Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar

Document #:

LIGO-P070118-x0

Document type:

P - Publications

Abstract:

We present direct upper limits on gravitational wave emission from the Crab pulsar using data from the first 9 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.

Files in Document:

• P070118-00.pdf (file is not accessible)

Other Files:

• P070118-P.pdf (file is not accessible)

Topics:

• Document Migration from the old DCC
• Public relations

Author Groups:

• LSC

Notes and Changes:

Rev P070118-00-Z:
- Full document number: LIGO-P070118-00-Z
- Author(s): Ligo Scientific Collaboration
- Document date: 2007-03-07
- Document received date: 2008-03-11
- Document entry date: 2008-03-11

Journal References:

Published in ApJ Letters vol. 683 pg. L45-L49.

Publication Information:

http://www.iop.org/EJ/abstract/1538-4357/683/1/L45/591526.pdf?request-id=42d4aeb4-68f6-4806-9a74-0971ba3583fc