LRS Bianchi type-II dark energy model in a scalar-tensor theory of gravitation
DOI10.1007/s10509-011-0935-zzbMath1270.83011OpenAlexW2756788614MaRDI QIDQ422289
R. L. Naidu, D. R. K. Reddy, Bhavanari Satyanarayana
Publication date: 16 May 2012
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-011-0935-z
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
Related Items (8)
Cites Work
- Interacting holographic dark energy model in non-flat universe
- LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
- Bianchi type III models with anisotropic dark energy
- Exact spatially homogeneous cosmologies
- Quantum de Sitter cosmology and phantom matter
- Dark energy models with variable equation of state parameter
- Bianchi type III anisotropic dark energy models with constant deceleration parameter
- Dark energy and gravity
- Mach's Principle and a Relativistic Theory of Gravitation
- An alternative to quintessence
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