Why is Black Hole Entropy Affected by Rotation?

TL;DR

This paper investigates how rotation affects black hole entropy in both asymptotically flat and AdS spacetimes, revealing that rotation generally decreases entropy at fixed temperature and exploring implications via gauge-gravity duality.

Contribution

It demonstrates that rotating black holes have lower specific entropy than non-rotating ones at fixed temperature, extending the analysis to AdS$_5$-Kerr black holes and linking results to gauge-gravity duality.

Findings

Rotating Kerr black holes have smaller entropy than Schwarzschild at fixed temperature.

AdS$_5$-Kerr black holes generally have lower entropy than AdS$_5$-Schwarzschild.

Predictions from QGP theory align with the entropy behavior of AdS$_5$-Kerr black holes.

Abstract

It is well known that an asymptotically flat four-dimensional Kerr black hole has a smaller (specific) entropy than a Schwarzschild black hole of the same mass. We show here that the same is true if the temperature, rather than the mass, is held fixed; and we also show that an asymptotically AdS$_5$-Kerr black hole has a smaller specific entropy than an AdS$_5$-Schwarzschild black hole of the same temperature, except in a negligibly small class of special examples. The AdS$_5$-Kerr case is particularly interesting, because here the gauge-gravity duality applies; if we further accept that there is a useful analogy between the strongly coupled field theories dual to AdS black holes and the best-understood example of a strongly coupled fluid (the Quark-Gluon Plasma), then we can apply QGP theory to predict the behaviour of black hole entropy in this case. The prediction agrees with our study of AdS$_5$-Kerr entropy. The hope is that such results might lead ultimately to an identification of black hole microstates.