Phase-space Delaunay tessellation field estimator

ABSTRACT The reconstruction of density and velocity fields is of central importance to the interpretation of N-body simulations. We propose a phase-space extension of the Delaunay tessellation field estimator (DTFE) that uses the mapping from Lagrangian to Eulerian space to track the dark matter fluid in phase-space. The new reconstruction scheme removes several artefacts from the conventional DTFE in multistream regions, while preserving the adaptive resolution in high-density regions and yielding continuous fields. The estimator also removes some tessellation artifacts of a previously proposed phase-space reconstruction scheme. The method is particularly suitable to the estimation of density and velocity fields of N-body simulations with multiple particle species and/or starting with glass initial conditions.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-12-03
DOI
https://doi.org/10.1093/mnras/stae2627
Citations
4
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
1.33

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article

Phase-space Delaunay tessellation field estimator

Job Feldbrugge
4 citations
Monthly Notices of the Royal Astronomical Society
Galaxies: Formation, Evolution, Phenomena
1.33
article

Phase-space Delaunay tessellation field estimator

Job Feldbrugge
article en
4 citations

Abstract

ABSTRACT The reconstruction of density and velocity fields is of central importance to the interpretation of N-body simulations. We propose a phase-space extension of the Delaunay tessellation field estimator (DTFE) that uses the mapping from Lagrangian to Eulerian space to track the dark matter fluid in phase-space. The new reconstruction scheme removes several artefacts from the conventional DTFE in multistream regions, while preserving the adaptive resolution in high-density regions and yielding continuous fields. The estimator also removes some tessellation artifacts of a previously proposed phase-space reconstruction scheme. The method is particularly suitable to the estimation of density and velocity fields of N-body simulations with multiple particle species and/or starting with glass initial conditions.

Monthly Notices of the Royal Astronomical SocietyVol. 536(1)
University of Edinburgh (GB)
University of Edinburgh
Sustainable cities and communities
Openalex Percentile: Top 19%
Galaxies: Formation, Evolution, Phenomena
1.33
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