Interaction between phantom field and modified Chaplygin gas
arXiv:1012.5633 · doi:10.1007/s10509-009-0237-x
Abstract
In this letter, we have considered a flat FRW universe. Instead of considering only one candidate for dark energy, we have considered interaction between phantom field and modified Chaplygin gas. It has been shown that the potential of the phantom field increases from a lower value with evolution of the Universe. It has been observed that, the field has an increasing tendency and potential has also an increasing tendency with passage of cosmic time. In the evolution of the universe the crossing of has been realized by this interacting model.
6 pages
References in corpus (24)
- Dynamics of dark energy
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- An alternative to quintessence
- A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
- Can the dark energy equation-of-state parameter w be less than -1?
- The Cosmic Triangle: Revealing the State of the Universe
- Exploring the Expanding Universe and Dark Energy using the Statefinder Diagnostic
- Cosmological Evolution of a Quintom Model of Dark Energy
- Can dark energy evolve to the Phantom?
- Transition of the dark energy equation of state in an interacting holographic dark energy model
- Interacting Quintessence
- Cosmological Dynamics of Phantom Field
- Can the Chaplygin gas be a plausible model for dark energy?
- The State of the Dark Energy Equation of State
- Role of Modified Chaplygin Gas in Accelerated Universe
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Interacting generalized Chaplygin gas model in non-flat universe
- Phantom-like GCG and the constraints of its parameters via cosmological dynamics
- Cosmology with a Variable Chaplygin Gas
- Variable Modified Chaplygin Gas and Accelerating Universe
- Exact models with non-minimal interaction between dark matter and (either phantom or quintessence) dark energy
- Interacting cosmic fluids in power-law Friedmann-Robertson-Walker cosmological models
- Density Evolution in the New Modified Chaplygin Gas Model
Cited by in corpus (5)
- Two-fluid evolving Lorentzian wormholes
- Dynamics of interacting phantom and quintessence dark energies
- Phantom evolving wormholes with big rip singularities
- Reconstructing f(R) Gravity from a Chaplygin Scalar Field in de Sitter Spacetimes
- Canonical and phantom scalar fields as an interaction of two perfect fluids