As a guest user you are not logged in or recognized by your IP address. You have
access to the Front Matter, Abstracts, Author Index, Subject Index and the full
text of Open Access publications.
Modeling thermonuclear supernovae is a premier application for leadership-class supercomputers and requires multi-physics simulation codes to capture hydrodynamics, nuclear burning, gravitational forces, etc. As a nuclear detonation burns through the stellar material, it also increases the temperature. An equation of state (EOS) is then required to determine, for example, the new pressure associated with this temperature increase. In fact, an EOS is needed after thermodynamic conditions are changed by any physics routines. This means it is called many times throughout a simulation, requiring the need for a fast EOS implementation. Fortunately, these calculations can be performed independently during each time step, so the work can be offloaded to GPUs. Using results from the IBM/NVIDIA early test system (Summitdev, a precursor to the upcoming Summit supercomputer) at Oak Ridge National Laboratory, we describe a hybrid OpenMP implementation with offloaded work to GPUs. We compare performance results between the two implementations, with a discussion of some of the currently available features of OpenACC and OpenMP 4.5.
This website uses cookies
We use cookies to provide you with the best possible experience. They also allow us to analyze user behavior in order to constantly improve the website for you. Info about the privacy policy of IOS Press.
This website uses cookies
We use cookies to provide you with the best possible experience. They also allow us to analyze user behavior in order to constantly improve the website for you. Info about the privacy policy of IOS Press.