Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/48271
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Type: Journal article
Title: Beating the spin-down limit on gravitational wave emission from the Crab pulsar
Author: Abbott, B.
Abbott, R.
Adhikari, R.
Ajith, P.
Allen, B.
Allen, G.
Amin, R.
Anderson, S.
Anderson, W.
Arain, M.
Araya, M.
Armandula, H.
Armor, P.
Aso, Y.
Aston, S.
Aufmuth, P.
Aulbert, C.
Babak, S.
Ballmer, S.
Bantilan, H.
et al.
Citation: Astrophysical Journal, 2008; 683(1):L45-L49
Publisher: University of Chicago Press
Issue Date: 2008
ISSN: 0004-637X
1538-4357
Statement of
Responsibility: 
B. Abbott... A. Brooks... D. J. Hosken... J. Munch... D. J. Ottaway... P. J. Veitch... et al.
Abstract: We present direct upper limits on gravitational wave emission from the Crab pulsar using data from the first nine months of the fifth science run of the Laser Interferometer Gravitational-wave Observatory (LIGO). These limits are based on two searches. In the first we assume that the gravitational wave emission follows the observed radio timing, giving an upper limit on gravitational wave emission that beats indirect limits inferred from the spin-down and braking index of the pulsar and the energetics of the nebula. In the second we allow for a small mismatch between the gravitational and radio signal frequencies and interpret our results in the context of two possible gravitational wave emission mechanisms.
Description: Submitted to Cornell University's online archive www.arXiv.org in 2008 by Matthew Pitkin. Post-print sourced from www.arxiv.org. Erratum Appears within Astrophysical Journal, 2009; 706(1): L203-L204. DOI: http://dx.doi.org/10.1088/0004-637X/706/1/L203
Rights: © 2008 IOP Publishing
RMID: 0020082363
DOI: 10.1086/591526
Appears in Collections:Chemistry and Physics publications
Environment Institute publications

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