CORDIS Project
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This project develops a comprehensive framework to understand how binary black holes form and merge in active galactic nuclei disks. It combines numerical and analytical methods to analyze the dynamics of black hole interactions, aiming to provide predictions that can be tested with gravitational wave data.
The growing list of binary black hole (BBH) mergers detected in gravitational waves (GWs) by LIGO/Virgo, have been used to put tight constraints on Einstein's Theory of Gravity.
However, their astrophysical origin still remains a major open question.
Recently, active galactic nuclei (AGN) disks have been suggested to be a promising location for forming BBH mergers.
In such environments, black holes (BHs) either form in the disk or are captured through gas-drag from the surrounding nuclear star c…
KOBENHAVNS UNIVERSITET
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