Stochastic gravitational wave background from highly-eccentric stellar-mass binaries in the millihertz band-Reference-Cited by-同舟云学术

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Stochastic gravitational wave background from highly-eccentric stellar-mass binaries in the millihertz band

Published:2024-07-15 Issue:2 Volume:110 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Xuan Zeyuan¹¹^ORCID,Naoz Smadar¹¹^ORCID,Kocsis Bence²^ORCID,Michaely Erez¹¹^ORCID

Affiliation:

1. UCLA

2. Oxford

Funder

National Aeronautics and Space Administration

National Science Foundation

Science and Technology Facilities Council

Bhaumik Institute for Theoretical Physics summer fellowship

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.110.023020/fulltext

Reference143 articles.

1. Observing complete gravitational wave signals from dynamical capture binaries

2. THE FORMATION OF ECCENTRIC COMPACT BINARY INSPIRALS AND THE ROLE OF GRAVITATIONAL WAVE EMISSION IN BINARY-SINGLE STELLAR ENCOUNTERS

3. Detectability of eccentric compact binary coalescences with advanced gravitational-wave detectors

4. Eccentric Black Hole Gravitational-wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters

5. Accuracy of Estimating Highly Eccentric Binary Black Hole Parameters with Gravitational-wave Detections

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