Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/99159
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dc.contributor.authorMcFerran, J.J.-
dc.contributor.authorDawkins, S.T.-
dc.contributor.authorStanwix, P.L.-
dc.contributor.authorTobar, M.E.-
dc.contributor.authorLuiten, A.N.-
dc.date.issued2006-
dc.identifier.citationOptics Express, 2006; 14(10):4316-4327-
dc.identifier.issn1094-4087-
dc.identifier.issn1094-4087-
dc.identifier.urihttp://hdl.handle.net/2440/99159-
dc.description.abstractWe demonstrate an optical frequency comb with fractional frequency instability of </=2x10(-14) at measurement times near 1 s, when the 10th harmonic of the comb spacing is controlled by a liquid helium cooled microwave sapphire oscillator. The frequency instability of the comb is estimated by comparing it to a cavity-stabilized optical oscillator. The less conventional approach of synthesizing low-noise optical signals from a microwave source is relevant when a laboratory has microwave sources with frequency stability superior to their optical counterparts. We describe the influence of high frequency environmental noise and how it impacts the phase-stabilized frequency comb performance at integration times less than 1 s.-
dc.description.statementofresponsibilityJ. J. McFerran, S. T. Dawkins, P. L. Stanwix, M. E. Tobar and A. N. Luiten-
dc.language.isoen-
dc.publisherOptical Society of America-
dc.rights© 2006 Optical Society of America-
dc.source.urihttp://dx.doi.org/10.1364/oe.14.004316-
dc.titleOptical frequency synthesis from a cryogenic microwave sapphire oscillator-
dc.typeJournal article-
dc.identifier.doi10.1364/OE.14.004316-
pubs.publication-statusPublished-
dc.identifier.orcidLuiten, A.N. [0000-0001-5284-7244]-
Appears in Collections:Aurora harvest 7
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