Entropy, black holes, and the new cyclic universe

Entropy, black holes, and the new cyclic universe

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We track the evolution of entropy and black holes in a cyclic universe that undergoes repeated intervals of expansion followed by slow contraction and a smooth (non-singular) bounce.In this kind of cyclic scenario, there is no big crunch emtek 2113 and no chaotic mixmaster behavior.We explain why the entropy following each bounce is naturally partitioned into near-maximal entropy in g5210t-p90 the matter-radiation sector and near-minimal in the gravitational sector, satisfying the Weyl curvature conditions conjectured to be essential for a cosmology consistent with observations.As a result, this kind of cyclic universe can undergo an unbounded number of cycles in the past and/or the future.