Coincidence Problem in Gravity Models
arXiv:1012.0405 · doi:10.1103/PhysRevD.82.124041
Abstract
The gravity models formulated in Einstein conformal frame are equivalent to Einstein gravity together with a minimally coupled scalar field. The scalar field couples with the matter sector and the coupling term is given by the conformal factor. We use this interacting model to derive a necessary condition for alleviating the coincidence problem.
10 pages, 2 figures. To appear in Physical Review D
References in corpus (39)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- The Cosmological Constant and Dark Energy
- Cosmological Constant - the Weight of the Vacuum
- Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
- The Case for a Positive Cosmological Lambda-term
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- The Cosmological Constant
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Modified gravity with negative and positive powers of the curvature: unification of the inflation and of the cosmic acceleration
- Coupled Quintessence
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Disappearing cosmological constant in f(R) gravity
- Late-time cosmology in (phantom) scalar-tensor theory: dark energy and the cosmic speed-up
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Can modified gravity explain accelerated cosmic expansion?
- Cosmological viability of f(R)-gravity as an ideal fluid and its compatibility with a matter dominated phase
- Conditions for the cosmological viability of f(R) dark energy models
- Interacting Quintessence
- The Cosmology of Generalized Modified Gravity Models
- Curvature quintessence matched with observational data
- On Physical Equivalence between Nonlinear Gravity Theories
- Extended Gravity Theories and the Einstein-Hilbert Action
- Dynamics of dark energy with a coupling to dark matter
- Solar system and equivalence principle constraints on f(R) gravity by chameleon approach
- Matter instability in modified gravity
- Accelerated Cosmological Models in Ricci squared Gravity
- Reconstruction of the deceleration parameter and the equation of state of dark energy
- Scaling Cosmology
- The Force of Gravity from a Lagrangian containing Inverse Powers of the Ricci Scalar
- Stationary dark energy with a baryon-dominated era: solving the coincidence problem with a linear coupling
- Interacting models may be key to solve the cosmic coincidence problem
- Cosmological Evolution in 1/R-Gravity Theory
- Observational constraints on the acceleration of the Universe
- K-Chameleon and the Coincidence Problem
- Phantom boundary crossing and anomalous growth index of fluctuations in viable f(R) models of cosmic acceleration
- Quintessence in brane cosmology
- Coincidence Problem in an Oscillating Universe
- Solar System Constraints on a Cosmologically Viable Theory
- Gravitational Coupling and Dynamical Reduction of The Cosmological Constant
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- Power-law entropy corrected new holographic scalar field models of dark energy with modified IR-cutoff
- 5D Elko spinor field non-minimally coupled to nonmetricity in gravity
- Towards a possible solution for the coincidence problem: f(G) gravity as background
- Coincidence Problem in f(T) Gravity Models
- The coincidence problem in gravity models
- Attractor Solutions in Interacting Dark Energy Models
- Cosmic Evolution in a Modified Brans-Dicke Theory
- Gravitational Coupling and the Cosmological Constant
- Ricci-Cubic Holographic Dark Energy: Confronting Observations, Stability and the Cosmic Coincidence Problem
- Coincidence Problem and Holographic Gravity in Spatially flat and Curved Universes
- The Coincidence Problem in Holographic f(R) Gravity
- Production of Primordial Gravitational Waves in Teleparallel Gravity
- Holographic dark energy models with Interactions and entropy corrections for different cutoffs in the Brans-Dicke cosmology