ACCELERATING DARK ENERGY MODELS IN BIANCHI TYPE-V SPACETIME
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Publication:2861199
DOI10.1142/S0217732311036620zbMath1274.83171arXiv1110.1019OpenAlexW3104012309MaRDI QIDQ2861199
Hassan Amirhashchi, Anirudh Pradhan
Publication date: 12 November 2013
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1110.1019
Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)
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Cites Work
- Dark energy model in anisotropic Bianchi type-III space-time with variable eos parameter
- LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
- Bianchi type III models with anisotropic dark energy
- Cosmological constant -- the weight of the vacuum
- Cosmography: Cosmology without the Einstein equations
- SOME BIANCHI TYPE-V MODELS OF ACCELERATING UNIVERSE WITH DARK ENERGY
- DYNAMICS OF DARK ENERGY
- Jerk, snap and the cosmological equation of state
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
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