A team led by Argonne National Laboratory used the recently developed Hardware/Hybrid Accelerated Cosmology Codes ( HACC ) framework to achieve nearly 14 petaflops on the 20-petaflop Sequoia, an IBM BlueGene/Q supercomputer, in a record-setting benchmark run with 3.6 trillion simulation particles. HACC provides cosmologists the ability to simulate entire survey-sized volumes of the universe at a high resolution, with the ability to track billions of individual galaxies.
Simulations of this kind are required by the next generation of cosmological surveys to help elucidate the nature of dark energy and dark matter. The HACC framework is designed for extreme performance in the weak scaling limit ( high levels of memory utilization ) by integrating innovative algorithms, as well as programming paradigms, in a way that easily adapts to different computer architectures. The HACC team is now conducting a fully-instrumented science run with more than a trillion particles on Argonne’s 10-petaflop Mira system, also an IBM BlueGene/Q system.
“The performance of these applications on Mira and Sequoia provides an early glimpse of the transformational science these machines make possible — science important to DOE missions,” said Barbara Helland, of DOE’s Office of Science. “By pushing the state-of-the-art, these two teams of scientists are advancing science and also the know-how to use these new resources to produce insight and discovery.”
LLNL, in collaboration with scientists at IBM Research, created a new simulation capability called Cardioid to realistically and rapidly model a beating human heart at near-cellular resolution. The highly scalable code models in exquisite detail the electrophysiology of the human heart, including activation of heart muscle cells and cell-to-cell electrical coupling. Developed to run with high efficiency in the extreme strong-scaling limit, the scientists were able to achieve a performance of nearly 12 petaflops on Sequoia, and demonstrated the ability to model a highly resolved whole heart beating in very nearly real time ( 67.2 seconds of wall-clock time to model 60 seconds of real time ). Using Cardioid, the team performed groundbreaking simulations demonstrating for the first time in a simulation of a whole heart the generation of a reentrant activation pattern that often leads to a kind of arrhythmia known as Torsades de Pointes, which can result in sudden cardiac death. The potential to elucidate detailed mechanisms of arrhythmia will have impact on a multitude of applications in medicine, pharmaceuticals and implantable devices.
“A vital DOE/NNSA mission is to push the state-of-the-art in high performance computing to not only ensure the nation’s security but its technological and economic competitiveness,” said NNSA Advanced Simulation and Computing Director Bob Meisner. “Sequoia and Mira are powerful computational engines that allow our skilled teams to run applications such as Cardioid and HACC at very high levels of performance. What we learn from these early science applications will inform a broad range of scientific computing including our national security applications.”
Sequoia at Livermore and Mira at Argonne represent the third generation of IBM Blue Gene supercomputers. Sequoia, second on the TOP500 list with 98,304 nodes ( 1.57 million central processing units ), and Mira, fourth on the list with 49,152 nodes ( 786,432 central processing units ), allow execution of massive calculations in parallel. Both teams took full advantage of the five levels of parallelism available in the hardware to achieve sustained performance levels of 58.8 percent for Cardioid and an astounding 69.2 percent for HACC of the theoretical peak performance of the machine, as well as near perfect scaling. Strong scaling measures the ability to speed up a problem by using more processors, so that a given simulation finishes in one-hundredth of the time by using 100 times as many processors. Weak scaling measures the ability to increase the size of problem by using more processors, so that in a given time, a simulation 100 times larger is executed by using 100 times as many processors.
DOE’s Office of Science is the single largest supporter of basic research in the physical sciences in the U.S. and is working to address some of the most pressing challenges of our time. For more information, see science.energy.gov.
About the NNSA
Established by Congress in 2000, NNSA is a semi-autonomous agency within the U.S. Department of Energy responsible for enhancing national security through the military application of nuclear science. NNSA maintains and enhances the safety, security, reliability and performance of the U.S. nuclear weapons stockpile without nuclear testing; works to reduce global danger from weapons of mass destruction; provides the U.S. Navy with safe and effective nuclear propulsion; and responds to nuclear and radiological emergencies in the U.S. and abroad.
Argonne National Laboratory seeks solutions to pressing national problems in science and technology. The nations first national laboratory, Argonne conducts leading-edge basic and applied scientific research in virtually every scientific discipline. Argonne researchers work closely with researchers from hundreds of companies, universities, and federal, state and municipal agencies to help them solve their specific problems, advance Americas scientific leadership and prepare the nation for a better future. With employees from more than 60 nations, Argonne is managed by UChicago Argonne, LLC for the U.S. Department of Energys Office of Science
Information Source: Media Newswire