Forschungsergebnisse und Animationen
Numerical-relativistic simulation of a binary neutron star merger
The visualization shows the electron fraction on the left, the density in the center, and the magnetic field strength (1015 Gauss) on the right.
Second-long numerical-relativistic simulation of a binary neutron star merger
The visualization shows profiles for rest-mass density (top-left), magnetic-field strength (top-second from left), magnetization parameter (top-second from right), unboundedness defined by the Bernoulli criterion (top-right), electron fraction (bottom-left), temperature (bottom-second from left), entropy per baryon (bottom-second from right), and Shakura-Sunyaev αM parameter (bottom-right).
General-relativistic neutrino-radiation magnetohydrodynamic simulation of seconds-long black hole-neutron star mergers
Numerical simulation of a black hole-neutron star merger
Properties of the remnant disk and the dynamical ejecta produced in low-mass black hole-neutron star mergers
Merger of a low-mass black hole and neutron star leading to a black hole surrounded by an accretion disk
Mass ejection from disks surrounding a low-mass black hole: Viscous neutrino-radiation hydrodynamics simulation in full general relativity
Viscous evolution of disks for Mdisk = 0.1 M⊙