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New software to support interest in extreme science

Date:
April 29, 2011
Source:
University of Chicago
Summary:
The University of Chicago's Flash Center for Computational Science has just released a major new version of supercomputer code, called FLASH 4-alpha. Based on previous software for simulating exploding stars, this is the first version of the FLASH code that has extensive capabilities for simulating high-energy density physics experiments.

The University of Chicago's Flash Center for Computational Science released a major new version of supercomputer code, called FLASH 4-alpha, on April 29. Based on previous software for simulating exploding stars, this is the first version of the FLASH code that has extensive capabilities for simulating high-energy density physics experiments.

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The U.S. Department of Energy's National Nuclear Security Administration Advanced Simulation and Computing Program has funded the addition of the new capabilities to this software, which will help scientists at universities across the nation better understand the fundamental properties of matter at high densities and high temperatures.

"The enhanced FLASH code is an open toolset for designing and analyzing experiments that address questions about the nature of planetary interiors, the creation of elements via nuclear processes, and how matter behaves in violent shocks and other extreme conditions," said Don Lamb, Flash Center director and the Robert A. Millikan Distinguished Service Professor in Astronomy & Astrophysics.

The code will support academic HEDP research at a variety of laboratories, including major national facilities such as the National Ignition Facility at Lawrence Livermore National Laboratory in California, the Z machine at Sandia National Laboratories in New Mexico and the Omega Laser Facility at the University of Rochester.

"These facilities use extremely powerful lasers or large amounts of electric current to generate conditions that allow scientists to investigate and address important issues in areas such as astrophysics, material science, planetary science and fusion energy," said Milad Fatenejad, a Flash Center research scientist. "Simulations play a vital role in demonstrating the viability of proposed experiments and analyzing experimental results. The enhanced FLASH code will be able to fill both of these roles."

The Flash Center is already using the new capabilities in FLASH to simulate radiative shock experiments conducted by the Center for Radiative Shock Hydrodynamics at the University of Michigan and at the Omega Laser Facility, said Fatenejad.

LLNL and other laboratories have developed highly capable codes for in-house research in HEDP, Lamb said. "Unlike FLASH, these codes were never designed with the academic community in mind," he said. "Having a workhorse open toolset for scientists at universities is absolutely essential, and until now has not existed."

The addition of new HEDP capabilities in the FLASH code has benefited from a collaboration the Flash Center has initiated with scientists at the universities of Michigan and Wisconsin, and at Los Alamos National Laboratory and Lawrence Livermore National Laboratory.


Story Source:

The above story is based on materials provided by University of Chicago. Note: Materials may be edited for content and length.


Cite This Page:

University of Chicago. "New software to support interest in extreme science." ScienceDaily. ScienceDaily, 29 April 2011. <www.sciencedaily.com/releases/2011/04/110429162926.htm>.
University of Chicago. (2011, April 29). New software to support interest in extreme science. ScienceDaily. Retrieved December 21, 2014 from www.sciencedaily.com/releases/2011/04/110429162926.htm
University of Chicago. "New software to support interest in extreme science." ScienceDaily. www.sciencedaily.com/releases/2011/04/110429162926.htm (accessed December 21, 2014).

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