Citations
When using this package for scientific research, please cite
@software{Feldbrugge:2026,
author = {Job Feldbrugge},
title = {jfeldbrugge/Nbody2D.jl: Nbody2D.jl},
month = may,
year = 2026,
publisher = {Zenodo},
version = {v1.0.0},
doi = {10.5281/zenodo.20115154},
url = {https://doi.org/10.5281/zenodo.20115154},
}and the related Python code
@software{Hidding:2020,
author = {Johannes Hidding},
title = {jhidding/nbody2d: 2d PM n-body code},
month = oct,
year = 2020,
publisher = {Zenodo},
version = {v0.1.0},
doi = {10.5281/zenodo.4158731},
url = {https://doi.org/10.5281/zenodo.4158731}
}References
For more information about constrained Gaussian random field theory, see
@ARTICLE{Hoffman:1991,
author = {{Hoffman}, Yehuda and {Ribak}, Erez},
title = "{Constrained Realizations of Gaussian Fields: A Simple Algorithm}",
journal = {\apjl},
keywords = {Astronomical Models, Computational Astrophysics, Computerized Simulation, Cosmology, Algorithms, Dark Matter, Fast Fourier Transformations, Galactic Clusters, Many Body Problem, Power Spectra, Astrophysics, COSMOLOGY, GALAXIES: CLUSTERING},
year = 1991,
month = oct,
volume = {380},
pages = {L5},
doi = {10.1086/186160},
adsurl = {https://ui.adsabs.harvard.edu/abs/1991ApJ...380L...5H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Weygaert:1996,
author = {{van de Weygaert}, Rien and {Bertschinger}, Edmund},
title = "{Peak and gravity constraints in Gaussian primordial density fields: An application of the Hoffman-Ribak method}",
journal = {\mnras},
keywords = {METHODS: NUMERICAL GALAXIES: CLUSTERS: GENERAL, COSMOLOGY: THEORY, LARGE-SCALE STRUCTURE OF UNIVERSE, Astrophysics},
year = 1996,
month = jul,
volume = {281},
pages = {84},
doi = {10.1093/mnras/281.1.84},
archivePrefix = {arXiv},
eprint = {astro-ph/9507024},
primaryClass = {astro-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/1996MNRAS.281...84V},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Feldbrugge:2023,
author = {{Feldbrugge}, Job and {van de Weygaert}, Rien},
title = "{Cosmic web \& caustic skeleton: non-linear constrained realizations - 2D case studies}",
journal = {\jcap},
keywords = {cosmic web, cosmological simulations, dark matter simulations, Statistical sampling techniques, Astrophysics - Cosmology and Nongalactic Astrophysics, General Relativity and Quantum Cosmology},
year = 2023,
month = feb,
volume = {2023},
number = {2},
eid = {058},
pages = {058},
doi = {10.1088/1475-7516/2023/02/058},
archivePrefix = {arXiv},
eprint = {2212.07840},
primaryClass = {astro-ph.CO},
adsurl = {https://ui.adsabs.harvard.edu/abs/2023JCAP...02..058F},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}For more information about cosmological particle mesh codes, see
@ARTICLE{Klypin:1997,
author = {{Klypin}, Anatoly and {Holtzman}, Jon},
title = "{Particle-Mesh code for cosmological simulations}",
journal = {arXiv e-prints},
keywords = {Astrophysics},
year = 1997,
month = dec,
eid = {astro-ph/9712217},
pages = {astro-ph/9712217},
doi = {10.48550/arXiv.astro-ph/9712217},
archivePrefix = {arXiv},
eprint = {astro-ph/9712217},
primaryClass = {astro-ph},
adsurl = {https://ui.adsabs.harvard.edu/abs/1997astro.ph.12217K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}For more information about the Phase-Space Delaunay Tessellation Field Estimator, see
@article{Feldbrugge:2024,
author = {Feldbrugge, Job},
title = {Phase-space Delaunay tessellation field estimator},
journal = {Monthly Notices of the Royal Astronomical Society},
volume = {536},
number = {1},
pages = {807-815},
year = {2024},
month = {12},
issn = {0035-8711},
doi = {10.1093/mnras/stae2627},
url = {https://doi.org/10.1093/mnras/stae2627},
eprint = {https://academic.oup.com/mnras/article-pdf/536/1/807/61019429/stae2627.pdf}
}For the estimator applied to three-dimensional $N$-body simulation see PhaseSpaceDTFE.jl.