Hannam, Mark ORCID: https://orcid.org/0000-0001-5571-325X 2014. Modelling gravitational waves from precessing black-hole binaries: progress, challenges and prospects. General Relativity and Gravitation 46 (9) , 1767. 10.1007/s10714-014-1767-2 |
Preview |
PDF
- Published Version
Available under License Creative Commons Attribution. Download (569kB) | Preview |
Abstract
The inspiral and merger of two orbiting black holes is among the most promising sources for the first (hopefully imminent) direct detection of gravitational waves (GWs), and measurements of these signals could provide a wealth of information about astrophysics, fundamental physics and cosmology. Detection and measurement require a theoretical description of the GW signals from all possible black-hole-binary configurations, which can include complicated precession effects due to the black-hole spins. Modelling the GW signal from generic precessing binaries is therefore one of the most urgent theoretical challenges facing GW astronomy. This article briefly reviews the phenomenology of generic-binary dynamics and waveforms, and recent advances in modelling them
Item Type: | Article |
---|---|
Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QC Physics |
Publisher: | Springer Verlag |
ISSN: | 0001-7701 |
Funders: | STFC |
Date of First Compliant Deposit: | 30 March 2016 |
Date of Acceptance: | 30 June 2014 |
Last Modified: | 06 May 2023 05:35 |
URI: | https://orca.cardiff.ac.uk/id/eprint/63698 |
Citation Data
Cited 27 times in Scopus. View in Scopus. Powered By Scopus® Data
Actions (repository staff only)
Edit Item |