Interacting phantom energy
- 3 January 2005
- journal article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 71 (2) , 023501-1
- https://doi.org/10.1103/physrevd.71.023501
Abstract
We investigate the role of a suitable interaction between a matter fluid and a phantom field for the coincidence problem. There exists a stationary scaling solution which is a stable attractor at late times. Furthermore, the cosmic doomsday is avoided in one region of the parameter space.Keywords
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This publication has 36 references indexed in Scilit:
- Is there supernova evidence for dark energy metamorphosis?Monthly Notices of the Royal Astronomical Society, 2004
- The case for dynamical dark energy revisitedJournal of Cosmology and Astroparticle Physics, 2004
- How to test stringy dark energy?Physics Letters B, 2003
- Cosmology and the fate of dilatation symmetryPublished by Elsevier ,2002
- A phantom menace? Cosmological consequences of a dark energy component with super-negative equation of statePublished by Elsevier ,2002
- Modified dispersion relations from closed strings in toroidal cosmologyPhysical Review D, 2002
- Relic dark energy from the trans-Planckian regimePhysical Review D, 2001
- Cosmological tracking solutionsPhysical Review D, 1999
- Quintessence, Cosmic Coincidence, and the Cosmological ConstantPhysical Review Letters, 1999
- Cosmological consequences of a rolling homogeneous scalar fieldPhysical Review D, 1988