2012
DOI: 10.1038/nphoton.2012.217
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A sub-40-mHz-linewidth laser based on a silicon single-crystal optical cavity

Abstract: State-of-the-art optical oscillators based on lasers frequency stabilized to high finesse optical cavities are limited by thermal noise that causes fluctuations of the cavity length. Thermal noise represents a fundamental limit to the stability of an optical interferometer and plays a key role in modern optical metrology. We demonstrate a novel design to reduce the thermal noise limit for optical cavities by an order of magnitude and present an experimental realization of this new cavity system, demonstrating … Show more

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Cited by 644 publications
(472 citation statements)
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“…Steady work on ultrastable lasers [18][19][20]31,32 and interrogation sequences 17,33 has brought OLCs close to this limit [17][18][19][20] . Here, the two atomic clouds are probed independently by pulses delivered by an ultrastable laser (spectral width o1 Hz).…”
Section: Olc Architecturementioning
confidence: 99%
“…Steady work on ultrastable lasers [18][19][20]31,32 and interrogation sequences 17,33 has brought OLCs close to this limit [17][18][19][20] . Here, the two atomic clouds are probed independently by pulses delivered by an ultrastable laser (spectral width o1 Hz).…”
Section: Olc Architecturementioning
confidence: 99%
“…Such pure spectral instruments with high phase stability and long coherence times are essential to investigations of physics beyond the standard model, e.g., the drift of fundamental physical constants [9,10] or the detection of gravitational waves [11] as predicted by the general theory of relativity. The stability of the current state-of-the-art lasers are limited by Brownian motions of the reference cavity mirror substrates and coatings [12][13][14], and the emergence of new technologies [15] seems necessary if further improvements are to be made commonly available.…”
Section: Introductionmentioning
confidence: 99%
“…This is roughly an order of magnitude reduction in the shift and a factor of 50 reduction in the uncertainty due to secular motion time dilation in comparison with −ð16.3 AE 5.0Þ × 10 −18 , reported in the previous 27 Al þ optical clock [8]. Extending the clock interrogation time to 1 s [33][34][35][36], the fractional time-dilation shift due to secular motion is estimated to be −ð5.7 AE 0.3Þ × 10 −18 .…”
Section: Prl 118 053002 (2017) P H Y S I C a L R E V I E W L E T T Ementioning
confidence: 61%