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26 April 2024
 
  » arxiv » gr-qc/0405036

 Article overview



Incorporating information from source simulations into searches for gravitational-wave bursts
Patrick R Brady ; Saikat Ray-Majumder ;
Date 6 May 2004
Journal Class.Quant.Grav. 21 (2004) S1839-S1848
Subject gr-qc
AbstractThe detection of gravitational waves from astrophysical sources of gravitational waves is a realistic goal for the current generation of interferometric gravitational-wave detectors. Short duration bursts of gravitational waves from core-collapse supernovae or mergers of binary black holes may bring a wealth of astronomical and astrophysical information. The weakness of the waves and the rarity of the events urges the development of optimal methods to detect the waves. The waves from these sources are not generally known well enough to use matched filtering however; this drives the need to develop new ways to exploit source simulation information in both detections and information extraction. We present an algorithmic approach to using catalogs of gravitational-wave signals developed through numerical simulation, or otherwise, to enhance our ability to detect these waves. As more detailed simulations become available, it is straightforward to incorporate the new information into the search method. This approach may also be useful when trying to extract information from a gravitational-wave observation by allowing direct comparison between the observation and simulations.
Source arXiv, gr-qc/0405036
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