paper

Phantom Thermodynamics Revisited

arXiv:astro-ph/0412704

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.

4 pages; 1 figure

Phantom Thermodynamics Revisited · wovepaper