Physics Colloquium

Core Collapse Supernovae and their Nucleosynthesis

Dr. Raph Hix, UT Department of Physics/ORNL

Core-collapse supernovae, the culmination of massive stellar evolution, are among the brightest and most powerful explosions in the universe and are the principle actors in the story of our elemental origins. Our developing paradigm for the initiation of a core-collapse supernova reveals a supernova shock that stalls for hundreds of milliseconds before reviving. Though brought back to life by neutrino heating, the development of the supernova is inextricably linked to three dimensional fluid flows, with large scale hydrodynamic instabilities allowing successful explosions that spherical symmetry would prevent. Unfortunately, our understanding of the nucleosynthesis that occurs in these explosions, and their impact on galactic chemical evolution, is based on spherically symmetric simulations with parameterized explosions, ignoring much that we have learned about the central engine of these supernovae over the past two decades. I will present recent results from two and three dimensional simulations of core-collapse supernovae using the CHIMERA code and discuss how the multi-dimensional character of the explosions directly impacts the nucleosynthesis and other observables of core-collapse supernovae.

Monday, 10 March, 2014


Department of Physics and Astronomy

Phone: 974-3342
Website: Click to Visit



The Science and Engineering Research Facility

1414 Circle Drive
Room 307
Knoxville, TN USA
See all events at this location

Contribute to big ideas. Give to UT.

The University of Tennessee, Knoxville. Big Orange. Big Ideas.

The University of Tennessee, Knoxville. Knoxville, Tennessee 37996 | 865-974-1000

The flagship campus of the University of Tennessee System and partner in the Tennessee Transfer Pathway.