collaborators

5 papers

gr-qc2025

Resolving white dwarf binaries within globular clusters with LISA

Wouter G. J. van Zeist, Gijs Nelemans, Shu-Xu Yi +1

Context: Globular clusters (GCs) around the Milky Way (MW) are expected to host white dwarf (WD) binaries emitting gravitational waves that could be detectable by LISA. Aims: Our a…

astro-ph.HE2025

White dwarf-neutron star binaries: a plausible pathway for long-duration gamma-ray bursts from compact object mergers?

A. A. Chrimes, N. Gaspari, A. J. Levan +7

Two long-duration gamma-ray bursts were recently discovered with kilonovae, the signature of r-process element production in a compact binary merger, rather than supernovae. This h…

astro-ph.SR2025

Comparing population synthesis models of compact double white dwarfs to electromagnetic observations

Wouter G. J. van Zeist, Jan van Roestel, Gijs Nelemans +3

Context: Studies of the Galactic population of double white dwarfs (DWDs) that would be detectable in gravitational waves by LISA have found differences in the number of predicted…

astro-ph.GA2024

Predicting gravitational wave signals from BPASS White Dwarf Binary and Black Hole Binary populations of a Milky Way-like galaxy model for LISA

Petra Tang, Jan Eldridge, Renate Meyer +3

Galactic white dwarf binaries (WDBs) and black hole binaries (BHBs) will be gravitational wave (GW) sources for LISA. Their detection will provide insights into binary evolution an…

gr-qc2024

Evaluating the gravitational wave detectability of globular clusters and the Magellanic Clouds for LISA

Wouter G. J. van Zeist, Gijs Nelemans, Simon F. Portegies Zwart +1

We use the stellar evolution code BPASS and the gravitational wave simulation code LEGWORK to simulate populations of compact binaries that may be detected by the in-development sp…