Point Absorber Limits to Future Gravitational-Wave Detectors
High-quality optical resonant cavities require low optical loss, typically on the scale of parts per million. However, unintended micron-scale contaminants on the resonator mirrors that absorb the light circulating in the cavity can deform the surface thermoelastically, and thus increase losses b...
Main Author: | Mavalvala, Nergis |
---|---|
Other Authors: | LIGO (Observatory : Massachusetts Institute of Technology) |
Format: | Article |
Language: | English |
Published: |
American Physical Society (APS)
2022
|
Online Access: | https://hdl.handle.net/1721.1/142160 |
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