A String-Inspired Quintom Model Of Dark Energy
arXiv:hep-th/0701016 · doi:10.1016/j.physletb.2007.05.056
Abstract
We propose in this paper a quintom model of dark energy with a single scalar field given by the lagrangian . In the limit of 0 our model reduces to the effective low energy lagrangian of tachyon considered in the literature. We study the cosmological evolution of this model, and show explicitly the behaviors of the equation of state crossing the cosmological constant boundary.
6 pages, 4 figures, accepted by PLB
References in corpus (40)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
- Dark Energy Constraints from the Cosmic Age and Supernova
- Rolling Tachyon
- Tachyon Matter
- 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
- Cosmological Evolution of a Quintom Model of Dark Energy
- Can dark energy evolve to the Phantom?
- Field Theory of Tachyon Matter
- Cosmological Evolution of the Rolling Tachyon
- Cosmology with tachyon field as dark energy
- Constraints on holographic dark energy from type Ia supernova observations
- Some Exact Results on Tachyon Condensation in String Field Theory
- Oscillating Quintom and the Recurrent Universe
- Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom
- What is needed of a tachyon if it is to be the dark energy?
- On Exact Tachyon Potential in Open String Field Theory
- Perturbations of the Quintom Models of Dark Energy and the Effects on Observations
- Crossing of the w=-1 Barrier by D3-brane Dark Energy Model
- Quintom models with an equation of state crossing -1
- Generalized Second Law of Thermodynamics in Quintom Dominated Universe
- Two-field Models of Dark Energy with Equation of State Across -1
- Crossing w=-1 in Gauss-Bonnet Brane World with Induced Gravity
- A Single Scalar Field Model of Dark Energy with Equation of State Crossing -1
- Brane cosmology driven by the rolling tachyon
- Dark-Energy Evolution Across the Cosmological-Constant Boundary
- On the Cosmological Relevance of the Tachyon
- Interacting Vector-like Dark Energy, the First and Second Cosmological Coincidence Problems
- Time and Tachyon
- Cosmic Duality in Quintom Universe
- Decay of Unstable D-branes with Electric Field
- Tachyonic Inflation in the Braneworld Scenario
- Late acceleration and crossing in induced gravity
- Crossing by a single scalar on a Dvali-Gabadadze-Porrati brane
- Critical comments on the paper "Crossing by a single scalar field on a Dvali-Gabadadze-Porrati brane" by H Zhang and Z-H Zhu [Phys.Rev.D75,023510(2007)]
- Reconstructing the Equation of State of Tachyon
- Avoiding the Big-Rip Jeopardy in a Quintom Dark Energy Model with Higher Derivatives
- Supernova Constraints on Models of Neutrino Dark Energy
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- Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy
- Bouncing Galileon Cosmologies
- Crossing of the phantom divide in modified gravity
- On Perturbations of Quintom Bounce
- The Cosmological Dynamics of Interacting Holographic Dark Energy Model
- Noether Symmetry Approach in f(R) Tachyon Model
- Age Problem in the Holographic Dark Energy Model
- Dark Energy Model with Spinor Matter and Its Quintom Scenario
- Holographic dark energy in a cyclic universe
- Thermodynamical Interpretation of the Interacting Holographic Dark Energy Model in a non-flat Universe
- Two-Fluid Scenario for Dark Energy Models in an FRW Universe-Revisited
- Dark energy in light of the early JWST observations: case for a negative cosmological constant?
- Evolution of Metric Perturbations in Quintom Bounce model
- Internal space structure generalization of the quintom cosmological scenario
- Quintom cosmology and modified gravity after DESI 2024
- Dark energy model with higher derivative of Hubble parameter
- The past and future dynamics of quintom dark energy models
- Primordial perturbation with a modified dispersion relation
- Dynamics of interacting phantom scalar field dark energy in Loop Quantum Cosmology
- Inflationary universe in loop quantum cosmology
- A Completely Regular Quantum Stress Tensor with
- Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
- Crossing the phantom divide in an interacting generalized Chaplygin gas
- Emergent Universe Scenario via Quintom Matter
- Tachyonic Teleparallel Dark Energy
- Implications of the possible 21-cm line excess at cosmic dawn on dynamics of interacting dark energy
- Tachyon Reconstruction of Ghost Dark Energy
- Phantom-Like Behavior in -Gravity
- Generalised teleparallel quintom dark energy non-minimally coupled with the scalar torsion and a boundary term
- Gauss-Bonnet Chameleon Mechanism of Dark Energy
- Reconstructing a String-Inspired Quintom Model of Dark Energy
- Bounce Inflation Cosmology with Standard Model Higgs Boson
- Cyclic Universe with Quintom matter in Loop Quantum Cosmology
- Two-fluid atmosphere from decelerating to accelerating FRW dark energy models
- Cosmology of F(R) nonlinear massive gravity
- Multiple kinetic k-essence, phantom barrier crossing and stability
- Crossing of with Tachyon and Non-minimal Derivative Coupling
- Tachyon Inflation in Teleparallel Gravity
- A Non-minimally Coupled Quintom Dark Energy Model on the Warped DGP Brane
- Theoretical Aspects of Quintom Models
- Interaction between viscous varying modified cosmic Chaplygin gas and Tachyonic fluid
- Cosmological Evolution of a Tachyon-Quintom Model of Dark Energy
- On dark energy models of single scalar field
- String Inspired Quintom Model with Non-minimally Coupled Modified Gravity
- Reexploration of interacting holographic dark energy model: Cases of interaction term excluding the Hubble parameter
- Thermodynamics of Spinor Quintom
- Holographic approach for dark energy - dark matter interaction in curved FLRW spacetime
- Self-interacting holographic dark energy
- Inflationary Krylov complexity
- Can the Big Bang Singularity be avoided by a single scalar field?
- Null Energy Condition and Dark Energy Models
- Crossing the cosmological constant line in a dilatonic brane-world model with and without curvature corrections
- Chameleon Cosmology Model Describing the Phantom Divide Line Crossing
- Gaussian-process reconstructions and model building of quintom dark energy from latest cosmological observations
- Density perturbation in an interacting holographic dark energy model
- Stability analysis of the cosmological solutions with induced gravity and scalar field on the brane
- Crossing the Phantom divide line in the Chaplygin gas model
- Multi-fluid cosmology in Einstein gravity: analytical solutions
- Unification of cosmological scalar fields
- Quintom potentials from quantum cosmology using the FRW cosmological model
- Falsifying Field-based Dark Energy Models
- Phantom without phantom or how the PT symmetry saves us from the Big Rip
- Qualitative analysis and characterization of two cosmologies including scalar fields
- Deformation of the quintom cosmological model and its consequences
- Cosmological complexity of the modified dispersion relation
- Phantom Divide Crossing with General Non-minimal Kinetic Coupling
- Black Holes in Accelerated Universe
- The torsion cosmology in Kaluza-Klein theory
- A short review on Quintom dark energy theory
- Perturbations In Some Dark Energy Models