Kavli Affiliate: Salvatore Vitale | Summary:Pair-instability supernovae leave behind no compact remnants, resulting in a predicted gap in the distribution of stellar black-hole masses. Gravitational waves from binary black-hole mergers probe the relevant mass range and analyses of the LIGO-Virgo-KAGRA catalog (GWTC-4) indicate a possible mass cutoff at $40$-$50M_odot$. However, the robustness of this result […]
Continue.. Measurement prospects for the pair-instability mass cutoff with gravitational waves