• Develop a standard model of core collapse supernovae
    • 3D
    • Accurate multigroup neutrino transport
    • Realistic nuclear and weak interaction physics
    • General Relativity
 
 
 
 
  • Scalable 3D, multigroup neutrino transport
  • 3D MHD
  • Realistic nuclear structure models for stellar nuclei
  • Better understanding of physics at high densities
  • High-density equation of state
  • Neutrino opacities, emissivities in nuclear matter
  • Neutrino transport and mixing in nuclear matter
 
 
 
 

Scalable algorithms for solution of large, sparse linear systems and large eigenvalue problems

Collaborative visualization and steering.


Requires an interdisciplinary team effort: astrophysicists, nuclear physicists, applied mathematicians, computer scientists