Gravitational radiation of a differentially rotating superfluid neutron star |
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| Authors: | M V Hayrapetyan |
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| Institution: | (1) Erevan State University, Erevan, Armenia |
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| Abstract: | The gravitational radiation of a neutron star with a weakly coupled superfluid component is considered. It is assumed that
regions can exist in the star's core which rotate at substantially higher angular velocities than the observed angular velocities
of pulsars. A star of this sort has a quadrupole moment on the order of the maximum value for the neutron star configurations
that have been discussed, so it could be a powerful source of gravitational radiation for the planned Advanced LIGO detector.
Translated from Astrofizika, Vol. 51, No. 4, pp. 647–652 (November 2008). |
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| Keywords: | stars neutron rotation |
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