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

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Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar. / LIGO Scientific Collaboration.
In: Astrophysical Journal Letters, Vol. 683, No. 1, 18.07.2008, p. L45-L49.

Research output: Contribution to Journal/MagazineLetterpeer-review

Harvard

LIGO Scientific Collaboration 2008, 'Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar', Astrophysical Journal Letters, vol. 683, no. 1, pp. L45-L49. https://doi.org/10.1086/591526

APA

LIGO Scientific Collaboration (2008). Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar. Astrophysical Journal Letters, 683(1), L45-L49. https://doi.org/10.1086/591526

Vancouver

LIGO Scientific Collaboration. Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar. Astrophysical Journal Letters. 2008 Jul 18;683(1):L45-L49. doi: 10.1086/591526

Author

LIGO Scientific Collaboration. / Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar. In: Astrophysical Journal Letters. 2008 ; Vol. 683, No. 1. pp. L45-L49.

Bibtex

@article{bafcb0886a7d4f3c88d7baadc2e4a985,
title = "Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar",
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.",
keywords = "gravitational waves, pulsars: individual: Crab pulsar, Astrophysics, General Relativity and Quantum Cosmology",
author = "{LIGO Scientific Collaboration} and M. Pitkin",
year = "2008",
month = jul,
day = "18",
doi = "10.1086/591526",
language = "English",
volume = "683",
pages = "L45--L49",
journal = "Astrophysical Journal Letters",
issn = "2041-8205",
publisher = "IOP Publishing Ltd",
number = "1",

}

RIS

TY - JOUR

T1 - Beating the Spin-Down Limit on Gravitational Wave Emission from the Crab Pulsar

AU - LIGO Scientific Collaboration

AU - Pitkin, M.

PY - 2008/7/18

Y1 - 2008/7/18

N2 - 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.

AB - 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.

KW - gravitational waves

KW - pulsars: individual: Crab pulsar

KW - Astrophysics

KW - General Relativity and Quantum Cosmology

U2 - 10.1086/591526

DO - 10.1086/591526

M3 - Letter

VL - 683

SP - L45-L49

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

SN - 2041-8205

IS - 1

ER -