Large and extremely low loss: the unique challenges of gravitational wave mirrors - Archive ouverte HAL
Article Dans Une Revue Journal of the Optical Society of America. A Optics, Image Science, and Vision Année : 2019

Large and extremely low loss: the unique challenges of gravitational wave mirrors

Résumé

This paper describes the making of large mirrors for laser interferometer gravitational wave detectors. These optics, working in the near infrared, are among the best optics ever created and played a crucial role in the first direct detection of gravitational waves from black holes or neutron star fusions.

Domaines

Sciences de l'ingénieur [physics] Chimie Physique [physics]

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https://hal.science/hal-02417232

Soumis le : mercredi 18 décembre 2019-09:52:07

Dernière modification le : lundi 4 novembre 2024-08:00:03

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Dates et versions

hal-02417232 , version 1 (18-12-2019)

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Citer

Jérôme Degallaix, Christophe Michel, Benoît Sassolas, Annalisa Allocca, Gianpietro Cagnoli, et al.. Large and extremely low loss: the unique challenges of gravitational wave mirrors. Journal of the Optical Society of America. A Optics, Image Science, and Vision, 2019, 36 (11), pp.C85. ⟨10.1364/JOSAA.36.000C85⟩. ⟨hal-02417232⟩

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