We present the optical and structural characterization of films of
Mechanical loss of dielectric mirror coatings sets fundamental limits for both gravitational wave detectors and cavity-stabilized optical local oscillators for atomic clocks. Two approaches are used to determine the mechanical loss: ringdown measurements of the coating quality factor and direct measurement of the coating thermal noise. Here we report a systematic study of the mirror thermal noise at 4, 16, 124, and 300 K by operating reference cavities at these temperatures. The directly measured thermal noise is used to extract the mechanical loss for
- Award ID(s):
- 1734006
- NSF-PAR ID:
- 10210894
- Publisher / Repository:
- Optical Society of America
- Date Published:
- Journal Name:
- Optics Letters
- Volume:
- 46
- Issue:
- 3
- ISSN:
- 0146-9592; OPLEDP
- Format(s):
- Medium: X Size: Article No. 592
- Size(s):
- Article No. 592
- Sponsoring Org:
- National Science Foundation
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