Blind source separation in 3rd generation gravitational-wave detectors

Fuente: arXiv
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Hauptverfasser: Badaracco, Francesca, Banerjee, Biswajit, Branchesi, Marica, Chincarini, Andrea
Format: Preprint
Veröffentlicht: 2024
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author Badaracco, Francesca
Banerjee, Biswajit
Branchesi, Marica
Chincarini, Andrea
author_facet Badaracco, Francesca
Banerjee, Biswajit
Branchesi, Marica
Chincarini, Andrea
contents Third generation and future upgrades of current gravitational-wave detectors will present exquisite sensitivities which will allow to detect a plethora of gravitational wave signals. Hence, a new problem to be solved arises: the detection and parameter estimation of overlapped signals. The problem of separating and identifying two signals that overlap in time, space or frequency is something well known in other fields (e.g. medicine and telecommunication). Blind source separation techniques are all those methods that aim at separating two or more unknown signals. This article provides a methodological review of the most common blind source separation techniques and it analyses whether they can be successfully applied to overlapped gravitational wave signals or not, while comparing the limits and advantages of each method.
format Preprint
id arxiv_https___arxiv_org_abs_2409_06458
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Blind source separation in 3rd generation gravitational-wave detectors
Badaracco, Francesca
Banerjee, Biswajit
Branchesi, Marica
Chincarini, Andrea
Instrumentation and Methods for Astrophysics
General Relativity and Quantum Cosmology
Third generation and future upgrades of current gravitational-wave detectors will present exquisite sensitivities which will allow to detect a plethora of gravitational wave signals. Hence, a new problem to be solved arises: the detection and parameter estimation of overlapped signals. The problem of separating and identifying two signals that overlap in time, space or frequency is something well known in other fields (e.g. medicine and telecommunication). Blind source separation techniques are all those methods that aim at separating two or more unknown signals. This article provides a methodological review of the most common blind source separation techniques and it analyses whether they can be successfully applied to overlapped gravitational wave signals or not, while comparing the limits and advantages of each method.
title Blind source separation in 3rd generation gravitational-wave detectors
topic Instrumentation and Methods for Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2409.06458