Waveform model for an eccentric binary black hole based on the effective-one-body-numerical-relativity formalism-Reference-Cited by-同舟云学术

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Waveform model for an eccentric binary black hole based on the effective-one-body-numerical-relativity formalism

Published:2017-08-23 Issue:4 Volume:96 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Cao Zhoujian,Han Wen-Biao

Funder

National Natural Science Foundation of China

Youth Innovation Promotion Association of the Chinese Academy of Sciences

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.96.044028/fulltext

Reference83 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

3. GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

4. Gravitational wave astronomy: chance and challenge to fundamental physics and astrophysics

5. Effective-one-body model for black-hole binaries with generic mass ratios and spins

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1. Effective-one-body numerical-relativity waveform model for eccentric spin-precessing binary black hole coalescence;Classical and Quantum Gravity;2024-09-06

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3. Eccentricity Estimation for Five Binary Black Hole Mergers with Higher-order Gravitational-wave Modes;The Astrophysical Journal;2024-08-26

4. Probing eccentric higher-order modes through an effective chirp-mass model;Physical Review D;2024-08-09

5. Detectability of eccentric binary black holes with matched filtering and unmodeled pipelines during the third observing run of LIGO-Virgo-KAGRA;Physical Review D;2024-08-05

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