Collisions of black holes and neutron stars, named mixed binaries in the following, are interesting because of at least two reasons. Firstly, it is expected that they emit a large amount of energy as gravitational waves, which could be measured by new detectors. The form of those waves is expected to carry information about the internal structure of such systems. Secondly, collisions of such objects are the prime suspects of short gamma ray bursts. The exact mechanism for the energy emission is unknown so far...thesi
With the first direct detections of gravitational waves (GWs) from the coalescence of compact binari...
This dissertation investigates the signatures of electromagnetic radiation that may accompany two sp...
In this review we highlight a few physical properties of neutron stars and their theoretical treatme...
Collisions of black holes and neutron stars, named mixed binaries in the following, are interesting ...
The era of Gravitational Waves Astronomy was launched after the success of the first observation run...
We present the results of fully three dimensional, post-Newtonian hydrodynamical simulations of the...
We present the first simulations in full general relativity of the head-on collision between a neutr...
Black hole-neutron star mergers are extremely energetic events with the potential to generate gravit...
We present the first simulations in full General Relativity of the head-on collision between a neutr...
Hydrodynamic simulations of the merging of stellar mass black hole - neutron star binaries (BH/NS) a...
Black hole-neutron star (BH-NS) mergers are promising candidates for the progenitors of short-durat...
General relativistic simulations of black hole-neutron star mergers have currently been limited to l...
We present our latest results for simulation for merger of black hole (BH)-neutron star (NS) binarie...
Neutron star black hole (NSBH) mergers have captured the interest of physicists for more than 50 yea...
The first detections of black hole - neutron star mergers (GW200105 and GW200115) by the LIGO-Virgo-...
With the first direct detections of gravitational waves (GWs) from the coalescence of compact binari...
This dissertation investigates the signatures of electromagnetic radiation that may accompany two sp...
In this review we highlight a few physical properties of neutron stars and their theoretical treatme...
Collisions of black holes and neutron stars, named mixed binaries in the following, are interesting ...
The era of Gravitational Waves Astronomy was launched after the success of the first observation run...
We present the results of fully three dimensional, post-Newtonian hydrodynamical simulations of the...
We present the first simulations in full general relativity of the head-on collision between a neutr...
Black hole-neutron star mergers are extremely energetic events with the potential to generate gravit...
We present the first simulations in full General Relativity of the head-on collision between a neutr...
Hydrodynamic simulations of the merging of stellar mass black hole - neutron star binaries (BH/NS) a...
Black hole-neutron star (BH-NS) mergers are promising candidates for the progenitors of short-durat...
General relativistic simulations of black hole-neutron star mergers have currently been limited to l...
We present our latest results for simulation for merger of black hole (BH)-neutron star (NS) binarie...
Neutron star black hole (NSBH) mergers have captured the interest of physicists for more than 50 yea...
The first detections of black hole - neutron star mergers (GW200105 and GW200115) by the LIGO-Virgo-...
With the first direct detections of gravitational waves (GWs) from the coalescence of compact binari...
This dissertation investigates the signatures of electromagnetic radiation that may accompany two sp...
In this review we highlight a few physical properties of neutron stars and their theoretical treatme...