FRW-cosmological model for conharmonically flat space time
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Publication:1945400
DOI10.1007/s10773-012-1364-7zbMath1263.83047OpenAlexW1972058664MaRDI QIDQ1945400
Rajesh Kumar, Sudhir Kumar Srivastava
Publication date: 8 April 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-012-1364-7
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
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Cites Work
- Concircular curvature tensor and fluid spacetimes
- A critical density cosmological model with varying gravitational and cosmological ``constants
- Generalized Maxwell equations and quantum mechanics. I: Dirac equation for the free electron
- Solutions to the field equations and the deceleration parameter
- Early universe with variable gravitational and cosmological constants
- A study of angular size-redshift relation for models in which Λ decays as the energy density
- BULK VISCOUS SOLUTIONS TO THE FIELD EQUATIONS AND THE DECELERATION PARAMETER-REVISITED
- BULK VISCOUS ANISOTROPIC COSMOLOGICAL MODELS WITH VARIABLE G AND Λ
- Cosmological vacuum decay, irreversible thermodynamics and event horizons
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