2 papers
astro-ph.HE2026
Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae
Bailey Sykes, Bernhard Müller
The quantitative impact of strong rotation on the amplitudes and frequencies of the post-bounce gravitational wave (GW) signal from core-collapse supernovae (CCSNe) is still not fu…
astro-ph.HE2026
The deci-Hz gravitational wave signal from the collapse of rotating very massive stars
Bailey Sykes, Jade Powell, Bernhard Müller +1
We calculate the gravitational wave signal from the collapse of a rotating 300 star at the upper end of the pair-instability regime. The large-scale asymmetries that deve…