Gravitational Wave Modelling

Numerical simulation of a black-hole binary merger with asymmetric masses and orbital precession. [more]

This numerical simulation represents the binary neutron star coalescence and merger which resulted in the detected gravitational-wave event GW190425. [more]

This discovery marks first cosmic event observed in both gravitational waves and light. [more]

When binary neutron stars inspiral and finally merge they emit gravitational waves. [more]

These numerical relativity simulations show the merging of two neutron stars. [more]

The figures and the animation show the coalescence of two orbiting black holes as detected by the Advanced LIGO and Advanced Virgo observatories on the 14^th of August 2017. [more]

The video and the images show a numerical simulation of the gravitational-wave event GW170104 associated to the third binary black-hole coalescence detected by LIGO. [more]

The video and the images show a numerical simulation of the gravitational-wave event GW151226 associated to a binary black-hole coalescence. [more]

Numerical-relativity simulations of the first binary black-hole merger observed by the Advanced LIGO detector on September 14, 2015. [more]

These images are the result if the numerical simulation of two inspiralling black holes that merge to form a new black hole. [more]

In this model, a smaller and a large black hole move linearly towards each other and collide head-on. The smaller black hole moves faster, has a high downward momentum and emits strong gravitational waves downwards. [more]

Electromagnetic Counterparts of Binary Black-Hole Mergers. [more]

Inspiraling Neutron Stars merge and form a Black Hole. [more]

Head-on collision of two neutron stars to a black hole or a neutron star. [more]

Computer simulations showing the formation of a neutron star by the gravitational collapse of a stellar core and the gravitational collapse of a neutron star to a rotating black hole. [more]

Computer simulations of an unstable spherical neutron star and of a rapidly spinning neutron star that is bar-like deformed by a dynamical instability. [more]