The Generalized Second Law implies a Quantum Singularity Theorem
Aron C. Wall

TL;DR
This paper demonstrates that the generalized second law of thermodynamics leads to a quantum version of Penrose's singularity theorem, constraining the nature of spacetime, black holes, and cosmological models in quantum gravity.
Contribution
It extends Penrose's classical singularity theorem to quantum scenarios using the generalized second law, introducing a quantum notion of trapped surfaces and implications for spacetime structure.
Findings
Spacetime is null geodesically incomplete inside black holes.
The law rules out traversable wormholes and faster-than-light travel.
Finite entropy processes imply a reversal of the arrow of time in finite space.
Abstract
The generalized second law can be used to prove a singularity theorem, by generalizing the notion of a trapped surface to quantum situations. Like Penrose's original singularity theorem, it implies that spacetime is null geodesically incomplete inside black holes, and to the past of spatially infinite Friedmann--Robertson--Walker cosmologies. If space is finite instead, the generalized second law requires that there only be a finite amount of entropy producing processes in the past, unless there is a reversal of the arrow of time. In asymptotically flat spacetime, the generalized second law also rules out traversable wormholes, negative masses, and other forms of faster-than-light travel between asymptotic regions, as well as closed timelike curves. Furthermore it is impossible to form baby universes which eventually become independent of the mother universe, or to restart inflation.…
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