December 09, 2017: Postdoctoral position available
Multi-messenger Modelling of Compact Binary Mergers.
The merger of two neutron stars or a neutron star and a black hole is an astrophysical
event with many implications:
The physical modelling of such mergers is very challenging since their dynamics is shaped a multitude of physics ingredients:
- Such mergers are --together with binary black holes-- prime candidates to be detected by terrestrial
gravitational wave detectors.
- They likely produce the heaviest elements (such as platinum or gold) in the cosmos.
- The radioactive decay of freshly synthesized, heavy elements causes an electromagnetic transient
("macronova") that accompanies the expected gravitational wave signal and is crucial for
pinpointing and understanding the gravitational wave source.
Some introductory explanation of macronovae can be found under this link.
- Such mergers are likely the 'engine' behind short gamma-ray bursts.
We are looking for candidates with experience in computational modelling, (relativistic) magneto-/hydrodynamics, radiative transfer or similar.
- General Relativity: neutron stars and black holes have sizes comparable to their Schwarzschild radii, therefore strong-field gravity is important.
- Apart from gravity, the structure of a neutron star is shaped by the nuclear matter equation of state.
- The merger releases ~10^53 erg of gravitational energy which is released to a large extent in neutrinos.
- Despite their tiny interaction cross-sections, neutrinos can drive a strong baryonic wind from the remnant
of a compact binary merger. Such winds can also produce heavy elements and cause electromagnetic emission.
Closing date for the application is January 15, 2018.
Further details can be found under this link.