Fundamental differences between SPH and grid methods |
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| Authors: | Oscar Agertz,Ben Moore,Joachim Stadel,Doug Potter,Francesco Miniati,Justin Read,Lucio Mayer,Artur Gawryszczak,rey Kravtsov,Å ke Nordlund,Frazer Pearce,Vicent Quilis,Douglas Rudd,Volker Springel,James Stone,Elizabeth Tasker,Romain Teyssier,James Wadsley, Rolf Walder |
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| Affiliation: | Institute for Theoretical Physics, University of Zürich, CH-8057 Zürich, Switzerland;Department of Physics, Institute für Astronomie, ETH Zürich, CH-8093 Zürich, Switzerland;Nicolaus Copernicus Astronomical Centre, Bartycka 18, Warsaw PL-00-716, Poland;Department of Astronomy &Astrophysics, The University of Chicago, Chicago, IL 60637, USA;Niels Bohr Institute, Copenhagen University, Juliane Maries Vej 30, DK-2100 København Ø, Denmark;School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD;Departemento de Astronomia y Astrofisica, Universidad de Valencia, 46100 Burjasott, Valencia, Spain;Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85740 Garching, Germany;Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA;Department of Astronomy, Columbia University, New York, NY 10027, USA;Service d'Astrophysique, CEA/DSM/DAPNIA/SAp, Centre d'Etudes de Saclay, L'orme des Merisiers, 91191 Gif-sur-Yvette Cedex, France;Department of Physics and Astronomy, McMaster University, Hamilton, Ontario L88 4M1, Canada;Institute für Astronomie, ETH Zürich, CH-8092 Zürich, Switzerland |
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| Abstract: | |
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| Keywords: | hydrodynamics instabilities turbulence methods: numerical ISM: clouds galaxies: evolution galaxies: formation galaxies: general |
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