Measurement of the Fundamental Thermal Noise Limit in a Cryogenic Sapphire Frequency Standard Using Bimodal Maser Oscillations

Karim Benmessai, Daniel Lloyd Creedon, Michael Edmund Tobar, Pierre-Yves Bourgeois, Yann Kersalé, and Vincent Giordano
Phys. Rev. Lett. 100, 233901 – Published 9 June 2008

Abstract

We report observations of the Schawlow-Townes noise limit in a cryogenic sapphire secondary frequency standard. The effect causes a fundamental limit to the frequency stability, and was measured through the novel excitation of a bimodal maser oscillation of a Whispering Gallery doublet at 12.04 GHz. The beat frequency of 10 kHz between the oscillations enabled a sensitive probe for this measurement of fractional frequency instability of 1014τ1/2 with only 0.5 pW of output power.

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  • Received 20 March 2008

DOI:https://doi.org/10.1103/PhysRevLett.100.233901

©2008 American Physical Society

Authors & Affiliations

Karim Benmessai1, Daniel Lloyd Creedon2, Michael Edmund Tobar2,*, Pierre-Yves Bourgeois1,2, Yann Kersalé1,†, and Vincent Giordano1

  • 1Institut FEMTO-ST, UMR 6174 CNRS, Université de Franche, Comté, 25044 Besançon, France
  • 2University of Western Australia, School of Physics M013, 35 Stirling Hwy., Crawley 6009 WA, Australia

  • *mike@physics.uwa.edu.au
  • yann.kersale@femto-st.fr

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Vol. 100, Iss. 23 — 13 June 2008

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