Search for Gravitational Wave Bursts from Six Magnetars

Authors

J. Abadie, LIGO - California Institute of Technology
B. P. Abbott, University of Glasgow
R. Abbott, Universite de Savoie
M. Abernathy, University of Naples Federico II
T. Accadia, University of Salerno
F. Acernese, California Institute of Technology
C. Adams, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
R. Adhikari, Leibniz University Hannover
C. Affeldt, University of Wisconsin-Milwaukee
B. Allen, Stanford University
G. S. Allen, University of Florida
E. Amador Ceron, Louisiana State University
D. Amariutei, National Institute for Nuclear Physics
R. S. Amin, University of Birmingham
S. B. Anderson, National Science Foundation
W. G. Anderson, Montana State University
F. Antonucci, European Gravitational Observatory
K. Arai, Carleton College
M. A. Arain, University of Western Australia
M. C. Araya, Massachusetts Institute of Technology
S. M. Aston, Universite Paris 7
P. Astone, Columbia University
D. Atkinson, Sezione di Pisa
P. Aufmuth, University of Pisa
C. Aulbert, National Institute for Subatomic Physics
B. E. Aylott, University of Texas at Brownsville
S. Babak, San Jose State University
P. Baker, Lomonosov Moscow State University
G. Ballardin, Universite de Nice-Sophia Antipolis
S. Ballmer, ComUE Paris-Saclay
Shaon Ghosh, Montclair State UniversityFollow

Document Type

Article

Publication Date

6-20-2011

Journal / Book Title

The Astrophysical journal letters

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 2 1erg and 1.4 × 10 47 d 2 1erg, 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.

DOI

10.1088/2041-8205/734/2/L35

MSU Digital Commons Citation

Abadie, J.; Abbott, B. P.; Abbott, R.; Abernathy, M.; Accadia, T.; Acernese, F.; Adams, C.; Adhikari, R.; Affeldt, C.; Allen, B.; Allen, G. S.; Amador Ceron, E.; Amariutei, D.; Amin, R. S.; Anderson, S. B.; Anderson, W. G.; Antonucci, F.; Arai, K.; Arain, M. A.; Araya, M. C.; Aston, S. M.; Astone, P.; Atkinson, D.; Aufmuth, P.; Aulbert, C.; Aylott, B. E.; Babak, S.; Baker, P.; Ballardin, G.; Ballmer, S.; and Ghosh, Shaon, "Search for Gravitational Wave Bursts from Six Magnetars" (2011). Department of Physics and Astronomy Faculty Scholarship and Creative Works. 107.
https://digitalcommons.montclair.edu/physics-astron-facpubs/107

Published Citation

Abadie, J., Abbott, B. P., Abbott, R., Abernathy, M., Accadia, T., Acernese, F., ... & Corbitt, T. R. (2011). Search for gravitational wave bursts from six magnetars. The Astrophysical journal letters, 734(2), L35.