Stray light is one of the major limitations of the sensitivity of interferometric gravitational wave detectors, as introduced in Sect. 2.2.6 . The laser beam propagates through several optical elements that can back-reflect and scatter it.

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Stray Light in Gravitational Waves Detectors

  • Eleonora Polini

摘要

Stray light is one of the major limitations of the sensitivity of interferometric gravitational wave detectors, as introduced in Sect. 2.2.6 . The laser beam propagates through several optical elements that can back-reflect and scatter it.