Observation of Faraday Rotation in Cold Atoms in an Integrating Sphere
The Faraday rotation of weak linearly polarized probe light is observed as it passes through a sample of cold ^87Rb atoms prepared by diffused light in an integrating sphere. The rotation angle of the probe light-polarization as functions of laser intensity, detuning and biased magnetic field is mea...
Saved in:
Published in | Chinese physics letters Vol. 31; no. 7; pp. 81 - 84 |
---|---|
Main Author | |
Format | Journal Article |
Language | English |
Published |
01.07.2014
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | The Faraday rotation of weak linearly polarized probe light is observed as it passes through a sample of cold ^87Rb atoms prepared by diffused light in an integrating sphere. The rotation angle of the probe light-polarization as functions of laser intensity, detuning and biased magnetic field is measured. A Ramsey fringe with a linewidth of 35 Hz and contrast up to 92% is demonstrated. This method has potential applications in improving the performance of atomic clocks with cold atoms. |
---|---|
Bibliography: | The Faraday rotation of weak linearly polarized probe light is observed as it passes through a sample of cold ^87Rb atoms prepared by diffused light in an integrating sphere. The rotation angle of the probe light-polarization as functions of laser intensity, detuning and biased magnetic field is measured. A Ramsey fringe with a linewidth of 35 Hz and contrast up to 92% is demonstrated. This method has potential applications in improving the performance of atomic clocks with cold atoms. 11-1959/O4 ZHENG Ben-Chang, CHENG Hua-Dong., MENG Yan-Ling, XIAO Ling, WAN Jin-Yin, LIU Liang( 1Key Laboratory of Quantum Optics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Shanghai 201899 ;2 Key Laboratory of Atomic Frequency Standards, Wuhan Institute of Physics and Mathematics Chinese Academy of Sciences, Wuhan 430071) ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0256-307X 1741-3540 |
DOI: | 10.1088/0256-307X/31/7/073701 |