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Optical frequency combs for low phase noise microwave generation

  • F. Quinlan*
  • , T. M. Fortier
  • , M. S. Kirchner
  • , J. A. Taylor
  • , J. C. Bergquist
  • , T. Rosenband
  • , N. Lemke
  • , A. Ludlow
  • , Y. Jiang
  • , C. W. Oates
  • , S. A. Diddams
  • *Corresponding author for this work
  • National Institute of Standards and Technology

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

An optical frequency comb locked to a stable optical reference can serve as a source for microwave signals having very low close-to-carrier phase noise. This has recently been confirmed by comparing two independent systems, yielding an absolute phase noise of -104 dBc/Hz at 1 Hz offset from a 10 GHz carrier. The corresponding timing jitter is 760 attoseconds, integrated from 1 Hz to 1 MHz. Here we describe the system architecture, as well as technical and fundamental noise limitations.

Original languageEnglish
Title of host publication2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011
DOIs
StatePublished - 2011
Event2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011 - Istanbul, Turkey
Duration: 13 Aug 2011 → 20 Aug 2011

Publication series

Name2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011

Conference

Conference2011 30th URSI General Assembly and Scientific Symposium, URSIGASS 2011
Country/TerritoryTurkey
CityIstanbul
Period13/08/11 → 20/08/11

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