PIRSA:11110132 Conference Cosmology

DOI10.48660/11110132

Conference/School: Effective Field Theory and Gravitational Physics Conference - 2011

Smolkin, M. (2011). Tidal deformations of a Schwarzschild black hole via effective field theory approach.. Perimeter Institute. https://pirsa.org/11110132

Smolkin, Misha. Tidal deformations of a Schwarzschild black hole via effective field theory approach.. Perimeter Institute, Nov. 28, 2011, https://pirsa.org/11110132 

@misc{ pirsa_PIRSA:11110132,
  doi = {10.48660/11110132},
  url = {https://pirsa.org/11110132},
  author = {Smolkin, Misha},
  keywords = {Cosmology},
  language = {en},
  title = {Tidal deformations of a Schwarzschild black hole via effective field theory approach.},
  publisher = {Perimeter Institute},
  year = {2011},
  month = {nov},
  note = {PIRSA:11110132 see, \url{https://pirsa.org}}
}

Abstract

In my talk I will discuss the static subsector of the black hole effective action in an arbitrary dimension. In particular, the derivation of the induced mass multipoles as a result of an external (static) gravitational field will be elucidated. In 4d these constants vanish, however in general they are non-vanishing in higher dimensions. Moreover, in certain cases they exhibit a (classical) renormalization group flow consistent with the divergences of the effective field theory.

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