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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…
Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes
Vassiliki Kalogera, Christopher P L Berry, Monica Colpi +10
Next-generation observations will revolutionize our understanding of binary black holes and will detect new sources, such as intermediate-mass black holes. Primary science goals in…
Detectability of modulated X-rays from LISA's supermassive black hole mergers
Tito Dal Canton, Alberto Mangiagli, Scott C. Noble +5
One of the central goals of LISA is the detection of gravitational waves from the merger of supermassive black holes. Contrary to stellar-mass black hole mergers, such events are e…