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A search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar
The LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +499
The physical mechanisms responsible for pulsar timing glitches are thought to excite quasi-normal mode oscillations in their parent neutron star that couple to gravitational wave e…
High-frequency corrections to the detector response and their effect on searches for gravitational waves
M. Rakhmanov, J. D. Romano, J. T. Whelan
Searches for gravitational waves with km-scale laser interferometers often involve the long-wavelength approximation to describe the detector response. The prevailing assumption is…
Determination of the angular momentum distribution of supernovae from gravitational wave observations
Kazuhiro Hayama, Shantanu Desai, Kei Kotake +4
Significant progress has been made in the development of an international network of gravitational wave detectors, such as TAMA300, LIGO, VIRGO, and GEO600. For these detectors, on…
Source Tracking for Sco X-1
Kazuhiro Hayama, Shantanu Desai, Soumya D. Mohanty +3
Sco X-1, the brightest low mass X-ray binary, is likely to be a source for gravitational wave emission. In one mechanism, emission of a gravitational wave arrests the increase in s…
Searches for gravitational waves associated with pulsar glitches using a coherent network algorithm
Kazuhiro Hayama, Shantanu Desai, Soumya D. Mohanty +3
Pulsar glitches are a potential source of gravitational waves for current and future interferometric gravitational wave detectors. Some pulsar glitch events were observed by radio…
First joint search for gravitational-wave bursts in LIGO and GEO600 data
LIGO Scientific Collaboration, B. Abbott
We present the results of the first joint search for gravitational-wave bursts by the LIGO and GEO600 detectors. We search for bursts with characteristic central frequencies in the…