Abstract
The Einstein theory of gravitation breaks down at very high curvatures. We propose a modification of the theory at Planck curvatures for which all isotropic cosmological solutions (even including matter) are nonsingular. All solutions asymptotically approach de Sitter space, a solution with limiting curvature.
- Received 11 December 1991
DOI:https://doi.org/10.1103/PhysRevLett.68.1969
©1992 American Physical Society