Talk detail

MG13 - Talk detail

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 Participant

Laguna, Pablo

Institution

Georgia Tech  - 837 State Street - Atlanta - Georgia - USA

Session

AN4

Accepted

Order

Time

Talk

Oral abstract

Title

Binary Black Holes in Astrophysical Environments
Co-authors

Abstract

Modeling the late inspiral and merger of supermassive black holes is central to understanding accretion processes and the conditions under which electromagnetic emission accompanies gravitational waves. In this regime, magneto-hydrodynamic numerical relativity simulations are needed to investigate how electromagnetic signatures correlate with black hole spins, mass ratios, and the gaseous environment in this final phase of binary evolution. I will review the current status of simulations that address binary black holes in hot accretion flows and circumbinary disks.

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