Fluorescence Detection and Buffer Gas Cooling of Trapped Mercury Ions in Paul Trap
SHE Lei1,2,3, WANG Wen-Ming1,2,3, BAI Lei1,2,3, SUN Huan-Yao1,2,3, ZHU Xi-Wen1,2, LI Jiao-Mei1,2, GAO Ke-Lin 1,2
1State Key Laboratory of Magnetic Resonance and Atomic and Molecular Physics, Wuhan Institute of Physics and Mathematics, Chinese Academy of Sciences, Wuhan 4300712Center for Cold Atom Physics, Chinese Academy of Sciences, Wuhan 430071 3Graduate School of Chinese Academy of Sciences, Beijing 100080
Fluorescence Detection and Buffer Gas Cooling of Trapped Mercury Ions in Paul Trap
SHE Lei1,2,3;WANG Wen-Ming1,2,3;BAI Lei1,2,3;SUN Huan-Yao1,2,3;ZHU Xi-Wen1,2;LI Jiao-Mei1,2;GAO Ke-Lin 1,2
1State Key Laboratory of Magnetic Resonance and Atomic and Molecular Physics, Wuhan Institute of Physics and Mathematics, Chinese Academy of Sciences, Wuhan 4300712Center for Cold Atom Physics, Chinese Academy of Sciences, Wuhan 430071 3Graduate School of Chinese Academy of Sciences, Beijing 100080
摘要Hg ions are confined in a hyperboloid ion trap. With the rf discharge 202Hg isotope lamp, the fluorescence signal of trapped Hg ions is observed. By means of buffer gas cooling, the ionic temperature is reduced. As a result, the trapping time is increased and the signal-to-noise ratio (SNR) of the fluorescent signal is improved. The temperature of ion cloud is estimated by measuring the space charge shift.
Abstract:Hg ions are confined in a hyperboloid ion trap. With the rf discharge 202Hg isotope lamp, the fluorescence signal of trapped Hg ions is observed. By means of buffer gas cooling, the ionic temperature is reduced. As a result, the trapping time is increased and the signal-to-noise ratio (SNR) of the fluorescent signal is improved. The temperature of ion cloud is estimated by measuring the space charge shift.
SHE Lei;;WANG Wen-Ming;;BAI Lei;;SUN Huan-Yao;;ZHU Xi-Wen;LI Jiao-Mei;GAO Ke-Lin;. Fluorescence Detection and Buffer Gas Cooling of Trapped Mercury Ions in Paul Trap[J]. 中国物理快报, 2008, 25(5): 1653-1656.
SHE Lei, , WANG Wen-Ming, , BAI Lei, , SUN Huan-Yao, , ZHU Xi-Wen, LI Jiao-Mei, GAO Ke-Lin,. Fluorescence Detection and Buffer Gas Cooling of Trapped Mercury Ions in Paul Trap. Chin. Phys. Lett., 2008, 25(5): 1653-1656.
[1] Blatt R, Schnatz H and werth G 1983 Z. Phys. A 312 143 [2] Dick R H 1953 Phys. Rev. 89 472 [3] Werth G 1986 Metrologia 22 190 [4] Major F G and Werth G 1973 Phys. Rev. Lett. 23 1155 [5] Jardino M, Desainfuscien M, Barillet R, Viennet J, Petit P andAudoin C 1981 Appl. Phys. 24 107 [6] Culter L S, Giffard R P, Wheeler P J and Winkler G 1987 Proceedings of the 41st Annual Frequency Control Symposium(Philadelphia 27--29 May 1987) p 12 [7] Prestage J D, Dick G J and Maleki L 1987 Proceedings of the 41st Annual Frequency Control Symposium(Philadelphia 27--29 May 1987) p 21 [8] Tjoelker R L, Prestage J D, Koppang P and Swanson T 2003 Joint Meeting EFTF and IEEE IFCS (Tampa 5--8 May 2003) p1066 [9] Prestage J D, Chung S, Le T, Lim L and Maleki L 2005 Frequency Control Symposium and Exposition, Proceedings ofthe 2005 IEEE International (Vancouver 29--31 August 2005) p 472 [10] Culter L S, Flory C A, Giffard R P and McGuire M D 1986 Appl.Phys. B 39 251 [11] Culter L S, Giffard R P and McGuire M D 1985 Appl. Phys. B 36 137 [12] Bitter F, Davis S P, Richter B and Young J E R 1954 Phys.Rev. 96 1531 [13] ehmelt H G D 1967 Adv. At. Mol. Phys. 3 53 [14] Culter L S, Giffard R P and McGuire M D 1983 Proceedings of the 37th Frequency Control Symposium (Philadelphia1--3 June 1983) p 32 [15] Schaaf H, Schmeling V and Werth G 1981 Appl. Phys. 25249 [16] Shu H L, Guan H, Huang X R, LI J M and Gao K L 2005 Chin. Phys.Lett. 22 1641 [17] Dehmelt H G 1969 Adv. At. Mol. Phys. 5 109 [18] Sheretov E P, Zenkin V A and Samodurov Y F 1973 Sov. Phys.Tech. Phys. 18 2 [19] Gaboriaud M N, Desainfuscien M and Major F G 1981 Int. J. Mass Spectrom. Ion Phys. 41 109 [20] Schuessler H A, Holder C H and Jr. 1979 J. Appl. Phys. 50 5110 [21] Blatt R, Zoller P, Holzmuller G and Siemers I 1986 Z.Phys. D 4 121