The "physical process" version of the first law and the generalized second law for charged and rotating black holes
Sijie Gao, Robert M. Wald

TL;DR
This paper proves the physical process version of the first law and confirms the generalized second law of thermodynamics for charged and rotating black holes during matter infall and lowering processes, without assuming entropy bounds.
Contribution
It derives formulas for first-order variations in black hole parameters and proves the GSL for charged, rotating black holes during specific physical processes.
Findings
The first law holds for charged, rotating black holes under linear perturbations.
The generalized second law is valid during matter lowering and release processes.
No entropy bounds on matter are required for the GSL to hold.
Abstract
We investigate both the ``physical process'' version of the first law and the second law of black hole thermodynamics for charged and rotating black holes. We begin by deriving general formulas for the first order variation in ADM mass and angular momentum for linear perturbations off a stationary, electrovac background in terms of the perturbed non-electromagnetic stress-energy, , and the perturbed charge current density, . Using these formulas, we prove the "physical process version" of the first law for charged, stationary black holes. We then investigate the generalized second law of thermodynamics (GSL) for charged, stationary black holes for processes in which a box containing charged matter is lowered toward the black hole and then released (at which point the box and its contents fall into the black hole and/or thermalize with the ``thermal…
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