中文

Phantom Thermodynamics Revisited

天体物理学 2007-05-23 v3

摘要

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 (β\beta) which is closely related to the canonical kinetic term in kk-essence formalism. The scale factor a(t)a(t) could be negative and decreasing within a specific range of β\beta during the initial evolutional period. There will be no singularity for the scale factor for all times once β\beta is carefully selected.

引用

@article{arxiv.astro-ph/0412704,
  title  = {Phantom Thermodynamics Revisited},
  author = {A. Kwang-Hua Chu},
  journal= {arXiv preprint arXiv:astro-ph/0412704},
  year   = {2007}
}

备注

4 pages; 1 figure