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Riccardo Penco (Carnegie Mellon University)

Date: Tue. February 12th, 2019, 11:30 am-12:30 pm
Location: Foldy Room

Constraining the gravitational sector with black hole perturbations

In this talk, I will introduce an effective field theory (EFT) for perturbations around spherically symmetric spacetimes with a non-trivial scalar field profile. I will then apply this framework to study quasi-normal modes of static black holes with a scalar hair. Assuming that the deviation of the background from Schwarzschild is small, I will use a WKB approximation to introduce the notion of “light ring expansion”. This approximation is analogous to the slow-roll expansion used for inflation, and it allows us to express the quasinormal mode spectrum in terms of a small number of model-independent parameters to be constrained by observations. This is the first step towards an EFT framework for placing model-independent constraints on the gravitational sector based on the ringdown phase of LIGO events.

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