Shape invariance method for quintom model in the bent brane background
arXiv:0712.1873 · doi:10.1016/j.physletb.2008.01.024
Abstract
In the present paper, we study the braneworld scenarios in the presence of quintom dark energy coupled by gravity. The first-order formalism for the bent brane (for both de Sitter and anti-de Sitter geometry), leads us to discuss the shape invariance method in the bent brane systems. So, by using the fluctuations of metric and quintom fields we obtain the Schrodinger equation. Then we factorize the corresponding Hamiltonian in terms of multiplication of the first-order differential operators. These first-order operators lead us to obtain the energy spectrum with the help of shape invariance method.
13 pages, no figure
References in corpus (15)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Supersymmetry and Quantum Mechanics
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- Cosmological Tracking Solutions
- Tachyon Matter
- Accelerated expansion of the universe driven by tachyonic matter
- Constraints on Cosmological Models from Hubble Space Telescope Observations of High-z Supernovae
- Unified phantom cosmology: inflation, dark energy and dark matter under the same standard
- Oscillating Quintom and the Recurrent Universe
- Interacting Holographic Phantom
- Generalized Second Law of Thermodynamics in Quintom Dominated Universe
- Holographic tachyon model of dark energy
- Constraints on Oscillating Quintom from Supernova, Microwave Background and Galaxy Clustering
Cited by in corpus (64)
- Quintom Cosmology: Theoretical implications and observations
- Thermodynamics of dark energy interacting with dark matter and radiation
- Non-minimally coupled canonical, phantom and quintom models of holographic dark energy
- Holographic dark energy with varying gravitational constant
- Coupled oscillators as models of quintom dark energy
- Quintom model with O() symmetry
- Observational constraints on holographic dark energy with varying gravitational constant
- Interacting tachyon dark energy in non-flat universe
- Quintom Cosmology with General Potentials
- Holographic dark energy in Brans-Dicke cosmology with chameleon scalar field
- Superintegrability with third order integrals of motion, cubic algebras and supersymmetric quantum mechanics II:Painleve transcendent potentials
- Internal space structure generalization of the quintom cosmological scenario
- Braneworld models with a non-minimally coupled phantom bulk field: a simple way to obtain the -1-crossing at late times
- Reconstruction of cosmic history from a simple parametrization of H
- Theoretical Limits on the Equation-of-State Parameter of Phantom Cosmology
- Statefinder diagnostic and stability of modified gravity consistent with holographic and new agegraphic dark energy
- A Completely Regular Quantum Stress Tensor with
- Quintom dark energy models with nearly flat potentials
- The bouncing cosmology with gravity and its reconstructing
- Correspondence between entropy-corrected holographic and Gauss-Bonnet dark energy models
- Phantom phase power-law solution in gravity
- Viscous dark energy and generalized second law of thermodynamics
- Power-law solutions in gravity
- Non-minimal Maxwell-Modified Gauss-Bonnet Cosmologies: Inflation and Dark Energy
- Cosmic acceleration and crossing of in non-minimal modified Gauss-Bonnet gravity
- Bounce cosmology in gravity
- Thermodynamics of viscous dark energy in an RSII braneworld
- Interacting new agegraphic viscous dark energy with varying
- Reconstructing a String-Inspired Quintom Model of Dark Energy
- Statefinder diagnostic for modified Chaplygin gas cosmology in f(R,T) gravity with particle creation
- Thermodynamics of the viscous gravity in the new agegraphic dark energy model
- Reconstructing a String-Inspired Non-minimally Coupled Quintom Model
- Interacting Dark Energy in Hořava-Lifshitz Cosmology
- Cosmological Evolution of a Tachyon-Quintom Model of Dark Energy
- Thermodynamics and stability of gravity with viscous fluid by observational constraints
- On dark energy models of single scalar field
- Cosmological Evolution Across Phantom Crossing and the Nature of the Horizon
- String Inspired Quintom Model with Non-minimally Coupled Modified Gravity
- Stability and interacting gravity with modified Chaplygin gas
- Interacting gravity with modified Chaplygin gas
- A Dark Energy Model in Lyra Manifold
- Cosmological Tests of Dark Energy Model in FRW Universe
- Galileons, phantom fields, and the fate of the Universe
- Holographic dark energy with time depend gravitational constant in the non-flat Hoava-Lifshitz cosmology
- Quintom dark energy in DGP braneworld cosmology
- Interacting new agegraphic Phantom model of dark energy in non-flat universe
- Quantum cosmology with symmetry analysis for quintom dark energy model
- Quintom cosmological model and some possible solutions using Lie and Noether symmetries
- Observational constraints and stability in viscous gravity
- Non-minimal coupling of the phantom field and cosmic acceleration
- Extended Bose-Einstein condensate dark matter in viscous Gauss-Bonnet gravity
- The interaction of extended Bose-Einstein condensate dark matter with viscous gravity
- Observational Hubble parameter data constraints on the interactive model of gravity with particle creation
- Cosmological observations in non-local cosmology
- Friedmann-Robertson-Walker Models with Late-Time Acceleration
- Chameleon gravity on cosmological scales
- Dynamics of the self-interacting chameleon cosmology
- Cosmological models based on a complex scalar field with a power-law potential associated with a polytropic equation of state
- Interacting Three Fluid System and Thermodynamics of the Universe Bounded by the Event Horizon
- Interacting non-minimally coupled canonical, phantom and quintom models of holographic dark energy in non-flat universe
- Viscous interacting and stability on dark matter Bose-Einstein condensation with modified Chaplygin gas
- Reconstructing cosmic evolution with a density parametrization
- Evolution of the horizons for dark energy universe
- Correspondence between particle creation and dark components interaction in the context of gravity