Oct. 28, 2022
While Lawrence Livermore is eagerly awaiting the arrival of its first exascale-class supercomputer, El Capitan, physicists and computer scientists running scientific applications on testbeds for the machine are getting a taste of what to expect.
“I’m not exactly sure we’ve wrapped our head around exactly about how much compute power [El Capitan] is going to have, because it is so much of a jump from what we have now,” said Brian Ryujin, a computer scientist in the Applications, Simulations, and Quality (ASQ) division of LLNL’s Computing directorate. “I’m very interested to see what our users will do with it, because this machine is going to be simply enormous.”
Ryujin is one of the LLNL researchers who are using the third generation of early access (EAS3) machines for El Capitan — Hewlett Packard Enterprise (HPE)/AMD systems with predecessor nodes to those that will make up El Capitan — to port codes over to the future exascale system. Despite being a mere fraction of the El Capitan’s size and containing earlier generation components, the EAS3 systems rzVernal, Tenaya and Tioga currently rank among the top 200 of the world’s most powerful supercomputers. All three contain HPE Cray EX235a accelerator blades with 3rd generation AMD EPYC 64-core CPUs and AMD Instinct MI250X accelerators, identical nodes to what comprises the Oak Ridge National Laboratory’s Frontier system that holds the No. 1 spot on the Top500 List and the title of the world’s first exascale system.
Lawrence Livermore scientists are scaling up the production of vertically aligned single-walled carbon nanotubes (SWCNT) that could revolutionize diverse commercial products ranging from rechargeable batteries, automotive parts and sporting goods to boat hulls and water filters.
Most CNT production today is used in bulk composite materials and thin films, which rely on unorganized CNT architectures. For many uses, organized CNT architectures such as vertically aligned forests provide important advantages for exploiting the properties of individual CNTs in macroscopic systems.
“Robust synthesis of vertically-aligned carbon nanotubes at large scale is required to accelerate deployment of numerous cutting-edge devices to emerging commercial applications," LLNL scientist Francesco Fornasiero said. “To address this need, we demonstrated that the structural characteristics of single-walled CNTs produced at wafer scale in a growth regime dominated by bulk diffusion of the gaseous carbon precursor are remarkably invariant over a broad range of process conditions.”
The goal of the Vera C. Rubin Observatory project is to conduct the 10-year Legacy Survey of Space and Time (LSST). LSST will deliver a 500-petabyte set of images and data products that will address some of the most pressing questions about the structure and evolution of the universe and the objects in it. Scientists will use the 3,200 megapixel camera to help understand the mystery of dark matter and dark energy.
LLNL scientists were instrumental in designing and building the lens. LLNL scientist and LSST project manager Vincent Riot said the camera will be able to generate data for dozens of generations and after a year or so it may take more images than all the images ever taken by other telescopes and cameras.
In new experiments, Lawrence Livermore scientists have emulated the conditions of Lonsdaleite, a diamond formation, using picosecond time scale laser compression and observed the transition with state-of-the-art materials characterization using femtosecond X-ray pulses. This graphite-diamond phase transition is of particular interest for fundamental reasons and a wide range of applications.
The observation of Lonsdaleite subsequent to shock compression has been a persistent mystery, including debate over whether hexagonal diamond exists as an extended structure, or is cubic diamond with defects. Previous studies of the phase transition of graphite to diamond or Lonsdaleite under moderate shock compression support a diffusionless mechanism for the phase transition, but these studies did not observe atomic structure through the transition, so the transformation mechanism was not revealed.
“Lonsdaleite is formed under rapid compression — unique to shock compression," said LLNL scientist Mike Armstrong. “There has been speculation for decades about the mechanisms and intermediate states of this phase transition and why it only forms under rapid compression. Here we show that the Lonsdaleite structure is likely an intermediate state in the phase transition to cubic diamond.”
A five-year microbial study of the International Space Station (ISS) and its astronauts by Lawrence Livermore National Laboratory (LLNL) and NASA researchers has found that the ISS habitat is safe for its residents.
The research effort represents the first comprehensive characterization of the space station’s environmental profile (or microbiome) and is the first to compare the ISS microbiome to an astronaut’s microbiome using metagenomic DNA sequencing techniques.
“Although our survey found several opportunistic microbes, we concluded that the ISS is a safe environment for the astronauts,” said LLNL biologist Crystal Jaing.
“We have found that the microbiome of the ISS surfaces is stable and that most of the microbiome is associated with human skin,” Jaing said.