56 citations · 187 across the 15 of their papers we have counts for
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Minimum gas mass accreted by spinning intermediate-mass black holes in stellar clusters
Konstantinos Kritos, Luca Reali, Davide Gerosa +1
The spin of intermediate-mass black holes (IMBHs) growing through repeated black hole mergers in stellar clusters statistically asymptotes to zero. Putative observations of IMBHs w…
Searching for cosmological stochastic backgrounds by notching out resolvable compact binary foregrounds with next-generation gravitational-wave detectors
Haowen Zhong, Bei Zhou, Luca Reali +2
Stochastic gravitational-wave backgrounds can be of either cosmological or astrophysical origin. The detection of an astrophysical stochastic gravitational-wave background with gro…
Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks
Luca Reali, Roberto Cotesta, Andrea Antonelli +3
Astrophysical scenarios for the formation and evolution of intermediate-mass black holes (IMBHs) in the mass range remain uncertain,…
Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors
Veome Kapil, Luca Reali, Roberto Cotesta +1
Next-generation gravitational wave detectors such as the Einstein Telescope and Cosmic Explorer will have increased sensitivity and observing volumes, enabling unprecedented precis…
Possible Causes of False General Relativity Violations in Gravitational Wave Observations
Anuradha Gupta, K. G. Arun, Enrico Barausse +40
General relativity (GR) has proven to be a highly successful theory of gravity since its inception. The theory has thrivingly passed numerous experimental tests, predominantly in w…
Beyond the far side: Observing black hole mergers beyond the pair-instability mass gap with next-generation gravitational wave detectors
Gabriele Franciolini, Konstantinos Kritos, Luca Reali +2
Stellar evolution predicts the existence of a mass gap for black hole remnants produced by pair-instability supernova dynamics, whose lower and upper edges are very uncertain. We s…