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.
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.
“We are very excited about the science these new capabilities will make possible,” said Flash Center associate director Anshu Dubey. “The Center has been able to add HEDP capabilities to the FLASH code and make it run efficiently on the next generation of computers thanks to a decade of funding by the DOE NNSA ASC Academic Strategic Alliance Program and recent funding by the DOE Office of Advanced Scientific Computing Research, as well as access to the world’s fastest computers through the NNSA ASC Program and the Office of Science INCITE Program.”
The new software is a collaboration between the Center, the University’s Computation Institute and Argonne National Laboratory. DOE funding for the initiative is through the Argonne Institute for Computing in Science.
More than 700 scientists worldwide have used FLASH code, and they have published more than 400 papers reporting results based on its use. Although most of these scientists have used FLASH for astrophysical research, others have modified it for simulating atmospheric physics and biological processes. IBM, NVIDIA and other companies have also licensed FLASH to test and develop hardware and software.
—Prof. Jacqueline Stewart
