56 citations · 187 across the 15 of their papers we have counts for
15 papers
Not too close! Evaluating the impact of the baseline on the localization of binary black holes by next-generation gravitational-wave detectors
Francesco Iacovelli, Luca Reali, Emanuele Berti +3
Next-generation (XG) gravitational-wave detectors, such as Cosmic Explorer (CE) and the Einstein Telescope (ET), will observe compact binary coalescences at unprecedented rates and…
Two-Step Procedure to Detect Cosmological Gravitational Wave Backgrounds with Next-Generation Terrestrial Gravitational-Wave Detectors
Haowen Zhong, Luca Reali, Bei Zhou +2
Cosmological gravitational-wave backgrounds are an exciting science target for next-generation ground-based detectors, as they encode invaluable information about the primordial Un…
Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers
Konstantinos Kritos, Luca Reali, Ken K. Y. Ng +2
Next-generation ground-based gravitational wave observatories will observe mergers of intermediate-mass black holes (IMBHs) out to high redshift. Such IMBHs can form through runawa…
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…
Black hole spectroscopy beyond Kerr: agnostic and theory-based tests with next-generation interferometers
Andrea Maselli, Sophia Yi, Lorenzo Pierini +4
Black hole spectroscopy is a clean and powerful tool to test gravity in the strong-field regime and to probe the nature of compact objects. Next-generation ground-based detectors,…
The impact of compact binary confusion noise on tests of fundamental physics with next-generation gravitational-wave detectors
Luca Reali, Andrea Maselli, Emanuele Berti
Next-generation ground-based gravitational-wave observatories such as the Einstein Telescope and Cosmic Explorer will detect signals from compact binary coalesce…
The impact of confusion noise on golden binary neutron-star events in next-generation terrestrial observatories
Luca Reali, Andrea Antonelli, Roberto Cotesta +4
Next-generation terrestrial gravitational-wave observatories will detect signals from compact binary coalescences every year. These signals can last for sever…
Compact Binary Foreground Subtraction in Next-Generation Ground-Based Observatories
Bei Zhou, Luca Reali, Emanuele Berti +4
The stochastic gravitational-wave backgrounds (SGWBs) for current detectors are dominated by binary black-hole (BBH) and binary neutron-star (BNS) coalescences. The sensitivity of…
Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
Bei Zhou, Luca Reali, Emanuele Berti +4
Stochastic gravitational-wave backgrounds (SGWBs) derive from the superposition of numerous individually unresolved gravitational-wave (GW) signals. Detecting SGWBs provides us wit…
Mapping the asymptotic inspiral of precessing binary black holes to their merger remnants
Luca Reali, Matthew Mould, Davide Gerosa +1
Multiple approaches are required to study the evolution of black-hole binaries. While the post-Newtonian approximation is sufficient to describe the early inspiral (even from infin…