Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors-Reference-Cited by-同舟云学术

Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors

Published:2024-06-11 Issue:12 Volume:109 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Yi Sophia¹^ORCID,Kuntz Adrien²³^ORCID,Barausse Enrico²³^ORCID,Berti Emanuele¹^ORCID,Cheung Mark Ho-Yeuk¹^ORCID,Kritos Konstantinos¹^ORCID,Maselli Andrea⁴⁵^ORCID

Affiliation:

1. Johns Hopkins University

2. SISSA

3. IFPU - Institute for Fundamental Physics of the Universe

4. Gran Sasso Science Institute (GSSI)

5. Laboratori Nazionali del Gran Sasso

Funder

National Science Foundation

Croucher Foundation

Alexander S. Onassis Public Benefit Foundation

National Aeronautics and Space Administration

John Templeton Foundation

Simons Foundation

Ministero dell’Istruzione, dell’Università e della Ricerca

Multidisciplinary University Research Initiative

European Commission

European Research Council

Princeton University

HORIZON EUROPE Marie Sklodowska-Curie Actions

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.109.124029/fulltext

Reference130 articles.

1. Quasi-Normal Modes of Stars and Black Holes

2. Quasinormal modes of black holes and black branes

3. Extreme gravity tests with gravitational waves from compact binary coalescences: (II) ringdown

4. Inspiral, merger, and ring-down of equal-mass black-hole binaries

5. Mining information from binary black hole mergers: A comparison of estimation methods for complex exponentials in noise

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