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LOCATION:HG F 30
DTSTART;TZID=Europe/Stockholm:20190614T103000
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UID:submissions.pasc-conference.org_PASC19_sess122@linklings.com
SUMMARY:MS39 - Breaking the Wall in Computational Astrophysics: Current Bo
 ttlenecks and How to Address them towards the Exascale Era
DESCRIPTION:Minisymposium\nComputer Science and Applied Mathematics, Physi
 cs\n\nThe Euclid Flagship Simulations\n\nStadel, Potter\n\nUpcoming large 
 scale structure surveys such as Euclid, DES, LSST, WFIRST will measur
 e the result of billions of years of evolution from the small linear fluct
 uations observed in the Cosmic Microwave Background (CMB). On the ver
 y largest scales these fluctuations are still evolving linearly...\n\n----
 -----------------\nGPU-Accelerated Neutrino Transport Solver for Multi-Dim
 ensional Core-Collapse Supernovae\n\nPan\n\nSelf-consistent core-collapse 
 supernova simulations require lots of input physics to explore the explosi
 on mechanism and to predict the multi-messenger signals for future observa
 tions, including multi-dimensional hydrodynamics, neutrino radiation trans
 port, microphysics, and general relativity.&nbsp...\n\n-------------------
 --\nSPH-EXA: A Smoothed Particle Hydrodynamics Miniapp for Exascale Comput
 ing\n\nCiorba, Cavelan, Guerrera, Cabezon\n\nWe present the roadmap a
 nd developments of SPH-EXA, a miniapp designed to perform parallel Smoothe
 d Particles Hydrodynamics (SPH) simulations that scale and exploit the com
 putational power of existing and up and coming supercomputers. The SPH-EXA
  miniapp is a self-contained C++ software package...\n\n------------------
 ---\nComputational Challenges in Lagrangian Simulations of Magnetised Astr
 ophysical Fluids\n\nMayer, Deng\n\nMagnetohydrodynamical instabilities pla
 y an important role in a variety of astrophysical flows. In astrophysical 
 disks they are occurring along with other complex processes, often in the 
 presence of self-gravity, radiation and supersonic conditions. Lagrangian 
 codes are very well suited to treat the...\n
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