This approach assesses performance of gravitational waves detection in future configurations, suggesting potential enhancements.
This work introduces a geometrical method for analyzing transient gravitational waves recorded at interferometric observatories. This approach is intended to aid in assessing the performance and sensitivity of next-generation detector configurations, such as Cosmic Explorer, Einstein Telescope, and the South American Gravitational-wave Observatory.
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Osvaldo M. Moreschi (2026) studied this question.
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