, Johns Hopkins University
[Host: Alexander Saffer]
I will show how to derive analytic gravitational waveforms associated to the coalescence of a “hairy” black hole binary in Einstein-scalar-Gauss-Bonnet gravity (ESGB). I will present the ESGB post-Newtonian (PN) Lagrangian and gravitational wave fluxes. The PN framework relies on reducing the black holes to point particles with scalar-field-dependent masses. In light of the first law of thermodynamics of ESGB black holes, I will show that this procedure amounts to fixing their Wald entropies. As a consequence, inspiraling ESGB black holes can grow scalar “hair” until they turn into naked singularities. I will then extend the scope of the PN approximation to the strong field regime near merger by generalizing the Effective-One-Body (EOB) formalism to ESGB gravity.
Monday, October 18, 2021
Online, Room via Zoom
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Meeting ID: 983 6836 9604 Passcode: 130144
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