A Generalized Solution for Parallelized Computation of the Three-dimensional Gravitational Potential on a Multipatch Grid in Spherical Geometry
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[1] E. Wigner. Gruppentheorie und ihre Anwendung auf die Quantenmechanik der Atomspektren , 1931 .
[2] K. V. Roberts,et al. The optimization of particle calculations in 2 and 3 dimensions , 1969 .
[3] Donald Ervin Knuth,et al. The Art of Computer Programming, 2nd Ed. (Addison-Wesley Series in Computer Science and Information , 1978 .
[4] J. Jernigan. Direct N-body simulations with a recursive center of mass reduction and regularization , 1985 .
[5] Andrew W. Appel,et al. An Efficient Program for Many-Body Simulation , 1983 .
[6] Piet Hut,et al. A hierarchical O(N log N) force-calculation algorithm , 1986, Nature.
[7] L. Hernquist,et al. TREESPH: A Unification of SPH with the Hierarchical Tree Method , 1989 .
[8] E. Steinmetz. Simulating self-gravitating hydrodynamic flows , 1994, astro-ph/9402070.
[9] P. Paolucci,et al. The “Cubed Sphere” , 1996 .
[10] B. Fryxell,et al. FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes , 2000 .
[11] H. Janka,et al. Radiation hydrodynamics with neutrinos - Variable Eddington factor method for core-collapse supernova simulations , 2002, astro-ph/0203101.
[12] Rajeev Thakur,et al. Optimization of Collective Communication Operations in MPICH , 2005, Int. J. High Perform. Comput. Appl..
[13] P. Ricker. A Direct Multigrid Poisson Solver for Oct-Tree Adaptive Meshes , 2007, 0710.4397.
[14] Andrew Siegel,et al. Extensible component-based architecture for FLASH, a massively parallel, multiphysics simulation code , 2009, Parallel Comput..
[15] E. Muller,et al. An axis-free overset grid in spherical polar coordinates for simulating 3D self-gravitating flows , 2010, 1003.1633.
[16] E. Wes Bethel,et al. High Performance Visualization - Enabling Extreme-Scale Scientific Insight , 2012, High Performance Visualization.
[17] C. Graziani,et al. AN IMPROVED MULTIPOLE APPROXIMATION FOR SELF-GRAVITY AND ITS IMPORTANCE FOR CORE-COLLAPSE SUPERNOVA SIMULATIONS , 2013, 1307.3135.
[18] O. E. Bronson Messer,et al. THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVA SIMULATED USING A 15 M⊙ PROGENITOR , 2015, 1505.05110.
[19] H. Janka,et al. NEUTRINO-DRIVEN SUPERNOVA OF A LOW-MASS IRON-CORE PROGENITOR BOOSTED BY THREE-DIMENSIONAL TURBULENT CONVECTION , 2015, 1501.01961.
[20] E. Muller,et al. APSARA: A multi-dimensional unsplit fourth-order explicit Eulerian hydrodynamics code for arbitrary curvilinear grids , 2016, 1607.04272.
[21] H. Janka,et al. Production and Distribution of 44Ti and 56Ni in a Three-dimensional Supernova Model Resembling Cassiopeia A , 2016, 1610.05643.
[22] H. Janka,et al. Parallelized Solution Method of the Three-dimensional Gravitational Potential on the Yin–Yang Grid , 2018, The Astrophysical Journal.
[23] H. Janka,et al. Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition , 2017, 1708.04154.
[24] D. Radice,et al. A successful 3D core-collapse supernova explosion model , 2018, Monthly Notices of the Royal Astronomical Society.
[25] Stefanie Walch,et al. Tree-based solvers for adaptive mesh refinement code FLASH - I: gravity and optical depths , 2017, 1708.06142.
[26] M. Obergaulinger,et al. Three-dimensional Core-collapse Supernova Simulations with Multidimensional Neutrino Transport Compared to the Ray-by-ray-plus Approximation , 2018, The Astrophysical Journal.
[27] B. Müller,et al. An FFT-based Solution Method for the Poisson Equation on 3D Spherical Polar Grids , 2018, The Astrophysical Journal.