中文

Quantum cosmological perfect fluid models

广义相对论与量子宇宙学 2021-10-20 v2

摘要

Perfect fluid Friedmann-Robertson-Walker quantum cosmological models for an arbitrary barotropic equation of state p=αρp = \alpha\rho are constructed using Schutz's variational formalism. In this approach the notion of time can be recovered. By superposition of stationary states, finite-norm wave-packet solutions to the Wheeler-DeWitt equation are found. The behaviour of the scale factor is studied by applying the many-worlds and the ontological interpretations of quantum mechanics. Singularity-free models are obtained for α<1\alpha < 1. Accelerated expansion at present requires 1/3>α>1- 1/3 > \alpha > - 1.

关键词

引用

@article{arxiv.gr-qc/0106051,
  title  = {Quantum cosmological perfect fluid models},
  author = {F. G. Alvarenga and J. C. Fabris and N. A. Lemos and G. A. Monerat},
  journal= {arXiv preprint arXiv:gr-qc/0106051},
  year   = {2021}
}

备注

Latex file, 12 pages. New paragraphs in the Introduction and Conclusion, and other minor corrections in the text and in some formulas. Accepted for publication in General Relativity and Gravitation