2017
Lawrence E. Kidder, Scott E. Field, Francois Foucart, Erik Schnetter, Saul A. Teukolsky, Andy Bohn, Nils Deppe, Peter Diener, François Hébert, Jonas Lippuner, Jonah Miller, Christian D. Ott, Mark A. Scheel, and Trevor Vincent (2017):
SpECTRE: A Task-Based Discontinuous Galerkin Code for Relativistic Astrophysics, Journal of Computational Physics, Elsevier BV, Vol 335, pp84-114
2016
Luke F. Roberts, Christian D. Ott, Roland Haas, Evan P. O'Connor, Peter Diener, and Erik Schnetter (2016):
General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae, Astrophysical Journal, The American Astronomical Society, Vol 831, Num 1, pp98
2015
2014
Philipp Mösta, Sherwood Richers, Christian D. Ott, Roland Haas, Anthony L. Piro, Kristen Boydstun, Ernazar Abdikamalov, Christian Reisswig, and Erik Schnetter (2014):
Magnetorotational Core-Collapse Supernovae in Three Dimensions, Astrophysical Journal Letters, The American Astronomical Society, Vol 785, Num 2, ppL29
2013
2012
Marek Blazewicz, Steven R. Brandt, Peter Diener, David M. Koppelman, Krzysztof Kurowski, Frank Löffler, Erik Schnetter, and Jian Tao (2012):
A Massive Data Parallel Computational Framework for Petascale/Exascale Hybrid Computer Systems, IOS Press, Applications, Tools and Techniques on the Road to Exascale Computing (International Conference on Parallel Computing, ParCo 2011), Vol 22, pp351-58, Ghent, Belgium
A. Zebrowski, F. Löffler, and E. Schnetter (2012):
The BL-Octree: An Efficient Data Structure for Discretized Block-Based Adaptive Mesh Refinement, IOS Press, Applications, Tools and Techniques on the Road to Exascale Computing (International Conference on Parallel Computing, ParCo 2011), Vol 22, pp81-88, Ghent, Belgium
Frank Löffler, Joshua Faber, Eloisa Bentivegna, Tanja Bode, Peter Diener, Roland Haas, Ian Hinder, Bruno C Mundim, Christian D. Ott, Erik Schnetter, Gabrielle Allen, Manuela Campanelli, and Pablo Laguna (2012):
The Einstein Toolkit: A Community Computational Infrastructure for Relativistic Astrophysics, Classical and Quantum Gravity, IOP Publishing, Vol 29, Num 11, pp115001
2011
C. D. Ott, C. Reisswig, E. Schnetter, E. O'Connor, U. Sperhake, F. Löffler,, P. Diener, E. Abdikamalov, I. Hawke, and A. Burrows (2011):
Dynamics and Gravitational Wave Signature of Collapsar Formation, Physical Review Letters, American Physical Society, Vol 106, Num 16, pp161103
2010
Leonid Oliker, Jonathan Carter, Vincent Beckner, John Bell, Harvey Wasserman, Mark Adams, Stéphane Ethier, and Erik Schnetter (2010):
Large-Scale Numerical Simulations on High-End Computational Platforms, CRC Press, Performance Tuning of Scientific Applications, pp123-150
2018
Saul A. Teukolsky, Larry Kidder, Mark Scheel, Francois Foucart, Matt Duez, Harald Pfeiffer, Geoffrey Lovelace, Scott Field, Erik Schnetter, Peter Diener (2018):
Petascale Simulations of Merging Black Holes and Neutron Stars, 2018 Blue Waters Annual Report, pp48
Oct 1, 2014
The National Science Foundation (NSF) has awarded 14 new allocations on the Blue Waters petascale supercomputer at the National Center for Supercomputing Applications (NCSA) at the University of Illinois at Urbana-Champaign. Seven of the awards are for new projects.
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Jul 2, 2014
If you were to go back far enough into the Earth’s cosmic ancestry, you might be surprised to find it all started with a supernova explosion. These explosive cosmic events are like laboratories in space, generating elements that enable the creation of life later on; in fact, most of what makes up the Earth, including us humans, evolved from these fundamental elements. This is why simulating the process of a star going supernova is so important—it could potentially be the key to unlocking some of the bigger mysteries of how we came to be in the universe.
Philipp Mösta, postdoctoral scholar at Caltech, Christian D. Ott, professor of astrophysics at Caltech, and fellow researchers working with Peter Diener, research professor at the Center for Computation and Technology of Louisiana State University, are studying extreme core-collapse supernovae. These events make up only one percent of all supernovae that are observed but are the most extreme in terms of the energy emitted into the universe.
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