Statistical mechanics of self gravitating N body systems
by Scott Tremaine
at Physics Colloquium
Thu, 07 Jan 2016, 15:30
Physics building (#54) room 207
Abstract
There have been many attempts to apply the powerful tools of statistical mechanics to self gravitating N body systems such as star clusters galaxies and planetary systems I will describe why this is difficult some notable failures and successes and recent work on two arenas where these tools may offer new insight: the distribution of young stars in the central parsec of our Galaxy and the distribution of orbits of exoplanets Refreshments are served at 3:20pm
Created on 07-12-2015 by Bar Lev, Yevgeny (ybarlev)
Updaded on 07-12-2015 by Bar Lev, Yevgeny (ybarlev)