Beyond the Bowen-York extrinsic curvature for spinning black holes

Hannam, Mark ORCID: https://orcid.org/0000-0001-5571-325X, Husa, Sascha, Brügmann, Bernd, González, José A. and Sperhake, Ulrich 2007. Beyond the Bowen-York extrinsic curvature for spinning black holes. Classical and Quantum Gravity 24 (12) , S15-S24. 10.1088/0264-9381/24/12/S02

Full text not available from this repository.

Abstract

It is well known that Bowen–York initial data contain spurious radiation. Although this 'junk' radiation has been seen to be small for non-spinning black-hole binaries in circular orbit, its magnitude increases when the black holes are given spin. It is possible to reduce the spurious radiation by applying the puncture approach to multiple Kerr black holes, as we demonstrate for examples of head-on collisions of equal-mass black-hole binaries.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Publisher:	IOPscience
ISSN:	0264-9381
Last Modified:	20 Oct 2022 08:18
URI:	https://orca.cardiff.ac.uk/id/eprint/27897

Citation Data

Cited 41 times in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item