CRA Seminar: Vasilis Paschalidis (U. of Arizona)
Bogg 1-44 VizLabTitle: Magnetohydrodynamic accretion onto binary black holes as a source for multimessenger astronomy with gravitational waves Abstract: Supermassive black hole binaries can form in magnetized plasma following galaxy mergers, via bar-mode instability in rapidly rotating supermassive stars, or by other dynamical processes. After formation, a combination of dynamical friction and gas-driven migration is likely to … Continue reading "CRA Seminar: Vasilis Paschalidis (U. of Arizona)"