How a projectively flat geometry regulates F(R)-gravity theory?
In the present paper we examine a projectively flat spacetime solution of F(R)-gravity theory. It is seen that once we deploy projective flatness in the geometry of the spacetime, the matter field has constant energy density and isotropic pressure. We then make the condition weaker and discuss the e...
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my.um.eprints.262662022-02-22T04:48:17Z http://eprints.um.edu.my/26266/ How a projectively flat geometry regulates F(R)-gravity theory? Loo, Tee-How De, Avik Mandal, Sanjay Sahoo, P K QC Physics In the present paper we examine a projectively flat spacetime solution of F(R)-gravity theory. It is seen that once we deploy projective flatness in the geometry of the spacetime, the matter field has constant energy density and isotropic pressure. We then make the condition weaker and discuss the effects of projectively harmonic spacetime geometry in F(R)-gravity theory and show that the spacetime in this case reduces to a generalised Robertson-Walker spacetime with a shear, vorticity, acceleration free perfect fluid with a specific form of expansion scalar presented in terms of the scale factor. Role of conharmonic curvature tensor in the spacetime geometry is also briefly discussed. Some analysis of the obtained results are conducted in terms of couple of F(R)-gravity models. 2021-12 Article PeerReviewed Loo, Tee-How and De, Avik and Mandal, Sanjay and Sahoo, P K (2021) How a projectively flat geometry regulates F(R)-gravity theory? Physica Scripta, 96 (12). p. 125034. ISSN 0031-8949, DOI https://doi.org/10.1088/1402-4896/ac3a51 <https://doi.org/10.1088/1402-4896/ac3a51>. https://doi.org/10.1088/1402-4896/ac3a51 doi:10.1088/1402-4896/ac3a51 |
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QC Physics Loo, Tee-How De, Avik Mandal, Sanjay Sahoo, P K How a projectively flat geometry regulates F(R)-gravity theory? |
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In the present paper we examine a projectively flat spacetime solution of F(R)-gravity theory. It is seen that once we deploy projective flatness in the geometry of the spacetime, the matter field has constant energy density and isotropic pressure. We then make the condition weaker and discuss the effects of projectively harmonic spacetime geometry in F(R)-gravity theory and show that the spacetime in this case reduces to a generalised Robertson-Walker spacetime with a shear, vorticity, acceleration free perfect fluid with a specific form of expansion scalar presented in terms of the scale factor. Role of conharmonic curvature tensor in the spacetime geometry is also briefly discussed. Some analysis of the obtained results are conducted in terms of couple of F(R)-gravity models. |
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Article |
author |
Loo, Tee-How De, Avik Mandal, Sanjay Sahoo, P K |
author_facet |
Loo, Tee-How De, Avik Mandal, Sanjay Sahoo, P K |
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Loo, Tee-How |
title |
How a projectively flat geometry regulates F(R)-gravity theory? |
title_short |
How a projectively flat geometry regulates F(R)-gravity theory? |
title_full |
How a projectively flat geometry regulates F(R)-gravity theory? |
title_fullStr |
How a projectively flat geometry regulates F(R)-gravity theory? |
title_full_unstemmed |
How a projectively flat geometry regulates F(R)-gravity theory? |
title_sort |
how a projectively flat geometry regulates f(r)-gravity theory? |
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2021 |
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http://eprints.um.edu.my/26266/ https://doi.org/10.1088/1402-4896/ac3a51 |
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