Gravitational wave background from coalescing compact stars in eccentric orbits
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/327/2/531/3510696/327-2-531.pdf
Reference19 articles.
1. Confusion noise level due to galactic and extragalactic binaries
2. Gravitational-wave astronomy: new methods of measurements
3. Gravitational radiation and steady-state distribution of binary orbits: application to high-mass binary pulsars
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1. Non-Gaussianity from the cross-correlation of the astrophysical Gravitational Wave Background and the Cosmic Microwave Background;Journal of Cosmology and Astroparticle Physics;2023-10-01
2. Cross-correlation of the Astrophysical Gravitational Wave Background with the Cosmic Microwave Background;NUOVO CIM C-COLLOQ C;2023
3. OUP accepted manuscript;Monthly Notices of the Royal Astronomical Society;2020
4. Short gamma-ray bursts and gravitational-wave observations from eccentric compact binaries;Monthly Notices of the Royal Astronomical Society;2018-01-20
5. Synthetic model of the gravitational wave background from evolving binary compact objects;Physical Review D;2016-11-29
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