The phantom of ramses user guide for galaxy simulations using milgromian and newtonian gravity

S. T. Nagesh; I. Banik; I. Thies; P. Kroupa; B. Famaey; N. Wittenburg; R. Parziale; M. Haslbauer

doi:10.1139/cjp-2020-0624

The phantom of ramses user guide for galaxy simulations using milgromian and newtonian gravity

S. T. Nagesh^*, I. Banik, I. Thies, P. Kroupa, B. Famaey, N. Wittenburg, R. Parziale, M. Haslbauer

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

This document describes the general process of setting up, running, and analysing disc galaxy simulations using the freely available program Phantom of RAMSES (POR). This implements Milgromian dynamics (MOND) with a patch to the RAMSES grid-based N-body and hydrodynamical code that uses adaptive mesh refinement. We discuss the procedure of setting up isolated and interacting disc galaxy initial conditions for POR, running the simulations, and analysing the results. This manual also concisely documents all previously developed MOND simulation codes and the results obtained with them.

Original language	English
Pages (from-to)	607-613
Number of pages	7
Journal	Canadian Journal of Physics
Volume	99
Issue number	8
Early online date	3 Feb 2021
DOIs	https://doi.org/10.1139/cjp-2020-0624
Publication status	Published - Aug 2021

Keywords

Galaxy formation and evolution
Gravitation
Milgromian dynamics
Numerical simulations
Phantom of Ramses

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10.1139/cjp-2020-0624

Cite this

@article{e090b25bf2e848838320bbaa62b7db6e,

title = "The phantom of ramses user guide for galaxy simulations using milgromian and newtonian gravity",

abstract = "This document describes the general process of setting up, running, and analysing disc galaxy simulations using the freely available program Phantom of RAMSES (POR). This implements Milgromian dynamics (MOND) with a patch to the RAMSES grid-based N-body and hydrodynamical code that uses adaptive mesh refinement. We discuss the procedure of setting up isolated and interacting disc galaxy initial conditions for POR, running the simulations, and analysing the results. This manual also concisely documents all previously developed MOND simulation codes and the results obtained with them.",

keywords = "Galaxy formation and evolution, Gravitation, Milgromian dynamics, Numerical simulations, Phantom of Ramses",

author = "Nagesh, {S. T.} and I. Banik and I. Thies and P. Kroupa and B. Famaey and N. Wittenburg and R. Parziale and M. Haslbauer",

note = "Funding Information: IB is supported by an Alexander von Humboldt Foundation postdoctoral research fellowship. BF acknowledges funding from the Agence Nationale de la Recherche (ANR project ANR-18-CE31-0006 and ANR-19-CE31-0017) and from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No. 834148).",

year = "2021",

month = aug,

doi = "10.1139/cjp-2020-0624",

language = "English",

volume = "99",

pages = "607--613",

journal = "Canadian Journal of Physics",

issn = "0008-4204",

publisher = "National Research Council of Canada",

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TY - JOUR

T1 - The phantom of ramses user guide for galaxy simulations using milgromian and newtonian gravity

AU - Nagesh, S. T.

AU - Banik, I.

AU - Thies, I.

AU - Kroupa, P.

AU - Famaey, B.

AU - Wittenburg, N.

AU - Parziale, R.

AU - Haslbauer, M.

N1 - Funding Information: IB is supported by an Alexander von Humboldt Foundation postdoctoral research fellowship. BF acknowledges funding from the Agence Nationale de la Recherche (ANR project ANR-18-CE31-0006 and ANR-19-CE31-0017) and from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No. 834148).

PY - 2021/8

Y1 - 2021/8

N2 - This document describes the general process of setting up, running, and analysing disc galaxy simulations using the freely available program Phantom of RAMSES (POR). This implements Milgromian dynamics (MOND) with a patch to the RAMSES grid-based N-body and hydrodynamical code that uses adaptive mesh refinement. We discuss the procedure of setting up isolated and interacting disc galaxy initial conditions for POR, running the simulations, and analysing the results. This manual also concisely documents all previously developed MOND simulation codes and the results obtained with them.

AB - This document describes the general process of setting up, running, and analysing disc galaxy simulations using the freely available program Phantom of RAMSES (POR). This implements Milgromian dynamics (MOND) with a patch to the RAMSES grid-based N-body and hydrodynamical code that uses adaptive mesh refinement. We discuss the procedure of setting up isolated and interacting disc galaxy initial conditions for POR, running the simulations, and analysing the results. This manual also concisely documents all previously developed MOND simulation codes and the results obtained with them.

KW - Galaxy formation and evolution

KW - Gravitation

KW - Milgromian dynamics

KW - Numerical simulations

KW - Phantom of Ramses

UR - https://arxiv.org/abs/2101.11011

U2 - 10.1139/cjp-2020-0624

DO - 10.1139/cjp-2020-0624

M3 - Article

AN - SCOPUS:85112630195

SN - 0008-4204

VL - 99

SP - 607

EP - 613

JO - Canadian Journal of Physics

JF - Canadian Journal of Physics

IS - 8

ER -

The phantom of ramses user guide for galaxy simulations using milgromian and newtonian gravity

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Keywords

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