Petascale Core-Collapse Supernova Simulation

Event Sponsor: 
Argonne Leadership Computing Facility
Start Date: 
Jan 22 2010 - 3:00pm to 4:00pm
Building/Room: 
Building 240 / Conference Center Room 1404
Location: 
Argonne National Labortory
Speaker(s): 
Dr. Bronson Messer
Speaker(s) Title: 
Deputy Group Lead, Scientific Computing, Oak Ridge Leadership Computing Facility
Host: 

The advent of petascale computing brings with it the promise of substantial increases in physical fidelity for a host of scientific problems. However, the realities of computing on these resources are daunting, and the architectural features of petascale machines often require considerable innovation for effective use. Nevertheless, there exists a class of scientific problems whose ultimate answer requires the application of petascale (and beyond) computing. One example is ascertaining the core-collapse supernova mechanism and explaining the rich phenomenology associated with these events. These stellar explosions produce and disseminate a dominant fraction of the elements in the Universe; are prodigious sources of neutrinos, gravitational waves, and photons across the electromagnetic spectrum; and lead to the formation of neutron stars and black holes. I will describe our recent multidimensional supernova simulations performed on petascale platforms fielded by the DOE Office of Science and the National Science Foundation.

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