skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Rapid Optimal SPH Particle Distributions in Spherical Geometries For Creating Astrophysical Initial Conditions

Journal Article · · The Astrophysical Journal (Online)
 [1];  [1]
  1. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)

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.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC52-07NA27344
OSTI ID:
1438770
Report Number(s):
LLNL-JRNL-679768; TRN: US1900519
Journal Information:
The Astrophysical Journal (Online), Vol. 820, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 7 works
Citation information provided by
Web of Science

References (15)

Late‐Time Convection in the Collapse of a 23 M Star journal April 2007
Discreteness effects in simulations of hot/warm dark matter: Discreteness effects in HDM/WDM simulations journal August 2007
Collapse of a Molecular Cloud Core to Stellar Densities: The First Three-dimensional Calculations journal November 1998
An Alternative to Grids and Glasses: Quaquaversal Pre‐Initial Conditions for N ‐Body Simulations journal February 2007
Gamma‐Ray Lines from Asymmetric Supernovae journal September 2003
Smoothed Particle Hydrodynamics with particle splitting, applied to self-gravitating collapse journal February 2002
Stellar encounters involving neutron stars in globular cluster cores journal December 1992
Smoothed particle hydrodynamics: theory and application to non-spherical stars journal December 1977
Modeling Core-Collapse Supernovae in Three Dimensions journal July 2002
A numerical approach to the testing of the fission hypothesis journal December 1977
A simulation of the collapse and fragmentation of cooling molecular clouds journal July 1991
Stellar encounters involving red giants in globular cluster cores journal November 1991
Distributing many points on a sphere journal December 1997
Generating Optimal Initial Conditions for Smoothed Particle Hydrodynamics Simulations journal January 2015
The origin of the Moon and the single-impact hypothesis, II journal July 1987

Cited By (4)

Mass transfer in white dwarf–neutron star binaries journal February 2017
Planetary giant impacts: convergence of high-resolution simulations using efficient spherical initial conditions and swift journal June 2019
Consequences of Giant Impacts on Early Uranus for Rotation, Internal Structure, Debris, and Atmospheric Erosion journal July 2018
Consequences of Giant Impacts on Early Uranus for Rotation, Internal Structure, Debris, and Atmospheric Erosion text January 2018

Figures / Tables (8)