Dynamics of an Anisotropic Universe in f(R,T) Theory
Dynamics of an anisotropic universe is studied in f(R,T) gravity using a rescaled functional f(R,T), where R is the Ricci Scalar and T is the trace of energy-momentum tensor. Three models have been constructed assuming a power law expansion of the universe. Physical features of the models are discus...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Hindawi Limited
2016-01-01
|
| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2016/8543560 |
| id |
doaj-9044ca96639441f988bdba3620ae30c5 |
|---|---|
| record_format |
Article |
| spelling |
doaj-9044ca96639441f988bdba3620ae30c52020-11-24T23:02:46ZengHindawi LimitedAdvances in High Energy Physics1687-73571687-73652016-01-01201610.1155/2016/85435608543560Dynamics of an Anisotropic Universe in f(R,T) TheoryB. Mishra0Sankarsan Tarai1S. K. Tripathy2Department of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, IndiaDepartment of Mathematics, Birla Institute of Technology and Science-Pilani, Hyderabad Campus, Hyderabad 500078, IndiaDepartment of Physics, Indira Gandhi Institute of Technology, Sarang, Dhenkanal, Odisha 759146, IndiaDynamics of an anisotropic universe is studied in f(R,T) gravity using a rescaled functional f(R,T), where R is the Ricci Scalar and T is the trace of energy-momentum tensor. Three models have been constructed assuming a power law expansion of the universe. Physical features of the models are discussed. The model parameters are constrained from a dimensional analysis. It is found from the work that the anisotropic Bianchi type VIh (BVIh) model in the modified gravity generally favours a quintessence phase when the parameter h is either -1 or 0. We may not get viable models in conformity with the present day observation for h=1.http://dx.doi.org/10.1155/2016/8543560 |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
B. Mishra Sankarsan Tarai S. K. Tripathy |
| spellingShingle |
B. Mishra Sankarsan Tarai S. K. Tripathy Dynamics of an Anisotropic Universe in f(R,T) Theory Advances in High Energy Physics |
| author_facet |
B. Mishra Sankarsan Tarai S. K. Tripathy |
| author_sort |
B. Mishra |
| title |
Dynamics of an Anisotropic Universe in f(R,T) Theory |
| title_short |
Dynamics of an Anisotropic Universe in f(R,T) Theory |
| title_full |
Dynamics of an Anisotropic Universe in f(R,T) Theory |
| title_fullStr |
Dynamics of an Anisotropic Universe in f(R,T) Theory |
| title_full_unstemmed |
Dynamics of an Anisotropic Universe in f(R,T) Theory |
| title_sort |
dynamics of an anisotropic universe in f(r,t) theory |
| publisher |
Hindawi Limited |
| series |
Advances in High Energy Physics |
| issn |
1687-7357 1687-7365 |
| publishDate |
2016-01-01 |
| description |
Dynamics of an anisotropic universe is studied in f(R,T) gravity using a rescaled functional f(R,T), where R is the Ricci Scalar and T is the trace of energy-momentum tensor. Three models have been constructed assuming a power law expansion of the universe. Physical features of the models are discussed. The model parameters are constrained from a dimensional analysis. It is found from the work that the anisotropic Bianchi type VIh (BVIh) model in the modified gravity generally favours a quintessence phase when the parameter h is either -1 or 0. We may not get viable models in conformity with the present day observation for h=1. |
| url |
http://dx.doi.org/10.1155/2016/8543560 |
| work_keys_str_mv |
AT bmishra dynamicsofananisotropicuniverseinfrttheory AT sankarsantarai dynamicsofananisotropicuniverseinfrttheory AT sktripathy dynamicsofananisotropicuniverseinfrttheory |
| _version_ |
1725635299101376512 |