Success Stories

Back to Success Stories Nucleon Structure Using Lattice QCD Simulation with Physical Pion Mass The goal of this project is to understand the properties of elementary particles such as the proton, which forms most of

Back to Success Stories Supercharged Supercapacitors Nanoporous carbon is being used to create a new generation of supercapacitors that have greatly improved capacitance compared to their precursors, with little effect on charging time. Professor Mathieu

Back to Success Stories Numerical Simulations to Explain the Intensity of Star Formation Understanding the origins of our universe is the foundation to understanding its future. Professor Frederic Bournaud and his international team of collaborators

Back to Success Stories Pair-Dominated Plasmas and Radiation in Ultra Intense Fields Leveraging the petascale computing power of SuperMUC, an international team of researchers performed 2D/3D simulations of laser absorption in dense electron-positron plasmas self-consitently

Back to Success Stories The virtual laboratory Supercomputers can be used to simulate materials at vastly diverse scales, from the flow of air past an aeroplane’s wing down to the movement of electrons around individual

Back to Success Stories PRACE help researchers calculate mass difference between neutrons and protons With the help of PRACE HPC resources, a team of physicists from France, Germany, and Hungary headed by Zoltán Fodor, a

Back to Success Stories Working with PRACE: An insider’s perspective Professor Stephan Roche of the Catalan Institute of Technology in Spain is currently working on his project Longitudinal and Transverse Electronic Transport in Atomically Doped

Back to Success Stories Looking beyond the Standard Model PRACE awarded millions of core hours on three of Europe’s most powerful supercomputers (17.5 million on JUQUEEN (JSC@GCS); 7.5 million on FERMI (CINECA); 5 million on

Back to Success Stories Simulating activity on the Sun with large plasma models The SunFlare project group has studied the relationship between the sub-surface layers and visible layers of the Sun, with a focus on