Search for gravitational wave bursts from six magnetars

Authors

J. Abadie
B. P. Abbott
R. AbbottFollow
M. Abernathy
Matthew Benacquista, The University of Texas Rio Grande ValleyFollow
Teviet Creighton, The University of Texas Rio Grande ValleyFollow
Mario C. Diaz, The University of Texas Rio Grande ValleyFollow
Soumya D. Mohanty, The University of Texas Rio Grande ValleyFollow
Soma Mukherjee, The University of Texas Rio Grande ValleyFollow
Volker Quetschke, The University of Texas Rio Grande ValleyFollow
Malik Rakhmanov, The University of Texas Rio Grande ValleyFollow

Document Type

Article

Publication Date

6-20-2011

Abstract

Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely 1kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0-5408, gave a burst with an estimated isotropic energy >1044erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between 2006 November and 2009 June, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090Hz), are 3.0 × 1044 d 21erg and 1.4 × 10 47 d 21erg, respectively, where and d 0501 is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time. © 2011. The American Astronomical Society. All rights reserved.

Comments

© Astrophysical Journal Letters. Original version available at: http://doi.org/10.1088/2041-8205/734/2/L35

Recommended Citation

Abadie, J., B. P. Abbott, R. Abbott, M. Abernathy, T. Accadia, Fausto Acernese, C. Adams et al. "Search for gravitational wave bursts from six magnetars." The Astrophysical journal letters 734, no. 2 (2011): L35. http://doi.org/10.1088/2041-8205/734/2/L35

Publication Title

Astrophysical Journal Letters

DOI

10.1088/2041-8205/734/2/L35