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Intro
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Outline
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What are stochastic background searches
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Stochastic background searches
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Background characteristics
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Background direction
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Detection methods
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Crosscorrelation statistics
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Overlap functions
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Low signal limit
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Frequency space
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Directional dependence
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Overlap function
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Nongaussian background
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Numerical results
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Anisotropic searches
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Future prospects
Description:
Explore the fascinating world of stochastic background searches in gravitational wave experiments through this 50-minute lecture by Arianna Renzini from the California Institute of Technology. Delve into the concept of the stochastic gravitational wave background (SGWB), understanding how unresolved signals collectively form a background noise in gravitational wave detectors. Learn about various search methods employed in gravitational wave experiments, with a focus on ground-based networks. Discover the latest results from the LVK collaboration searches and gain insights into the estimated time-to-detection. Examine the potential for detection with LISA, the future space-borne gravitational wave observatory. Covering topics such as background characteristics, detection methods, cross-correlation statistics, and anisotropic searches, this comprehensive talk provides a thorough overview of current research and future prospects in the field of stochastic background searches in gravitational wave astronomy. Read more

Stochastic Background Searches in GW Experiments - IPAM at UCLA

Institute for Pure & Applied Mathematics (IPAM)
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