The Phantom of RAMSES user guide for galaxy simulations using Milgromian and Newtonian gravity-Reference-Cited by-同舟云学术

The Phantom of RAMSES user guide for galaxy simulations using Milgromian and Newtonian gravity

Published:2021-08 Issue:8 Volume:99 Page:607-613
ISSN:0008-4204
Container-title:Canadian Journal of Physics
language:en
Short-container-title:Can. J. Phys.

Author:

Nagesh S.T.¹,Banik I.²,Thies I.²,Kroupa P.²³,Famaey B.⁴,Wittenburg N.²,Parziale R.¹,Haslbauer M.²⁵

Affiliation:

1. Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, Bonn 53121, Germany.

2. Helmholtz-Institut für Strahlen- und Kernphysik, Universität Bonn, Nussallee 14-16, Bonn 53115, Germany.

3. Astronomical Institute, Faculty of Mathematics and Physics, Charles University in Prague, V Holešovičkách 2, Praha CZ-180 00, Czech Republic.

4. Université de Strasbourg, CNRS UMR 7550, Observatoire astronomique de Strasbourg, 11 rue de l’Université, Strasbourg 67000, France.

5. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, Bonn 53121, Germany.

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.

Publisher

Canadian Science Publishing

Subject

General Physics and Astronomy

Link

https://cdnsciencepub.com/doi/pdf/10.1139/cjp-2020-0624

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