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Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes

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arxiv 1903.09220 v1 pith:CZIYR4NB submitted 2019-03-21 astro-ph.HE gr-qc

Vassiliki Kalogera (Northwestern U) , Christopher P L Berry (Northwestern U.) , Monica Colpi (U. of Milano-Bicocca) , Steve Fairhurst (Cardiff U.) , Stephen Justham (UCAS , Beijing , U. of Amsterdam) , Ilya Mandel (Monash U.)
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Alberto Mangiagli (U. of Milano-Bicocca) Michela Mapelli (U. of Padova) Cameron Mills (Cardiff U.) B.S. Sathyaprakash (Penn State U. Cardiff U.) Raffaella Schneider (INFN Roma) Thomas Tauris (Aarhus U.) Rosa Valiante (INAF Roma)
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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 include: Discover binary black holes throughout the observable Universe; Reveal the fundamental properties of black holes; Uncover the seeds of supermassive black holes.

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Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Assessing the performance of future space-based detectors: Astrophysical foregrounds and individual sources

    astro-ph.HE 2025-10 conditional novelty 6.0 of 10

    A unified foreground simulation shows the μAres concept is heavily blurred by massive-black-hole-binary noise while the Decihertz Observatory is the cleanest post-LISA design.

  2. Beyond Gaussian Assumptions: A new robust statistical framework for gravitational-wave data analysis

    gr-qc 2026-02 conditional novelty 5.0 of 10

    A heavy-tailed hyperbolic likelihood, applied across the full frequency band, gives gravitational-wave parameter estimates that are as good as standard methods in Gaussian noise and less biased in glitchy or overlappi...

  3. Spin evolution and mass distribution of the Galactic Binary Neutron Stars

    astro-ph.HE 2024-12 conditional novelty 5.0 of 10

    A population synthesis model with detailed neutron star spin evolution reproduces the observed Galactic binary neutron star population and explains why heavy systems like GW190425 are rarely seen in radio surveys.

  4. Mapping the star formation peak with LIGO A# and Next-Generation detectors

    gr-qc 2026-06 unverdicted novelty 4.0 of 10

    Simulations show LIGO-A# constrains the peak redshift of binary black hole merger rate (tracing star formation) to ±0.1 in one year, improving to ±0.02 with next-generation detectors.

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