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Unveiling the Gravitational Universe at μ-Hz Frequencies
Alberto Sesana, Natalia Korsakova, Manuel Arca Sedda +31
We propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to -Hz frequency range. By the 2040s', the -Hz frequency band, bracketed in…
Merger rate of stellar black hole binaries above the pair instability mass gap
Alberto Mangiagli, Matteo Bonetti, Alberto Sesana +1
In current stellar evolutionary models, the occurrence of pair instability supernovae implies the lack of stellar black holes (BHs) with masses between about $[60, \, 120] \, \rm{M…
Neutron star binary orbits in their host potential: effect on early r-process enrichment
Matteo Bonetti, Albino Perego, Massimo Dotti +1
Coalescing neutron star binary (NSB) systems are primary candidates for -process enrichment of galaxies. The recent detection of -process elements in ultra-faint dwarf (UFD)…
The lifetime of binary black holes in Sérsic galaxy models
Nadia Biava, Monica Colpi, Pedro R. Capelo +5
In the local universe, black holes of M are hosted in galaxies displaying a variety of stellar profiles and morphologies. These black holes are the anticipated…