In this talk I will explain how certain aspects of black-hole physics can be understood using ideas from effective field theory. Many of the familiar notions from particle physics will play a role, including the renormalization group, universality and naturalness. In particular, I will explain why black holes naively seem like fine-tuned systems, but they are ultimately not thanks to an accidental symmetry of General Relativity. The talk is based on work in collaboration with Alessandro Podo.
By Donato Bini
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By Marie-Anne Bizouard
By Alessandro Nagar
By Simon Maenaut
By Keefe Mitman
By Carlos Lousto
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By Manuela Campanelli
By Marc Henneaux
By Niels Warburton
By Sergiu Klainerman
By Rod Gover
By Jérémie Szeftel
