A Cosmological Theory without Singularities
广义相对论与量子宇宙学
2009-10-22 v1 天体物理学
高能物理 - 理论
摘要
A theory of gravitation is constructed in which all homogeneous and isotropic solutions are nonsingular, and in which all curvature invariants are bounded. All solutions for which curvature invariants approach their limiting values approach de Sitter space. The action for this theory is obtained by a higher derivative modification of Einstein's theory. We expect that our model can easily be generalized to solve the singularity problem also for anisotropic cosmologies.
引用
@article{arxiv.gr-qc/9303001,
title = {A Cosmological Theory without Singularities},
author = {R. Brandenberger and V. Mukhanov and A. Sornborger},
journal= {arXiv preprint arXiv:gr-qc/9303001},
year = {2009}
}
备注
25 pages, 11 figures (available as hard copies from the authors), uses phyzzx, BROWN-HET-891