Surrogate model for gravitational wave signals from nonspinning, comparable-to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity-Reference-Cited by-同舟云学术

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Surrogate model for gravitational wave signals from nonspinning, comparable-to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity

Published:2022-11-14 Issue:10 Volume:106 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Islam Tousif^ORCID,Field Scott E.,Hughes Scott A.^ORCID,Khanna Gaurav^ORCID,Varma Vijay^ORCID,Giesler Matthew^ORCID,Scheel Mark A.,Kidder Lawrence E.,Pfeiffer Harald P.

Funder

National Science Foundation

Heising-Simons Foundation

Simons Foundation

H2020 Marie Skłodowska-Curie Actions

Office of Naval Research

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.106.104025/fulltext

Reference89 articles.

1. GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

2. GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run

3. Ultraluminous X-ray sources in the Chandra and XMM-Newton era

4. A 400-solar-mass black hole in the galaxy M82

5. Observational evidence for intermediate-mass black holes

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