The gravitational wave 'probability event horizon' for double neutron star mergers

Monthly Notices of the Royal Astronomical Society

Volumn 364, Issue 3, 2005, Pages 807-812

  Coward, D M ^a   Lilley, M ^a   Howell, E J ^a   Burman, R R ^a   Blair, D G ^a  

^a UNIVERSITY OF WESTERN AUSTRALIA   (Australia)

Author keywords

Binaries: close; Gravitational waves; Pulsars: general; Supernovae: general

Indexed keywords

GEOMETRY; GRAVITATIONAL EFFECTS; INTERFEROMETERS; LASER INTERFEROMETRY; MERGERS AND ACQUISITIONS; MERGING; PROBABILITY; SIGNAL PROCESSING; SIGNAL TO NOISE RATIO; STOCHASTIC SYSTEMS; WHITE NOISE;

BINARIES: CLOSE; BINARY SYSTEMS; EVENT HORIZON; GRAVITATIONAL-WAVES; LASER INTERFEROMETER GRAVITATIONAL-WAVE OBSERVATORIES; NEUTRON STARS; PULSARS: GENERAL; STARS: BINARIES; STOCHASTICS; SUPERNOVAE: GENERAL;

GRAVITY WAVES;

EID: 29144462038     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09613.x     Document Type: Article

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