Speaker
Prof.
Daniel Grumiller
(TU Wien)
Description
Despite the absence of a lightcone structure, some solutions of Carroll
gravity show black hole-like behaviour. We define Carroll black holes as
solutions of Carroll gravity that exhibit Carroll thermal properties and
have a Carroll extremal surface. Examples include Carroll versions of
Schwarzschild, Reissner-Nordström, BTZ, JT, and Witten black holes.
