Accuracy estimations of overtone vibrational transition frequencies of optically trapped 174Yb6Li molecules
被引:19
作者:
Kajita, Masatoshi
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机构:
Natl Inst Informat & Commun Technol, Koganei, Tokyo 1848795, JapanNatl Inst Informat & Commun Technol, Koganei, Tokyo 1848795, Japan
Kajita, Masatoshi
[1
]
Gopakumar, Geetha
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机构:
Tokyo Metropolitan Univ, Dept Chem, Hachioji, Tokyo 1920397, JapanNatl Inst Informat & Commun Technol, Koganei, Tokyo 1848795, Japan
Gopakumar, Geetha
[2
]
Abe, Minori
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机构:
Tokyo Metropolitan Univ, Dept Chem, Hachioji, Tokyo 1920397, JapanNatl Inst Informat & Commun Technol, Koganei, Tokyo 1848795, Japan
Abe, Minori
[2
]
Hada, Masahiko
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机构:
Tokyo Metropolitan Univ, Dept Chem, Hachioji, Tokyo 1920397, JapanNatl Inst Informat & Commun Technol, Koganei, Tokyo 1848795, Japan
Hada, Masahiko
[2
]
机构:
[1] Natl Inst Informat & Commun Technol, Koganei, Tokyo 1848795, Japan
[2] Tokyo Metropolitan Univ, Dept Chem, Hachioji, Tokyo 1920397, Japan
来源:
PHYSICAL REVIEW A
|
2012年
/
85卷
/
06期
关键词:
RATIO;
D O I:
10.1103/PhysRevA.85.062519
中图分类号:
O43 [光学];
学科分类号:
070207 ;
0803 ;
摘要:
The attainable accuracy of the X-2 Sigma(v, N) = (0,0) --> (v(u), 0) transition frequencies of optically trapped (YbLi)-Yb-174-Li-6 molecules are analyzed (v(u) = 1,2,3,4) to test the variation in the proton-to-electron mass ratio. We eliminate the Stark shifts induced by the trap and Raman lasers by choosing appropriate frequencies (magic frequencies). For v(u) = 1 and 2, we obtain more than one experimentally useful magic frequency, thereby leading to more choice in the trap laser. For v(u) = 3 and 4, the choice in the trap laser is limited. The systematic frequency uncertainty is given by the trap laser frequency detuning from the magic frequency and the fluctuation of the power ratio of the two Raman lasers and can be lower than 10(-16) for all these transition frequencies. To obtain lower statistical uncertainty, measurement with v(u) = 4 is more advantageous than that with v(u) = 1 - 3.
机构:
Natl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Univ Colorado, Boulder, CO 80309 USANatl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Zelevinsky, T.
Kotochigova, S.
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机构:
Temple Univ, Dept Phys, Philadelphia, PA 19122 USANatl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Kotochigova, S.
Ye, Jun
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机构:
Natl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Univ Colorado, Boulder, CO 80309 USANatl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
机构:
Natl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Univ Colorado, Boulder, CO 80309 USANatl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Zelevinsky, T.
Kotochigova, S.
论文数: 0引用数: 0
h-index: 0
机构:
Temple Univ, Dept Phys, Philadelphia, PA 19122 USANatl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Kotochigova, S.
Ye, Jun
论文数: 0引用数: 0
h-index: 0
机构:
Natl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA
Univ Colorado, Boulder, CO 80309 USANatl Inst Stand & Technol, Joint Inst Lab Astrophys, Boulder, CO 80309 USA