PIRSA:11110132

Tidal deformations of a Schwarzschild black hole via effective field theory approach.

APA

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

MLA

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

BibTex

          @misc{ pirsa_11110132,
            doi = {},
            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.