A Dark Energy Model in Lyra Manifold
arXiv:1204.0774 · doi:10.1016/j.geomphys.2012.08.004
Abstract
We consider, in normal-gauge Lyra's geometry, evolution of a homogeneous isotropic universe in a gravitational model involving only the standard matter in interaction with a displacement vector field . Considering both constant and time-dependent displacement vector field we show that the observed cosmic acceleration could be explained without considering an alien energy component with a negative pressure.
15 pages, 2 figures, LaTeX file
References in corpus (81)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Dynamics of dark energy
- The Cosmological Constant and Dark Energy
- Cosmological parameters from SDSS and WMAP
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Cosmological Constant - the Weight of the Vacuum
- The Case for a Positive Cosmological Lambda-term
- Cosmology and the Fate of Dilatation Symmetry
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- The Cosmological Constant
- 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 Model of Holographic Dark Energy
- k-Inflation
- Essentials of k-essence
- The 3D power spectrum of galaxies from the SDSS
- Kinetically Driven Quintessence
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis
- Curvature Quintessence
- Can the dark energy equation-of-state parameter w be less than -1?
- The Fourth Data Release of the Sloan Digital Sky Survey
- Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
- Accelerated expansion of the universe driven by tachyonic matter
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- The First Data Release of the Sloan Digital Sky Survey
- Dark Energy
- Cosmological Evolution of a Quintom Model of Dark Energy
- A Dark Energy Model Characterized by the Age of the Universe
- Cosmology with tachyon field as dark energy
- A New Model of Agegraphic Dark Energy
- Is there Supernova Evidence for Dark Energy Metamorphosis ?
- Quantum effects can render w<-1 on cosmological scales
- Constraints on holographic dark energy from type Ia supernova observations
- Modified gravity with terms and cosmic acceleration
- The Holographic Dark Energy in a Non-flat Universe
- Where new gravitational physics comes from: M-theory?
- Super-Acceleration from Massless, Minimally Coupled
- Oscillating Quintom and the Recurrent Universe
- Self-tuning flat domain walls in 5d gravity and string theory
- Hessence: A New View of Quintom Dark Energy
- Supernova Constraints on a holographic dark energy model
- Holographic dark energy models: A comparison from the latest observational data
- The foundations of observing dark energy dynamics with the Wilkinson Microwave Anisotropy Probe
- Quintom models with an equation of state crossing -1
- New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter
- Two Loop Scalar Self-Mass during Inflation
- Generalized Second Law of Thermodynamics in Quintom Dominated Universe
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error Limits
- Cosmological Evolution of Hessence Dark Energy and Avoidance of the Big Rip
- A Single Scalar Field Model of Dark Energy with Equation of State Crossing -1
- Probing interaction and spatial curvature in the holographic dark energy model
- Coupled oscillators as models of quintom dark energy
- Anthropic Principle Favors the Holographic Dark Energy
- Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
- Palatini Formulation of Modified Gravity with Terms
- Quintom model with O() symmetry
- Constraints on Oscillating Quintom from Supernova, Microwave Background and Galaxy Clustering
- Quintom Cosmology with General Potentials
- A Dynamical Approach to the Cosmological Constant
- Shape invariance method for quintom model in the bent brane background
- Current Observational Constraints to Holographic Dark Energy Model with New Infrared cut-off via Markov Chain Monte Carlo Method
- Non-minimally Coupled Quintom Model Inspired by String Theory
- The State Equation of the Yang-Mills field Dark Energy Models
- A Completely Regular Quantum Stress Tensor with
- Quintom dark energy models with nearly flat potentials
- A Brane World Solution to the Cosmological Constant Problem
- Alleviation of Cosmic Age Problem In Interacting Dark Energy Model
- 2-loop Quantum Yang-Mills Condensate as Dark Energy
- Yang-Mills condensate dark energy coupled with matter and radiation
- Coincidence Problem in YM Field Dark Energy Model
- Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations
- 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
- A cosmological constant from degenerate vacua
- Dynamical vacuum energy via adjustment mechanism
- An Approach to the Cosmological Constant Problem(s)
- Axially Symmetric Cosmological Mesonic Stiff Fluid Models in Lyra's Geometry
Cited by in corpus (6)
- Static traversable wormholes in Lyra manifold
- Cosmology with an Effective -Term in Lyra Manifold
- Trapped surfaces and nature of singularities in Lyra's geometry
- Dynamical stability of an interacting quintessence with varying-mass dark matter particles in Lyra manifold
- A Higher Dimensional Cosmological Model for the Search of Dark Energy Source
- Exact Cosmological Models with the Yang - Mills Fields on Lyra Manifold