Supernova Neutrinos, the Supernova Mechanism,
and Related Astrophysics
Working Group Session
September 21, 2000
The Supernova Mechanism and TeraScale Simulation
1:45-1:55: Arnett, Frontiers in Massive Star Evolution
1:55-2:05: Swesty, Multi-D Neutrino Transport
2:05-2:15: Blondin, Multi-D MHD
2:15-2:25: Matzner, Multi-D GR/LIGO
Supernova Nuclear Weak Interaction Physics
2:25-2:35: Dean, TeraScale Nuclear Structure Computation
2:35-2:45: McLaughlin, Neutrino-Nucleus Cross Sections
2:45-2:55: Reddy, High-Density Neutrino Opacities
2:55-3:30: Discussion of future possibilities, priorities
September 22
Primordial and Supernova/Neutron-Star-Merger Nucleosynthesis
2:15-2:25: Hogan, Light-Element Abundances in Primordial Nucleosynthesis
2:25-2:35: Meyer, Heavy-Element Nucleosynthesis
2:35-2:45: Qian, r-Process Nucleosynthesis and Galactic Chemical Evolution
2:45-2:55: Cardall, Neutrino Masses and Mixing-The Bridge Between Cosmology and Supernovae
Supernova Neutrino Detection (Theory):
2:55-3:05: Bruenn, Neutrino Signatures
3:05-3:15: Beacom, New Possibilities and Needs
Supernova Neutrino Detection
3:15 -3:25: Wildenhain, Chlorine and Iodine
3:25-3:35: Vogel, KamLand
3:35-3:45: Elliott, Lead Perchlorate
3:45 -3:55: Boyd, OMNIS
Break
4:30-4:40: Heise, SNO
4:40-4:50: Vagins, SuperKamiokande
4:50-6:15: Discussion of future possibilities, priorities
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