BOUNCING UNIVERSE WITH THE NON-MINIMALLY COUPLED SCALAR FIELD AND ITS RECONSTRUCTION
From MaRDI portal
Publication:3647706
DOI10.1142/S0217732309030783zbMath1175.83096arXiv0904.0110MaRDI QIDQ3647706
No author found.
Publication date: 23 November 2009
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0904.0110
Related Items (max. 100)
Thermodynamics of the viscous f(T,B) gravity in the new agegraphic dark energy model ⋮ Stability analysis in modified non-local gravity ⋮ Cosmic dynamics in \(F(R,\varphi)\) gravity ⋮ BOUNCING UNIVERSE AND PHANTOM CROSSING IN MODIFIED GRAVITY AND ITS RECONSTRUCTION ⋮ Bouncing universe with the modified gravity coupled to the Weyl tensor ⋮ Bouncing theory in the modified Weyl gravity and its stability conditions
Cites Work
- The phantom divide in string gas cosmology
- The gravitating perfect fluid-scalar field equations: quintessence and tachyonic matter
- Nonlinear dynamics equation in \(p\)-adic string theory
- Rolling tachyon in NS string field theory
- Numerical study of nonlinear equations with an infinite number of derivatives
- Cosmological Inflation and Large-Scale Structure
- Cosmology as geodesic motion
- 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
- Inflationary universe: A possible solution to the horizon and flatness problems
- Cosmological Imprint of an Energy Component with General Equation of State
- Tachyon condensation in superstring field theory.
This page was built for publication: BOUNCING UNIVERSE WITH THE NON-MINIMALLY COUPLED SCALAR FIELD AND ITS RECONSTRUCTION