Tensor classification of structure in smoothed particle hydrodynamics density fields
Duncan Forgan, Ian Bonnell, William Lucas, Ken Rice

TL;DR
This paper introduces tensor classification as an effective, parameter-free method for identifying complex structures in smoothed particle hydrodynamics density fields, enhancing analysis of astrophysical simulations.
Contribution
It demonstrates tensor classification's ability to detect diverse structures in SPH simulations without free parameters, using native smoothing and multiple tensors.
Findings
Successfully identifies filaments, shells, and sheets in molecular cloud simulations.
Detects spiral arms in galactic discs.
Shows how different tensors reveal physical process interactions.
Abstract
As hydrodynamic simulations increase in scale and resolution, identifying structures with non-trivial geometries or regions of general interest becomes increasingly challenging. There is a growing need for algorithms that identify a variety of different features in a simulation without requiring a "by-eye" search. We present tensor classification as such a technique for smoothed particle hydrodynamics (SPH). These methods have already been used to great effect in N-Body cosmological simulations, which require smoothing defined as an input free parameter. We show that tensor classification successfully identifies a wide range of structures in SPH density fields using its native smoothing, removing a free parameter from the analysis and preventing the need for tesselation of the density field, as required by some classification algorithms. As examples, we show that tensor classification…
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