CORDIS Project
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This project investigates the interactions between super-massive black hole binaries and their surrounding gas in merging galaxies. By using advanced simulations, it aims to develop models that explain the evolution of these binaries and their implications for gravitational wave observations.
Nearly all galaxies in the universe harbor a super-massive black hole (SMBH)---with mass a million to a billion times that of our sun---in their core.
When these galaxies merge, their super-massive black holes are brought together to form a super-massive black hole binary that interacts with the newly forming galaxy's stars and gas. A cosmic population of these super-massive binaries is hypothesized as the source for the gravitational wave background (GWB) detected for the first time this June.…
KOBENHAVNS UNIVERSITET
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