Bianchi type-II dark energy model in \(f(R,T)\) gravity
DOI10.1007/s10773-013-1939-yzbMath1300.83059OpenAlexW2013301359MaRDI QIDQ461883
J. Herrera, D. Rodríguez-Gómez
Publication date: 15 October 2014
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-013-1939-y
Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (15)
Cites Work
- Dark energy model in anisotropic Bianchi type-III space-time with variable eos parameter
- Some Bianchi type cosmological models in \(f(R)\) gravity
- LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
- Bianchi type III models with anisotropic dark energy
- Dark energy models with variable equation of state parameter
- Bianchi type III anisotropic dark energy models with constant deceleration parameter
- The cosmological constant and dark energy
- RECONSTRUCTING f(R, T) GRAVITY FROM HOLOGRAPHIC DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
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