The Stellar Populations and Dynamics Research Group

(The SPODYR Group)

Perth and the Indian Ocean, March 2016

Prof. Dr. Pavel Kroupa (CV)

Helmholtz-Institut fuer Strahlen- und Kernphysik, Theory Group, Universitaet Bonn
Rheinische Friedrich-Wilhelms-Universitaet
Nussallee 14-16
D-53115 Bonn
Germany

Postal and office address:
Argelander-Institut fuer Astronomie, Universitaet Bonn
Rheinische Friedrich-Wilhelms-Universitaet
Auf dem Huegel 71
D-53121 Bonn
Germany

Also professorem hospitem at:
Astronomical Institute of the Charles University in Prague
Faculty of Mathematics and Physics
v Holesovickach 2
18000 Praha 8
Czech Republic

e-mail: pkroupa @ uni-bonn.de
Tel: +49 (0)228 73-6140(office) // 73-3655 / -2366(secretary)
Fax: +49 (0)228 73-7666 / -2505

The functioning of galaxies: challenges for Newtonian and Milgromian dynamics
September 23-27, 2019 University of Bonn

A common Milgromian acceleration scale in nature

Correspondence (Nature Astronomy, Nov. 13th 2018) on D.C. Rodrigues et al. (2018, Nature Astronomy 2, 668)

Does the galaxy NGC1052-DF2 falsify Milgromian dynamics?

A Brief Communications Arising (Nature, Sept.12th 2018) from P. van Dokkum et al. Nature 555, 629–632 (2018)

2015: Phantom of Ramses (PoR) code for galaxy formation and evolution in Milgromian dynamics/MOND:

With a small grant from the Rectorate of the University of Bonn PK received in 2013, Fabian Lueghausen (in collaboration with Benoit Famaey and Pavel Kroupa) was able to develop in 2014 and 2015 a patch to Romain Teyssier's RAMSES code to allow dark-matter-free high-resolution simulations of galaxy formation and evolution.
The Phantom of Ramses (PoR) code is a patch to RAMSES. By default the patch comes with the RAMSES code whenever it is downloaded.

See the following link as to why cold or warm dark matter particles are not a dynamically relevant part of the Universe:
The Dark Matter Crisis: the rise and fall of a cosmological hypothesis

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