University of Cambridge > > DAMTP Friday GR Seminar > Signatures of Modified Gravity in Black Hole Quasinormal Modes

Signatures of Modified Gravity in Black Hole Quasinormal Modes

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I will describe how signatures of modified gravity, in particular scalar tensor theories of gravity, can arise when studying black hole quasinormal modes. In particular I will look at black holes both with and without hair in Horndeski gravity, and discuss how we might constrain fundamental parameters of Horndeski theory through black hole spectroscopy.

This talk is part of the DAMTP Friday GR Seminar series.

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