Astronomy Colloquium
Cahill, Hameetman Auditorium
Turbulence, Computers and Stars
David Arnett,
Kavli Institute for Theoretical Physics, UCSB, Steward Observatory, University of Arizona,
It is now feasible to numerically simulate moderately turbulent flow in the stellar context. The impact of such simulations on astrophysical theory will be illustrated, as well as a connection to deterministic chaos. There have been a number of surprises, whose implications are only beginning to be appreciated. Applications to solar abundances and helioseismology, and to gravitational collapse and supernovae will be stressed.
For more information, please contact Gina Armas by phone at 4671 or by email at [email protected] or visit http://www.astro.caltech.edu/~gma/colloquia.html.
Event Series
Astronomy Colloquium Series