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_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}} }
Hebrew University of Jerusalem
Talk Type
Subject
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.