Natures of statefinder parameters and \(Om\) diagnostic for Cardassian universe in Hořava-Lifshitz gravity
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Publication:1936355
DOI10.1007/S10773-012-1254-ZzbMath1264.83048arXiv1108.1186OpenAlexW1993105915MaRDI QIDQ1936355
Ujjal Debnath, Piyali Bagchi Khatua
Publication date: 4 February 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1108.1186
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) Astrophysical cosmology (85A40)
Cites Work
- Statefinder parameter for varying \(G\) in three fluid system
- Variable \(G\) corrections to statefinder parameters of dark energy
- Statefinder diagnostic and stability of modified gravity consistent with holographic and agegraphic dark energy
- Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
- Perturbative instabilities in Hořava gravity
- Quintessence with O ( N ) symmetry
- 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
- Cosmological Imprint of an Energy Component with General Equation of State
- Cosmology on a brane in Minkowski bulk
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