2006 APS April Meeting
Saturday–Tuesday, April 22–25, 2006;
Dallas, TX
Session Q1: Neutrinos I
1:30 PM–3:18 PM,
Monday, April 24, 2006
Hyatt Regency Dallas
Room: Landmark A
Sponsoring
Units:
DAP DPF
Chair: George Fuller, University of California, San Diego
Abstract ID: BAPS.2006.APR.Q1.2
Abstract: Q1.00002 : Neutrinos and Neutrino Physics: Still Center Stage in Core Collapse Supernovae
2:06 PM–2:42 PM
Preview Abstract
Abstract
Author:
Anthony Mezzacappa
(Oak Ridge National Laboratory)
Ascertaining the core collapse supernova mechanism and understanding all of
the phenomena associated with such stellar explosions, such as their element
synthesis and gravitational wave signatures, neutron star kicks, the spin of
pulsars at birth, etc., will require three-dimensional precision models that
include realistic neutrino transport, stellar core fluid instabilities,
rotation, magnetic fields, a realistic stellar core equation of state for
both sub- and super-nuclear densities, and realistic weak interactions. Only
in the last decade has supernova modeling broken free from the confines of
spherical symmetry. I will review the current state of the art. Even the
most fundamental questions remain: How do core collapse supernovae explode?
What role do the neutrinos play? While a recent emphasis has been placed on
the role of magnetic fields in generating core collapse supernova
explosions, the neutrinos still occupy center stage. Moreover, in light of
the now experimentally determined fact that neutrinos have mass, neutrino
transport in core collapse supernovae takes on a whole new complexity.
Previously, neutrino transport was well described by Boltzmann kinetic
theory, but now more faithful modeling will require quantum kinetics. The
role of neutrino mixing in the core collapse supernova mechanism remains
virtually unexplored, with the potential for significant surprises. It is,
as I will discuss, one of the frontiers in core collapse supernova theory.
Finally, the development of precision three-dimensional supernova models
will provide yet another scientific opportunity beyond the chance to
ascertain how stars die and produce the elements necessary for life.
Together with detailed observations, especially of the neutrino and
gravitational wave emissions in the event of a Galactic supernova, detailed
supernova models will allow us to use core collapse supernovae as
laboratories for fundamental physics. I will discuss some of the
possibilities.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2006.APR.Q1.2