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A&A 447, 1-7 (2006)
DOI: 10.1051/0004-6361:20053702
Gravitational wave background from magnetars
T. Regimbau and J. A. de Freitas PachecoObservatoire de la Côte d'Azur, Dpt. ARTEMIS and Dpt. CASSIOPEE, BP 4229, 06304 Nice Cedex 4, France
e-mail: regimbau@obs-nice.fr
(Received 27 June 2005 / Accepted 27 September 2005 )
Abstract
We investigate the gravitational wave background produced by
magnetars. The statistical properties of these highly magnetized
stars were derived by population synthesis methods and assumed to be
also representative of extragalactic objects. The adopted ellipticity
was calculated from relativistic models using equations of state and assumptions concerning the distribution of
currents in the neutron star interior. The maximum amplitude occurs
around 1.2 kHz, corresponding to
for a type I superconducting neutron star model. The expected signal is a continuous background
that could mask the cosmological contribution produced in the early stage of the Universe.
Key words: stars: neutron -- stars: magnetic fields -- gravitational waves
© ESO 2006
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