SNR degradation in matched-filter detection of GW chirps from coalescing binaries due to neglect of the relativistic periastron advance

Details SNR degradation in matched-filter detection of GW chirps from coalescing binaries due to neglect of the relativistic periastron advance SNR degradation in matched-filter detection of GW chirps from coalescing binaries due to neglect of the relativistic periastron advance

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phla..173..121p&link_type=abstract

Physics Letters A, Volume 173, Issue 2, p. 121-125.

Physics

2

Scientific paper

The signal-to-noise-ratio degradation due to the neglect of the relativistic periastron advance in matched-filter detection of gravitational wave chirps emitted from coalescing binary stars is computed. The result shows quite dramatically the relevance of this effect, as well as its dependence on the total mass and mass ratio of the companion stars.

Affiliated with

Also associated with

No associations

Rating

SNR degradation in matched-filter detection of GW chirps from coalescing binaries due to neglect of the relativistic periastron advance does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with SNR degradation in matched-filter detection of GW chirps from coalescing binaries due to neglect of the relativistic periastron advance, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and SNR degradation in matched-filter detection of GW chirps from coalescing binaries due to neglect of the relativistic periastron advance will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1276437