University of Cambridge > Talks.cam > DAMTP Astro Lunch > Dynamical evolution of binary supermassive black holes

Dynamical evolution of binary supermassive black holes

Add to your list(s) Download to your calendar using vCal

If you have a question about this talk, please contact Dr. Yufeng Lin.

Room changed

I review the life cycle of supermassive black hole binaries, focusing on their gravitational interactions with stars in the galactic nucleus, which produce many interesting astrophysical phenomena: tidal disruptions, ejection of hypervelocity stars, formation of galactic cores, and of course, the shrinking and eventual coalescence of the binary itself. I describe the challenges in modelling these systems with conventional N-body codes, and present an alternative Monte Carlo approach that overcomes these difficulties.

This talk is part of the DAMTP Astro Lunch series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

© 2006-2024 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity