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Speaker
Daniel Grumiller
(TU Wien)
Description
Carroll symmetries arise generically on null hypersurfaces, such as black hole event horizons or null infinity in asymptotically flat spacetimes. Carroll gravity is a gravitational theory based on Carroll symmetries. Carroll black holes are solutions of Carroll gravity that exhibit Carroll thermal properties and have a Carroll extremal surface. I review, motivate, and explain all these notions and address recent results on the Carroll Hawking effect.
Primary authors
Alfredo Perez
(CECs Valdivia)
Daniel Grumiller
(TU Wien)
Mr
Florian Ecker
(TU Wien)
Jelle Hartong
(Edinburgh U.)
Ricardo Troncoso
(CECs Valdivia)
Stefan Prohazka
(Edinburgh U.)
Co-authors
Ankit Aggarwal
(TU Wien)
Dmitri Vassilevich
(ABC Federal U.)
