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Guiding interferometer improvements with the frequency-dependent inspiral range

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arxiv 2502.07253 v1 pith:D5IBHQHP submitted 2025-02-11 astro-ph.IM gr-qc

Guiding interferometer improvements with the frequency-dependent inspiral range

classification astro-ph.IM gr-qc
keywords rangeinspiralmetricfrequency-dependentgravitational-waveguidinginterferometerinterferometers
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The inspiral range is the most common metric for characterizing the performance of ground-based gravitational-wave interferometers. However, there is no clear formalism for working with frequency-dependent inspiral range quantities. We introduce a metric for the cumulative normalized range of a gravitational-wave interferometer, as well as methods to compare two separate noise curves. We show how this metric is a valuable tool for guiding the commissioning of these interferometers and provides increased clarity compared to other commonly used approaches.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope

    astro-ph.IM 2026-07 accept novelty 6.0

    Degrading the Einstein Telescope's sensitivity in specific frequency bands hurts different science goals in predictable ways, but the mission remains scientifically strong even in the worst modelled cases.