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SNSPH: A Parallel 3-D Smoothed Particle Radiation Hydrodynamics Code

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arxiv astro-ph/0512532 v1 pith:YKWGN53T submitted 2005-12-21 astro-ph

C.L. Fryer , G. Rockefeller , & M.S. Warren This is my paper · ORCID
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keywords codehydrodynamicsparallelparticleradiationsnsphaspectsbelieve
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We provide a description of the SNSPH code--a parallel 3-dimensional radiation hydrodynamics code implementing treecode gravity, smooth particle hydrodynamics, and flux-limited diffusion transport schemes. We provide descriptions of the physics and parallelization techniques for this code. We present performance results on a suite of code tests (both standard and new), showing the versatility of such a code, but focusing on what we believe are important aspects of modeling core-collapse supernovae.

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Cited by 1 Pith paper

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  1. On the formation of strange quark stars from supernova in compact binaries

    astro-ph.HE 2025-07 conditional novelty 6.0 of 10

    In a binary containing a neutron star and an exploding star, hypercritical accretion can push neutron stars past the density threshold for quark deconfinement, forming strange quark stars.

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