2008/03/18 by M. Principe, Maria Principe, I. M. Pinto +1
Physics and Astronomy · #Acoustics #Algorithm #Artificial intelligence #Astrophysics #Cold Atom Physics and Bose-Einstein Condensates #Component (thermodynamics) #Computer science #Detector #Gravitational wave #Interferometry #Limit (mathematics) #Mathematical analysis #Noise (video) #Optics #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Representation (politics) #Simple (philosophy) #Statistical Mechanics and Entropy #gr-qc
paper · pdf · doi:10.1088/0264-9381/25/7/075013
published as Class.Quant.Grav.25:075013,2008 · 15 pages, 8 figures
openalex publication_date 2008/03/18 · arxiv created 2008/06/27 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
An analytic model á la Middleton of the impulsive noise component in the data of interferometric gravitational wave detectors is proposed, based on an atomic representation of glitches. A fully analytic characterization of the coherent network data analysis algorithm proposed by Rakhmanov and Klimenko is obtained, for the simplest relevant case of triggered detection of unmodeled gravitational wave bursts, using the above noise model. The detector's performance is evaluated under a suitable central-limit hypothesis, and the effects of both the noisiness of the pseudo -templates and the presence of the impulsive noise component are highlighted.