AN LRS BIANCHI TYPE-I COSMOLOGICAL MODEL WITH TIME-DEPENDENT Λ TERM
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Publication:5297848
DOI10.1142/S0218271807009863zbMath1119.83028OpenAlexW1967940706MaRDI QIDQ5297848
Rishi Kumar Tiwari, Jagdish Singh
Publication date: 13 July 2007
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0218271807009863
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)
Related Items (6)
Bianchi V cosmology with a specific Hubble parameter ⋮ Higher dimensional cosmological models with bulk viscous fluid ⋮ Bianchi type V viscous fluid cosmological models with varying cosmological term ⋮ Bianchi type V cosmological models with varying cosmological term ⋮ Bulk viscosity and decaying vacuum density in Friedmann universe ⋮ Viscous Bianchi type I universe with stiff matter and decaying vacuum energy density
Cites Work
- Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
- Cosmological models with variable G and \(\Lambda\)
- Cosmological models with variable gravitational and cosmological ``constants
- Anisotropic viscous cosmology with variable \(G\) and \(\Lambda\)
- Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant
- A model to explain varying \(\Lambda\), \(G\) and \(\sigma^{2}\) simultaneously
- Friedmann cosmology with decaying vacuum density
- A study of angular size-redshift relation for models in which Λ decays as the energy density
- Consequences on variable Λ-models from distant type Ia supernovae and compact radio sources
- BULK VISCOUS ANISOTROPIC COSMOLOGICAL MODELS WITH VARIABLE G AND Λ
- ON THE COSMOLOGICAL CONSTANT AND THE COSMIC COINCIDENCE PROBLEM
- Cosmic acceleration with a positive cosmological constant
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- The cosmological constant problem
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