Gravitational wave astrophysics
With the first detections of gravitational waves with Advanced LIGO a fact, with pulsar timing arrays reaching astrophysically interesting limits, and with the ESA LISA mission soon to be adopted, gravitational wave astrophysics will be the hot topic in astrophysics in the next decade(s). We are an institutional partner in the Virgo collaboration and were strongly involved in the discovery and interpretation of GW150914 and GW170817.
Our aim is to be a leading institute in the astronomical use of gravitational waves, i.e. the use of gravitational waves to understand their sources and the environments in which they originate. We lead the BlackGEM array for the detection of optical counterparts. We are involved in the LOFAR and MeerKAT radio arrays and lead the MeerLICHT project. Combining these initiatives with theory and modelling, we place ourselves in the midst of the action. Via Janssen we are part of the European Pulsar Timing array. Nelemans is the NL scientific lead on the LISA mission. There is strong interest in the Department to try and get the Einstein Telescope in the Netherlands, where Radboud could be the scientific/astrophysics centre, being closest to the proposed Dutch site.
Research questions to be addressed are:
- What is the population of gravitational sources detected with Advanced LIGO/Virgo?
- Can we detect the electromagnetic counterparts to conduct a combined GW/EM analysis?
- How do properties and rates of GW events constrain our understanding of massive star evolution?
- How did the elements form?
- What is the population of binaries to be seen in the LISA mission, both as Galactic sources and as Astrophysical GW background?
- Do intermediate mass black holes exist and can we see them merge?
- What do GW detected with pulsar timing arrays tell us about the (early) Universe?
Use is made of GW detectors, binary population modelling, stellar evolution codes, observations with LIGO/Virgo and, in particular, the BlackGEM array as well as MeerKAT/MeerLICHT.
Goals for the next six years
- Detect the electromagnetic counterparts of gravitational wave merger events
- Study the population of merger events in a combined analysis of GW+EM data.
- Connect the population of gravitational wave merger events to massive (binary) star evolution
- Understand the population of low-frequency gravitational wave emitters in our Milky Way Galaxy and beyond.
- Discover the first GW signals with pulsar timing arrays
- Build, operate, exploit and expand BlackGEM to cover ~40 square degrees instantaneously
Haven't found the information you were looking for? Please feel free to reach out to one of our experts: