[Colloquium] Special Flash Center Seminar - Prof. Dave Arnett, Thursday 5/3 2:00 PM LASR

Ninfa Mayorga ninfa at ci.uchicago.edu
Thu May 3 13:37:08 CDT 2012


~Reminder~

The Flash Center for Computational Science
Department of Astronomy & Astrophysics
The University of Chicago

Special Seminar

David Arnett
Steward Observatory
University of Arizona
Stellar Turbulence, and why we should care


Supercomputers allow the simulation of three-dimensional highly turbulent flow. Treating these numerical "experiments" as valid representations of the behavior of high energy density (HED) plasma, a view supported by laboratory experiments with inertial confinement fusion (ICF) devices, we are beginning to develop a theory of this behavior appropriate to stellar interiors. Unlike conventional astrophysical convection theory, the Richardson-Kolmogorov turbulent cascade and the Lorenz strange attractor make an appearance, as well as a rich set of boundary-region physics. The process of developing physical insight from numerical simulations will be illustrated, and implications for stellar evolution, from the Sun to gamma-ray bursts and supernovae, will be discussed.

Thursday, May 3, 2012
2:00 pm

LASR Conference room

Host:  Don Lamb, Flash Center Director

Persons with a disability who may need assistance, please call Mila Kuntu, Flash Center Secretary, in advance at (773) 834-2057

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