activity
20082022
most citedProspects for testing the nature of Sgr A*'s NIR flares on the basis of current VLT- and future VLTI-observations

93 citations · 208 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2022★ 32 cited

Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations

Metin Ata, Khee-Gan Lee, Claudio Dalla Vecchia +5

Cosmological simulations are crucial tools in studying the Universe, but they typically do not directly match real observed structures. Constrained cosmological simulations, on the…

gr-qc2014★ 6 cited

Wavefronts and Light Cones for Kerr Spacetimes

Francisco Frutos-Alfaro, Frank Grave, Thomas Mueller +1

We investigate the light propagation by means of simulations of wavefronts and light cones for Kerr spacetimes. Simulations of this kind give us a new insight to better understand…

physics.comp-ph2014★ 6 cited

Visual appearance of wireframe objects in special relativity

Thomas Müller, Sebastian Boblest

The visual appearance of a moving object in special relativity can be constructed in a straightforward manner when representing the surface of the object, or at least a wire frame…

physics.ed-ph2014★ 2 cited

MPPhys - A many-particle simulation package for computational physics education

Thomas Müller

In a first course to classical mechanics elementary physical processes like elastic two-body collisions, the mass-spring model, or the gravitational two-body problem are discussed…

physics.class-ph2012★ 4 cited

Charged particles constrained to a curved surface

Thomas Müller, Jörg Frauendiener

We study the motion of charged particles constrained to arbitrary two-dimensional curved surfaces but interacting in three-dimensional space via the Coulomb potential. To speed-up…

gr-qc2012★ 25 cited

Interactive visualization of a thin disc around a Schwarzschild black hole

Thomas Müller, Jörg Frauendiener

In the first course of general relativity, the Schwarzschild spacetime is the most discussed analytic solution to Einstein's field equations. Unfortunately, there is rarely enough…