Nonsingular Chaplygin gas cosmologies in universes connected by wormhole
arXiv:1205.1542 · doi:10.1134/S0202289313010076
Abstract
We present some exact solutions of the Einstein equations with an anisotropic fluid exploiting the Chaplygin equation of state. The solutions describe spacetimes with two identical T regions and an intermediate static spherically symmetric R region containing a wormhole. The metric in the T region represents an anisotropic Kantowski-Sachs cosmological model. Its evolution starts from an event horizon and develops according to different scenarios including eternal expansion, contraction and also a finite universe lifetime.
14 pages, 9 figures