• DocumentCode
    3428660
  • Title

    Laser-cooled microgravity clocks

  • Author

    Gibble, Kurt

  • Author_Institution
    Yale Univ., New Haven, CT, USA
  • fYear
    1998
  • fDate
    27-29 May 1998
  • Firstpage
    41
  • Lastpage
    45
  • Abstract
    The principle advantage of microgravity for atomic clocks is interrogation times longer than 1 s. With a 10 s interrogation time, a clock has a 50 mHz linewidth suggesting that accuracies may potentially exceed 10-16. However, to achieve greater accuracy within the same averaging time, greater stability is needed. Achieving greater stability in a microgravity clock constrains the design differently than for earth based fountains. In this paper, we discuss the design considerations for laser-cooled microgravity clocks highlighting the considerations that differ from those for earth-based fountains. As in earthbased fountains, the frequency shift due to cold collisions plays an important role in the design of the clock. Given our predictions (and measurements) for the shift in laser-cooled Rb clocks, we currently anticipate building a high performance Rb clock and discuss the relative merits of Rb and Cs microgravity clocks. Finally, we present our tentative designs for two microgravity clocks
  • Keywords
    atomic clocks; caesium; laser cooling; rubidium; space vehicle electronics; zero gravity experiments; 1 s; 10 s; Cs; Cs microgravity clocks; Rb; Rb microgravity clocks; atomic clocks; cold collisions; frequency shift; interrogation time; laser-cooled Rb clocks; Atom lasers; Atom optics; Atomic beams; Clocks; Frequency; Laser beams; Laser stability; Laser transitions; Masers; Optical scattering;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Frequency Control Symposium, 1998. Proceedings of the 1998 IEEE International
  • Conference_Location
    Pasadena, CA
  • ISSN
    1075-6787
  • Print_ISBN
    0-7803-4373-5
  • Type

    conf

  • DOI
    10.1109/FREQ.1998.717877
  • Filename
    717877