Chaplygin gas may prevent big trip
arXiv:astro-ph/0512117 · doi:10.1016/j.physletb.2006.01.060
Abstract
This paper deals with the study of the accretion of a generalized Chaplygin gas with equation of state onto wormholes. We have obtained that when dominant energy condition is violated the size of wormhole increases with the scale factor up to a given plateau. On the regime where the dominant energy condition is satisfied our model predicts a steady decreasing of the wormhole size as generalized Chaplygin gas is accreted. Our main conclusion is that the big trip mechanism is prevented in a large region of the physical parameters of the used model.
6 pages, no figures, uses Revtex. Several typos corrected. References updated
References in corpus (62)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- The Cosmological Constant and Dark Energy
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Cosmological parameters from SDSS and WMAP
- Cosmological Imprint of an Energy Component with General Equation of State
- Cosmological Constant - the Weight of the Vacuum
- Cosmology and the Fate of Dilatation Symmetry
- An alternative to quintessence
- Is Cosmic Speed-Up Due to New Gravitational Physics?
- Phantom Energy and Cosmic Doomsday
- 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
- k-Inflation
- Essentials of k-essence
- Cosmological Results from High-z Supernovae
- Kinetically Driven Quintessence
- Perturbations in k-inflation
- Accelerated Universe from Gravity Leaking to Extra Dimensions
- Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
- Cluster Abundance Constraints on Quintessence Models
- Cosmology on a Brane in Minkowski Bulk
- Braneworld models of dark energy
- The final state and thermodynamics of dark energy universe
- Phantom energy traversable wormholes
- Can the Chaplygin gas be a plausible model for dark energy?
- Black hole mass decreasing due to phantom energy accretion
- The end of unified dark matter?
- Extended tachyon field, Chaplygin gas and solvable k-essence cosmologies
- The dS/CFT Correspondence and the Big Smash
- WMAP and the Generalized Chaplygin Gas
- Generalized Chaplygin gas and CMBR constraints
- WMAP Constraints on the Generalized Chaplygin Gas Model
- K-Essential Phantom Energy: Doomsday around the corner?
- Density perturbations in an Universe dominated by the Chaplygin gas
- You need not be afraid of phantom energy
- Cosmological consequences of a Chaplygin gas dark energy
- Are Chaplygin gases serious contenders to the dark energy throne?
- Latest Supernova data in the framework of Generalized Chaplygin Gas model
- A new view of k-essence
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: observational constraints
- Resolving the Cosmological Missing Energy Problem
- K-essence and the coincidence problem
- Constraints on Chaplygin quartessence from the CLASS gravitational lens statistics and supernova data
- Avoidance of Big Rip In Phantom Cosmology by Gravitational Back Reaction
- Large scale structure and the generalised Chaplygin gas as dark energy
- Escaping the Big Rip?
- The Role of Baryons in Unified Dark Matter Models
- Achronal cosmic future
- FRW Quantum Cosmology with a Generalized Chaplygin Gas
- Nonlinear Realization of a Dynamical Poincare Symmetry by a Field-dependent Diffeomorphism
- The Imprint of Gravitational Waves in Models Dominated by a Dynamical Cosmic Scalar Field
- Phantom inflation and the "Big Trip"
- Generalized Chaplygin Gas Models tested with SNIa
- Cosmological models from quintessence
- Mass Power Spectrum in a Universe Dominated by the Chaplygin Gas
- Bayesian Analysis of the (Generalized) Chaplygin Gas and Cosmological Constant Models using the 157 gold SNe Ia Data
- A two-scalar model for a small but nonzero cosmological constant
- On the accretion of phantom energy onto wormholes
- Decelerating universes older than their Hubble times
- Apocalypse soon
Cited by in corpus (12)
- Chaplygin traversable wormholes
- Phantom stars and topology change
- Conformally symmetric traversable wormholes
- Finite-time Cosmological Singularities and the Possible Fate of the Universe
- Emergent Universe Scenario in the Einstein-Gauss-Bonnet Gravity with Dilaton
- On the formalism of dark energy accretion onto black- and worm-holes
- Phantom evolving wormholes with big rip singularities
- Pre-Inflationary Spacetime in String Cosmology
- Constraints on the generalized tachyon field models from latest observational data
- Accretions of Various Types of Dark Energies onto Morris-Thorne Wormhole
- No "big trips" for the universe
- Big rip avoidance via black holes production