Abstract
We discuss again the approach to cyclic cosmology based on the 2007 Baum–Frampton model. By introducing the relationship between entanglement entropy and space–time connectivity first introduced by Van Raamsdonck (2010) we show how vanishing entropy at the turnaround, and hence at the bounce after adiabatic contraction, can be better understood in this solution to the Tolman entropy conundrum.
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