Award Abstract #0521566
Acquisition of Beowulf Cluster for a Center for Computational Astrophysics at the University of California, Santa Cruz
NSF Org: |
AST
Division of Astronomical Sciences
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Initial Amendment Date: |
September 16, 2005 |
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Latest Amendment Date: |
April 6, 2006 |
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Award Number: |
0521566 |
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Award Instrument: |
Continuing grant |
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Program Manager: |
Andrew Clegg
AST Division of Astronomical Sciences
MPS Directorate for Mathematical & Physical Sciences
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Start Date: |
September 15, 2005 |
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Expires: |
August 31, 2007 (Estimated) |
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Awarded Amount to Date: |
$1100000 |
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Investigator(s): |
Stanford Woosley woosley@ucolick.org (Principal Investigator)
Joel Primack (Co-Principal Investigator) Gary Glatzmaier (Co-Principal Investigator) Donald Gavel (Co-Principal Investigator) Pascale Garaud (Co-Principal Investigator)
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Sponsor: |
University of California-Santa Cruz
1156 High Street
SANTA CRUZ, CA 95064 831/459-5278
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NSF Program(s): |
ADVANCED TECHNOLOGIES & INSTRM
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Field Application(s): |
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Program Reference Code(s): |
OTHR, 1206, 0000
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Program Element Code(s): |
V969, 1218
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ABSTRACT
AST-0521566/Woosley, UCSC
This project will provide the necessary supercomputing resources to study roughly a dozen grand-challenge problems in astrophysics, planetary science, and telescope instrument design at the University of California, Santa Cruz (UCSC). Principal users would include approximately 25 graduate students and postdocs. The equipment proposed is a 280-node Beowulf Linux cluster having two AMD 246 64 bit processors per node. Each node will also have 4 Gbytes of memory and the overall machine will be served by 20 TB of disk storage in a fast RAID system. A variety of highly parallelized, production-ready codes will be fielded on this system to simulate cosmology, structure formation, supernovae, gamma-ray bursts, magnetohydrodynamics, planetary formation and structure, planetesimal collisions, and adaptive optics.
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