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[en] t Glitches in pulsars are likely to trigger oscillation modes in the fluid interior of neutron stars. We examined these oscillations specifically at r-mode frequencies. The excited r-modes will emit gravitational waves and can have long damping time scales O(minutes - days). We use simple estimates of how much energy the glitch might put into the r-mode and assess the detectability of the emitted gravitational waves with future interferometers.
Journal
Journal of Physics. Conference Series (Online); ISSN 1742-6596; 
; v. 363(1); [5 p.]
; v. 363(1); [5 p.]