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Grand Challenge Problems in Computational Astrophysics

Workshop I: Astrophysical Fluid Dynamics

April 4 - 9, 2005

Schedule and Presentations

Program Poster PDF

Organizing Committee:

Richard Klein, Chair (University of California at Berkeley/Lawrence Livermore National Laboratory)
Willy Benz (University of Bern)
Phillip Colella (Lawrence Berkeley National Laboratory)
James McWilliams (UCLA)
Joseph Monaghan (Monash University, Australia)
Michael Norman (University of California at San Diego)
Robert Rosner (Univ. of Chicago)
Chi-Wang Shu (Brown University)
Jim Stone (Princeton University)
Marco Velli (University of Florence)

Scientific Background

The unifying theme of this workshop is the computational approach to astrophysical fluids, be they plasmas, neutral clouds, or some mix of the two. Emphasis will be placed on 1) the range of astrophysical applications appropriate to each computational technique, 2) the methodologies developed for including gravity, magnetic fields, radiation transport, dust, energy sinks and sources, and other physical processes, and 3) the algorithmic responses developed to avoid instabilities and unphysical dissipation in the computations. Topics to include:

  • hydrodynamics and magnetohydrodynamics.
    • accretion disk instabilities
    • jet formation
    • molecular cloud support
    • origin & growth of cosmic magnetic fields
    • evolution of galactic magnetic fields
    • planetary nebulae
    • astrophysical pair plasmas
  • multi-phase flows:
    • dust and gas in accretion disks & in radiatively-driven winds
  • turbulence, convection, chaos
  • evolution of molecular clouds
    • interstellar chemistry
    • turbulence
  • star formation
    • first generation
    • current star formation
    • star formation in high-pressure environments
    • multiple star and cluster formation
  • supernovae and novae
    • detonations, flame propagation
    • nuclear reaction networks
      • thermal pulses
      • r,s, and p processes
  • computational issues:
    • breakdown of the fluid approximation at small scales, low densities
    • comparisons of particle versus finite difference methodologies
    • advances in adaptive mesh refinement techniques
    • test cases for codes

Speakers

Matthew Bate (University of Exeter)
Mitchell Begelman (University of Colorado)
Axel Brandenburg (Nordita)
Greg Bryan (Columbia University)
Adam Burrows (University of Arizona)
Friedrich Busse (University of Bayreuth)
John Castor (Lawrence Livermore National Laboratory)
Roger Chevalier (University of Virginia)
Phillip Colella (Lawrence Berkeley National Laboratory)
Sam Falle (University of Leeds)
Robert Fisher (Lawrence Livermore National Laboratory)
Charles Gammie (University of Illinois)
John Hawley (University of Virginia)
Greg Howes (UCLA)
Richard Klein (University of California at Berkeley/Lawrence Livermore National Laboratory)
Philip Marcus (University of California at Berkeley)
Jose Marti (University of Valencia, Spain)
Chris McKee (University of California at Berkeley)
Joseph Monaghan (Monash University, Australia)
Michael Norman (University of California at San Diego)
Paolo Padoan (University of California at San Diego)
Alexei Poludnenko (University of Chicago)
Chi-Wang Shu (Brown University)
Jim Stone (Princeton University)
Juri Toomre (University of Colorado)
Gabor Toth (University of Michigan)
Marco Velli (University of Florence)
Markus Wetzstein (Ludwig-Maximilian-University, Munich)
Paul Woodward (University of Minnesota)

Registration

Online registration is closed for this workshop because we have reached capacity. You may still be able to register at the door on the day of the workshop but only on a space-available basis.

Contact Us:

Institute for Pure and Applied Mathematics (IPAM)
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Los Angeles CA 90095-7121
Phone: 310 825-4755
Fax: 310 825-4756
Email: ipam@ucla.edu
Website: http://www.ipam.ucla.edu/programs/pcaws1/


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