Rapid Optimal SPH Particle Distributions in Spherical Geometries For Creating Astrophysical Initial Conditions
Abstract
Creating spherical initial conditions in smoothed particle hydrodynamics simulations that are spherically conformal is a difficult task. Here in this paper, we describe two algorithmic methods for evenly distributing points on surfaces that when paired can be used to build three-dimensional spherical objects with optimal equipartition of volume between particles, commensurate with an arbitrary radial density function. We demonstrate the efficacy of our method against stretched lattice arrangements on the metrics of hydrodynamic stability, spherical conformity, and the harmonic power distribution of gravitational settling oscillations. We further demonstrate how our method is highly optimized for simulating multi-material spheres, such as planets with core–mantle boundaries.
- Authors:
-
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Publication Date:
- Research Org.:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1438770
- Report Number(s):
- LLNL-JRNL-679768
Journal ID: ISSN 1538-4357; TRN: US1900519
- Grant/Contract Number:
- AC52-07NA27344
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 820; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; 97 MATHEMATICS AND COMPUTING; methods: numerical; planets and satellites: terrestrial planets
Citation Formats
Raskin, Cody, and Owen, J. Michael. Rapid Optimal SPH Particle Distributions in Spherical Geometries For Creating Astrophysical Initial Conditions. United States: N. p., 2016.
Web. doi:10.3847/0004-637X/820/2/102.
Raskin, Cody, & Owen, J. Michael. Rapid Optimal SPH Particle Distributions in Spherical Geometries For Creating Astrophysical Initial Conditions. United States. https://doi.org/10.3847/0004-637X/820/2/102
Raskin, Cody, and Owen, J. Michael. Thu .
"Rapid Optimal SPH Particle Distributions in Spherical Geometries For Creating Astrophysical Initial Conditions". United States. https://doi.org/10.3847/0004-637X/820/2/102. https://www.osti.gov/servlets/purl/1438770.
@article{osti_1438770,
title = {Rapid Optimal SPH Particle Distributions in Spherical Geometries For Creating Astrophysical Initial Conditions},
author = {Raskin, Cody and Owen, J. Michael},
abstractNote = {Creating spherical initial conditions in smoothed particle hydrodynamics simulations that are spherically conformal is a difficult task. Here in this paper, we describe two algorithmic methods for evenly distributing points on surfaces that when paired can be used to build three-dimensional spherical objects with optimal equipartition of volume between particles, commensurate with an arbitrary radial density function. We demonstrate the efficacy of our method against stretched lattice arrangements on the metrics of hydrodynamic stability, spherical conformity, and the harmonic power distribution of gravitational settling oscillations. We further demonstrate how our method is highly optimized for simulating multi-material spheres, such as planets with core–mantle boundaries.},
doi = {10.3847/0004-637X/820/2/102},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 820,
place = {United States},
year = {Thu Mar 24 00:00:00 EDT 2016},
month = {Thu Mar 24 00:00:00 EDT 2016}
}
Web of Science
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