Phantom Thermodynamics Revisited
Astrophysics
2007-05-23 v3
Abstract
Although generalized Chaplygin phantom models do not show any big rip singularities, we investigated k-essence models together with noncanonical kinetic energy for which there might be a big rip future singularity in the phantom region. We present our results by finely tuning the parameter () which is closely related to the canonical kinetic term in -essence formalism. The scale factor could be negative and decreasing within a specific range of during the initial evolutional period. There will be no singularity for the scale factor for all times once is carefully selected.
Cite
@article{arxiv.astro-ph/0412704,
title = {Phantom Thermodynamics Revisited},
author = {A. Kwang-Hua Chu},
journal= {arXiv preprint arXiv:astro-ph/0412704},
year = {2007}
}
Comments
4 pages; 1 figure