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
Link To Document