An exact Chameleon cosmological model unifying phantom inflation with late-time acceleration
From MaRDI portal
Publication:641712
DOI10.1007/s10773-011-0718-xzbMath1229.83086OpenAlexW2020381953MaRDI QIDQ641712
Publication date: 25 October 2011
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-011-0718-x
Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) General geometric structures on manifolds (almost complex, almost product structures, etc.) (53C15) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (2)
Cosmic acceleration and ekpyrotic bounce with Chameleon field ⋮ Reconstruction of cosmic history from a simple parametrization of H
Cites Work
- Unnamed Item
- Phantom appearance of non-phantom matter
- de Sitter brane universe induced by phantom and quantum effects
- Effective equation of state and energy conditions in phantom/tachyon inflationary cosmology perturbed by quantum effects
- Quantum de Sitter cosmology and phantom matter
- Cosmological constant -- the weight of the vacuum
- Statefinder parameters for interacting dark energy
- Exorcising \(w < -1\)
- Unifying phantom inflation with late-time acceleration: scalar phantom-non-phantom transition model and generalized holographic dark energy
- Acceleration of the universe with a simple trigonometric potential
- A quintessence scalar field in Brans-Dicke theory
- The cosmological constant and dark energy
- Exact scalar field cosmologies
- PHANTOM UNIVERSE FROM CPT SYMMETRIC QFT
- COSMOLOGY IN SCALAR–TENSOR THEORY AND ASYMPTOTICALLY de SITTER UNIVERSE
- COSMIC DYNAMICS IN CHAMELEON COSMOLOGY
- SO (1, 1) dark energy model and the universe transition
- Dark energy cosmology with generalized linear equation of state
- Consistent modified gravity: dark energy, acceleration and the absence of cosmic doomsday
- LATE-TIME PHANTOM UNIVERSE IN SO(1, 1) DARK ENERGY MODEL WITH EXPONENTIAL POTENTIAL
- QUINTOM COSMOLOGY WITH GENERAL POTENTIALS
- 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
- The cosmological constant problem
- SELF INTERACTING BRANS–DICKE COSMOLOGY AND QUINTESSENCE
This page was built for publication: An exact Chameleon cosmological model unifying phantom inflation with late-time acceleration
