specific parameter. While doing so, we have used the general equation of state ρ m p where m ( 1 0 ≤ ≤ m ) is a constant. We also discussed the physical aspects of the models of the universe.

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Accelerating And Decelerating Hypersurface-Homogeneous Cosmological Models In Barberas Second Self-Creation Theory

Dr. S. D. Katore
Dr. S. D. Katore
R. S. Rane
R. S. Rane
K. S. Wankhade
K. S. Wankhade
S. A. Bhaskar
S. A. Bhaskar

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