Vacuum Solution of a Linear Red-Shift Based Correction in Gravity
arXiv:1104.5108 · doi:10.1007/s10714-011-1304-5
Abstract
In this paper we have considered a red-shift based linear correction in derivative of action in the context of vacuum gravity. Here we have found out that the linear correction may describe the late time acceleration which is appeared by SNeIa with no need of dark energy. Also we have calculated the asymptotic action for the desired correction. The value of all solutions may reduce to de' Sitter universe in the absence of correction term.
Revised version, 18 pages, 7 figures
References in corpus (62)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- f(R) Theories Of Gravity
- 4D Gravity on a Brane in 5D Minkowski Space
- 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
- An alternative to quintessence
- 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
- Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
- A Dynamical Solution to the Problem of a Small Cosmological Constant and Late-time Cosmic Acceleration
- Dark Energy and the Accelerating Universe
- k-Inflation
- Essentials of k-essence
- Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
- Chameleon Cosmology
- Kinetically Driven Quintessence
- Curvature Quintessence
- Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
- Disappearing cosmological constant in f(R) gravity
- Perturbations in k-inflation
- Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
- Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- Extended Theories of Gravity and their Cosmological and Astrophysical Applications
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- 1/R gravity and Scalar-Tensor Gravity
- Unifying inflation with LambdaCDM epoch in modified f(R) gravity consistent with Solar System tests
- Purely kinetic k-essence as unified dark matter
- Curvature quintessence matched with observational data
- Do consistent models mimic General Relativity plus ?
- Reconciling dark energy models with f(R) theories
- Can the Chaplygin gas be a plausible model for dark energy?
- Cross-correlation Tomography: Measuring Dark Energy Evolution with Weak Lensing
- Observational signatures of f(R) dark energy models that satisfy cosmological and local gravity constraints
- Where new gravitational physics comes from: M-theory?
- Modified gravity and its reconstruction from the universe expansion history
- Extended tachyon field, Chaplygin gas and solvable k-essence cosmologies
- Probing Newton's Constant on Vast Scales: DGP Gravity, Cosmic Acceleration and Large Scale Structure
- Cosmological dynamics of R^n gravity
- Tracking K-essence
- Cosmological consequences of a Chaplygin gas dark energy
- Accelerated Cosmological Models in Ricci squared Gravity
- Non-singular exponential gravity: a simple theory for early- and late-time accelerated expansion
- Are Chaplygin gases serious contenders to the dark energy throne?
- Differentiating between Modified Gravity and Dark Energy
- The Power of Brane-Induced Gravity
- Newton law corrections and instabilities in gravity with the effective cosmological constant epoch
- Power-law expansion in k-essence cosmology
- Generalizing the generalized Chaplygin gas
- Large scale structure and the generalised Chaplygin gas as dark energy
- f(R) Gravity: From the Pioneer Anomaly to the Cosmic Acceleration
- Extended quintessence with an exponential coupling
- Non-minimally coupled f(R) Cosmology
- Accelerating universe in scalar tensor models - confrontation of theoretical predictions with observations
- Constraints on extended quintessence from high-redshift Supernovae
- Inverse problem: Reconstruction of modified gravity action in Palatini formalism by Supernova Type Ia data
- Consistency Condition of Spherically Symmetric Solutions in Gravity
- A Model of f(R) Gravity as an Alternative for Dark Matter in Spiral Galaxies
- A Well-Behaved f(R) Gravity Model in Planetary Motions
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- Late Time Cosmological Evolution in f(R) theories with Ordinary and Collisional Matter
- Specific neutral and charged black holes in gravitational theory
- A Note on Gravitational Memory in F(R)-theories and their Equivalent Scalar-Tensor Theories