Logarithmic corrected Polynomial inflation mimicking a cosmological constant
arXiv:1510.02351 · doi:10.1142/S0218271816500772
Abstract
In this paper, we consider an inflationary model of gravity with polynomial form plus logarithmic term. We calculate some cosmological parameters and compare our results with the Plank 2015 data. We find that presence of both logarithmic and polynomial corrections are necessary to yield slow-roll condition. Also, we study critical points and stability of the model to find that it is a viable model.
15 pages, 9 figures
References in corpus (46)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- 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
- Essentials of k-essence
- Coupled Quintessence
- Kinetically Driven Quintessence
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Curvature Quintessence
- Quintom Cosmology: Theoretical implications and observations
- Conditions for the cosmological viability of f(R) dark energy models
- A classification of scalar field potentials with cosmological scaling solutions
- Curvature quintessence matched with observational data
- Prospects for probing the dark energy via supernova distance measurements
- Quantum effects can render w<-1 on cosmological scales
- Role of Modified Chaplygin Gas in Accelerated Universe
- On Physical Equivalence between Nonlinear Gravity Theories
- Quintessence without scalar fields
- Stationary dark energy: the present universe as a global attractor
- Cosmological inflation in gravity
- Tracking and coupled dark energy as seen by WMAP
- Quintom models with an equation of state crossing -1
- Constraints on Perturbative f(R) Gravity via Neutron Stars
- A polynomial f(R) inflation model
- Parametrizations of the Dark Energy Density and Scalar Potentials
- Viscous Modified Cosmic Chaplygin Gas Cosmology
- Dark energy from a quintessence (phantom) field rolling near potential minimum (maximum)
- Cosmo-dynamics and dark energy with non-linear equation of state: a quadratic model
- Aetherizing Lambda: Barotropic Fluids as Dark Energy
- FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space
- Structure of neutron stars in R-squared gravity
- Higher order corrections of the extended Chaplygin gas cosmology with varying and
- Modified gravity with logarithmic curvature corrections and the structure of relativistic stars
- Theoretical Limits on the Equation-of-State Parameter of Phantom Cosmology
- Bouncing inflation in nonlinear gravitational model
- Interacting Quintessence Models of Dark Energy
- Correspondence between DBI-essence and Modified Chaplygin Gas and the Generalized Second Law of Thermodynamics
- Neutron stars in a perturbative gravity model with strong magnetic fields
- The generalized second law for the interacting generalized Chaplygin gas model
- Logarithmic corrected gravity in the light of Planck 2015
- Thermodynamics of Chaplygin gas
- Thermodynamics of Modified Chaplygin Gas and Tachyonic Field
- A new model of arcsin-gravity
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- Gravity Effects on Charged Accelerating AdS Black Holes using Holographic Tools