activity
20002006
most citedAxisymmetric core collapse simulations using characteristic numerical relativity

61 citations · 213 across the 8 of their papers we have counts for

collaborators

8 papers

physics.soc-ph2006

Balanced vehicular traffic at a bottleneck

Florian Siebel, Wolfram Mauser, Salissou Moutari +1

The balanced vehicular traffic model is a macroscopic model for vehicular traffic flow. We use this model to study the traffic dynamics at highway bottlenecks either caused by the…

physics.soc-ph2005★ 52 cited

Synchronized flow and wide moving jams from balanced vehicular traffic

Florian Siebel, Wolfram Mauser

Recently we proposed an extension to the traffic model of Aw, Rascle and Greenberg. The extended traffic model can be written as a hyperbolic system of balance laws and numerically…

cond-mat.stat-mech2005

On the fundamental diagram of traffic flow

Florian Siebel, Wolfram Mauser

We present a new fluid-dynamical model of traffic flow. This model generalizes the model of Aw and Rascle [SIAM J. Appl. Math. 60 916-938] and Greenberg [SIAM J. Appl. Math 62 729-…

gr-qc2003★ 61 cited

Axisymmetric core collapse simulations using characteristic numerical relativity

Florian Siebel, Jose A. Font, Ewald Mueller +1

We present results from axisymmetric stellar core collapse simulations in general relativity. Our hydrodynamics code has proved robust and accurate enough to allow for a detailed a…

gr-qc2001★ 50 cited

Simulating the dynamics of relativistic stars via a light-cone approach

Florian Siebel, Jose A. Font, Ewald Mueller +1

We present new numerical algorithms for the coupled Einstein-perfect fluid system in axisymmetry. Our framework uses a foliation based on a family of light cones, emanating from a…

gr-qc2001★ 42 cited

Scalar field induced oscillations of neutron stars and gravitational collapse

Florian Siebel, Jose A. Font, Philippos Papadopoulos

We study the interaction of massless scalar fields with self-gravitating neutron stars by means of fully dynamic numerical simulations of the Einstein-Klein-Gordon perfect fluid sy…