FRW Viscous Fluid cosmological Model in f(R,T) Gravity

1
D.R.K.Reddy
D.R.K.Reddy
2
Dr. R.L.Naidu
Dr. R.L.Naidu
3
K.Dasu Naidu
K.Dasu Naidu
4
T.Ramprasad
T.Ramprasad
1 MVGR College of Engineering, Vizianagaram A.P, India

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Friedmann-Robertson-Walker (FRW) space time is considered in f(R,T) gravity proposed by Harko et al. (Phys.Rev.D 84, 024020, 2011) when the source for energy momentum tensor is a bulk viscous fluid. A barotropic equation of state for the pressure and energy density is assumed to get a determinate solution of the field equations. Also the bulk viscous pressure is assumed to be proportional to energy density. A physical discussion of the model is also presented.

39 Cites in Articles

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Funding

No external funding was declared for this work.

Conflict of Interest

The authors declare no conflict of interest.

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No ethics committee approval was required for this article type.

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Not applicable for this article.

D.R.K.Reddy. 2013. \u201cFRW Viscous Fluid cosmological Model in f(R,T) Gravity\u201d. Global Journal of Science Frontier Research - A: Physics & Space Science GJSFR-A Volume 13 (GJSFR Volume 13 Issue A3): .

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GJSFR Volume 13 Issue A3
Pg. 55- 57
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Crossref Journal DOI 10.17406/GJSFR

Print ISSN 0975-5896

e-ISSN 2249-4626

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April 22, 2013

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English

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Friedmann-Robertson-Walker (FRW) space time is considered in f(R,T) gravity proposed by Harko et al. (Phys.Rev.D 84, 024020, 2011) when the source for energy momentum tensor is a bulk viscous fluid. A barotropic equation of state for the pressure and energy density is assumed to get a determinate solution of the field equations. Also the bulk viscous pressure is assumed to be proportional to energy density. A physical discussion of the model is also presented.

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FRW Viscous Fluid cosmological Model in f(R,T) Gravity

Dr. R.L.Naidu
Dr. R.L.Naidu
K.Dasu Naidu
K.Dasu Naidu
T.Ramprasad
T.Ramprasad

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