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Machine-learning interpolation of population-synthesis simulations to interpret gravitational-wave observations: a case study
Kaze W. K. Wong, Davide Gerosa
We report on advances to interpret current and future gravitational-wave events in light of astrophysical simulations. A machine-learning emulator is trained on numerical populatio…
Black holes in the low mass gap: Implications for gravitational wave observations
Anuradha Gupta, Davide Gerosa, K. G. Arun +3
Binary neutron-star mergers will predominantly produce black-hole remnants of mass , thus populating the putative \emph{low mass gap} between neutron stars and…
Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap
Davide Gerosa, Emanuele Berti
Pair instabilities in supernovae might prevent the formation of black holes with masses between and . Multiple generations of black-hole mergers…
Gravitational-wave detection rates for compact binaries formed in isolation: LIGO/Virgo O3 and beyond
Vishal Baibhav, Emanuele Berti, Davide Gerosa +4
Using simulations performed with the population synthesis code MOBSE, we compute the merger rate densities and detection rates of compact binary mergers formed in isolation for sec…
Are stellar-mass black-hole binaries too quiet for LISA?
Christopher J. Moore, Davide Gerosa, Antoine Klein
The progenitors of the high-mass black-hole mergers observed by LIGO and Virgo are potential LISA sources and promising candidates for multiband GW observations. In this letter, we…
Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
Yann Bouffanais, Michela Mapelli, Davide Gerosa +4
Ten binary black-hole mergers have already been detected during the first two observing runs of advanced LIGO and Virgo, and many more are expected to be observed in the near futur…