We describe directed searches for continuous gravitational waves (GWs) in data from the sixth Laser Interferometer Gravitational-wave Observatory (LIGO) science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target ' s parameters are uncertain enough to warrant two searches, for a total of 10. Each search covered a broad band of frequencies and first and second frequency derivatives for a fixed sky direction. The searches coherently integrated data from the two LIGO interferometers over time spans from 5.3-25.3 days using the matched-filtering. -statistic. We found no evidence of GW signals. We set 95% confidence upper limits as strong (low) as 4 x 10(-25) on intrinsic strain, 2 x 10(-7) on fiducial ellipticity, and 4 x 10(-5) on r-mode amplitude. These beat the indirect limits from energy conservation and are within the range of theoretical predictions for neutron-star ellipticities and r-mode amplitudes.

SEARCHES for CONTINUOUS GRAVITATIONAL WAVES from NINE YOUNG SUPERNOVA REMNANTS / Aasi, J., Abbott, B.P., Abbott, R., Abbott, T., Abernathy, M.R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R.X., Adya, V., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O.D., Ain, A., Ajith, P., Alemic, A., et al.. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - 813:1(2015), pp. 39-54. [10.1088/0004-637X/813/1/39]

SEARCHES for CONTINUOUS GRAVITATIONAL WAVES from NINE YOUNG SUPERNOVA REMNANTS

Allocca, A.;CALLONI, ENRICO;DE LAURENTIS, MARTINA;DE ROSA, ROSARIO;GARUFI, FABIO;MILANO, LEOPOLDO;Pinto, I. M.;Sequino, V.;
2015

Abstract

We describe directed searches for continuous gravitational waves (GWs) in data from the sixth Laser Interferometer Gravitational-wave Observatory (LIGO) science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target ' s parameters are uncertain enough to warrant two searches, for a total of 10. Each search covered a broad band of frequencies and first and second frequency derivatives for a fixed sky direction. The searches coherently integrated data from the two LIGO interferometers over time spans from 5.3-25.3 days using the matched-filtering. -statistic. We found no evidence of GW signals. We set 95% confidence upper limits as strong (low) as 4 x 10(-25) on intrinsic strain, 2 x 10(-7) on fiducial ellipticity, and 4 x 10(-5) on r-mode amplitude. These beat the indirect limits from energy conservation and are within the range of theoretical predictions for neutron-star ellipticities and r-mode amplitudes.
2015
SEARCHES for CONTINUOUS GRAVITATIONAL WAVES from NINE YOUNG SUPERNOVA REMNANTS / Aasi, J., Abbott, B.P., Abbott, R., Abbott, T., Abernathy, M.R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R.X., Adya, V., Affeldt, C., Agathos, M., Agatsuma, K., Aggarwal, N., Aguiar, O.D., Ain, A., Ajith, P., Alemic, A., et al.. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - 813:1(2015), pp. 39-54. [10.1088/0004-637X/813/1/39]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/618245
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