Does Vacuum Energy Allow for Computational “Bits” at the Start of Cosmological Evolution, and Their Possible Ties to Torsion Physics

Abstract

Based on the notion that torsion cancels cosmological vacuum energy [1], we
consider if relic black holes at the start of inflation may allow for the observed
cosmological constant. If thermal energy used at the start of inflation creates
conceptual issues, an energy term based on Corda’s treatment of black holes
may provide a solution, a leftover cosmological constant 10−121 times vacuum
energy. Considerations as to how black-hole physics may contribute to torsion
and the cosmological constant are considered in several numerical cases. Also
we present entanglement entropy in the early universe with a shrinking scale
factor [2] and show that consequences arise due to initial entangled for a timedependent
horizon radius in cosmology with flat space conditions for conformal
time. This construction preserves a minimum nonzero vacuum energy, and, in
doing so, keeps the computational bits for cosmological evolution. The bits are
ascribed to initial torsion as we describe.