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199Hg+光频标的黑体辐射频移

刘李辉 邹宏新 刘曲 李玺

199Hg+光频标的黑体辐射频移

刘李辉, 邹宏新, 刘曲, 李玺
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  • 光学频率标准会受到环境温度的黑体辐射影响发生频移,进而影响其准确度. 本文估算了199Hg+的超精细能级5d106s2S1/2 (F=0)和5d96s2 2D5/2 (F=2)的极化率,得到了室温(300 K)下黑体辐射引起的相对频移为-5.410-17, 最后讨论了低温环境下黑体辐射对199Hg+光频标的影响.
    • 基金项目: 国家自然科学基金(批准号: 10904174)和湖南省自然科学基金(批准号: 11JJ2004)资助的课题.
    [1]

    Bender P L, Hall J L, Garstang R H, Pichanick F M J, Smith W W, Barger R L, West B J 1976 Bull. Am. Phys. Soc. 21 599

    [2]

    Rosenband T, Hume C W, Chou D B, Brusch A, Lorini L, Oskay W H, Drullinger R E, Fortier T M, Stalnaker J E, Diddams S A, Swann W C, Newbury N R, Itano W M, Wineland D J, Bergquist J C 2008 Science 319 1808

    [3]

    Mowat J R 1972 Phys. Rev. A 5 1059

    [4]

    Simon E, Laurent P, Clairon A 1998 Phys. Rev. A 57 426

    [5]

    Gao W, Ke X Z, Liu H F 2000 Acta Opt. Sin. 20 3 (in Chinese) [高卫, 柯熙政, 刘海峰 2000 光学学报 20 3]

    [6]

    Godone A, Calonico D, Levi F, Micalizio S, Calosso C 2005 Phys. Rev. A 71 063401

    [7]

    Angstmann E J, Dzuba V A, Flambaum V V 2006 Phys. Rev. A 74 023405

    [8]

    Beloy K, Safronova U I, Derevianko A 2006 Phys. Rev. Lett. 97 040801

    [9]

    Angstmann E J, Dzuba V A, Flambaum V 2006 Phys. Rev. Lett. 97 040802

    [10]

    Vanier J, Mandache C 2007 Appl. Phys. B 87 565

    [11]

    Farley J W, Wing W H 1981 Phys. Rev. A 23 2397

    [12]

    Safronova M S, Jiang D S, Safronova U I 2010 Phys. Rev. A 82 022510

    [13]

    Safronova U I 2010 Phys. Rev. A 82 022504

    [14]

    Safronova U I 2010 Phys. Rev. A 81 052506

    [15]

    Berengut J C, Flambaum V V, Lacroix J K 2009 Phys. Rev. A 80 064101

    [16]

    Safronova U I, Safronova M S 2009 Phys. Rev. A 79 022512

    [17]

    Porsev S G, Derevianko A 2006 Phys. Rev. A 74 020502

    [18]

    Rosenband T, Itano W M, Schmidt P O, Hume D B, Koelemeij J C J, Bergquist J C, Wineland D J 2006 Proceedings of the 20th EFTF, Braunschweig, Germany, 27-30, March 2006 pp289-292

    [19]

    Arora B, Safronova M S, Clark C 2007 Phys. Rev. A 76 064501

    [20]

    Safronova M S, Johnson W R 2007 Adv. at. Mol. Opt. Phys. 55 191

    [21]

    Hachisu H, Miyagishi K, Porsev S G, Derevianko A, Ovsiannikov V D, Palchikov V G, Takamoto M, Katori H 2008 Phys. Rev. Lett. 100 053001

    [22]

    Jiang D S, Arora B, Safronova M S, Clark C W 2009 J. Phys. B: Mol. Opt. Phys. 42 154020

    [23]

    Kallay M, Nataraj H S, Sahoo B K, Das B P, Visscher L 2011 Phys. Rev. A 83 030503

    [24]

    Folcke N, Bartlett R J 2004 J. Chem. Phys. 121 22

    [25]

    Zhou S X 1979 Quantum Mechanics (Beijing: Higher Education Press) p5 (in Chinese) [周世勋 1979 量子力学教程(北京:高等教育出版社) 第5页]

    [26]

    Bize S, Diddams S A, Tanaka U, Tanner C E, Oskay W H, Drullinger R E, Parker T E, Heavner T P, Jefferts S R, Hollberg L, Itano W M, Bergquist J C 2003 Phys. Rev. Lett. 90 150802

    [27]

    Itano W M 2000 J. Res. Natl. Inst. Stand. Technol. 105 829

    [28]

    Sansonetti C J, Joseph R 2001 Phys. Scripta 63 219

    [29]

    Becker T, Zanthier J V, Nevsky A Y, Schwedes C, Skvortsov M N, Walther H, Peik E 2001 Phys. Rev. A 63 051802

    [30]

    Hosaka K, Webster S A, Stannard A, Walton B R, Margolis H S, Gill P 2009 Phys. Rev. A 79 033403

    [31]

    Lorini L, Ashby N, Brusch A, Diddams S, Drullinger, Eason E, Fortier T, Hastings P, Heavner T, Hume D,Itano W, Jefferts S, Newbury N, Parker T, Rosenband T, Stalnaker J, Swann W, Wineland D, Bergquist J 2008 Eur. Phys. J. Special Topics 163 19

  • [1]

    Bender P L, Hall J L, Garstang R H, Pichanick F M J, Smith W W, Barger R L, West B J 1976 Bull. Am. Phys. Soc. 21 599

    [2]

    Rosenband T, Hume C W, Chou D B, Brusch A, Lorini L, Oskay W H, Drullinger R E, Fortier T M, Stalnaker J E, Diddams S A, Swann W C, Newbury N R, Itano W M, Wineland D J, Bergquist J C 2008 Science 319 1808

    [3]

    Mowat J R 1972 Phys. Rev. A 5 1059

    [4]

    Simon E, Laurent P, Clairon A 1998 Phys. Rev. A 57 426

    [5]

    Gao W, Ke X Z, Liu H F 2000 Acta Opt. Sin. 20 3 (in Chinese) [高卫, 柯熙政, 刘海峰 2000 光学学报 20 3]

    [6]

    Godone A, Calonico D, Levi F, Micalizio S, Calosso C 2005 Phys. Rev. A 71 063401

    [7]

    Angstmann E J, Dzuba V A, Flambaum V V 2006 Phys. Rev. A 74 023405

    [8]

    Beloy K, Safronova U I, Derevianko A 2006 Phys. Rev. Lett. 97 040801

    [9]

    Angstmann E J, Dzuba V A, Flambaum V 2006 Phys. Rev. Lett. 97 040802

    [10]

    Vanier J, Mandache C 2007 Appl. Phys. B 87 565

    [11]

    Farley J W, Wing W H 1981 Phys. Rev. A 23 2397

    [12]

    Safronova M S, Jiang D S, Safronova U I 2010 Phys. Rev. A 82 022510

    [13]

    Safronova U I 2010 Phys. Rev. A 82 022504

    [14]

    Safronova U I 2010 Phys. Rev. A 81 052506

    [15]

    Berengut J C, Flambaum V V, Lacroix J K 2009 Phys. Rev. A 80 064101

    [16]

    Safronova U I, Safronova M S 2009 Phys. Rev. A 79 022512

    [17]

    Porsev S G, Derevianko A 2006 Phys. Rev. A 74 020502

    [18]

    Rosenband T, Itano W M, Schmidt P O, Hume D B, Koelemeij J C J, Bergquist J C, Wineland D J 2006 Proceedings of the 20th EFTF, Braunschweig, Germany, 27-30, March 2006 pp289-292

    [19]

    Arora B, Safronova M S, Clark C 2007 Phys. Rev. A 76 064501

    [20]

    Safronova M S, Johnson W R 2007 Adv. at. Mol. Opt. Phys. 55 191

    [21]

    Hachisu H, Miyagishi K, Porsev S G, Derevianko A, Ovsiannikov V D, Palchikov V G, Takamoto M, Katori H 2008 Phys. Rev. Lett. 100 053001

    [22]

    Jiang D S, Arora B, Safronova M S, Clark C W 2009 J. Phys. B: Mol. Opt. Phys. 42 154020

    [23]

    Kallay M, Nataraj H S, Sahoo B K, Das B P, Visscher L 2011 Phys. Rev. A 83 030503

    [24]

    Folcke N, Bartlett R J 2004 J. Chem. Phys. 121 22

    [25]

    Zhou S X 1979 Quantum Mechanics (Beijing: Higher Education Press) p5 (in Chinese) [周世勋 1979 量子力学教程(北京:高等教育出版社) 第5页]

    [26]

    Bize S, Diddams S A, Tanaka U, Tanner C E, Oskay W H, Drullinger R E, Parker T E, Heavner T P, Jefferts S R, Hollberg L, Itano W M, Bergquist J C 2003 Phys. Rev. Lett. 90 150802

    [27]

    Itano W M 2000 J. Res. Natl. Inst. Stand. Technol. 105 829

    [28]

    Sansonetti C J, Joseph R 2001 Phys. Scripta 63 219

    [29]

    Becker T, Zanthier J V, Nevsky A Y, Schwedes C, Skvortsov M N, Walther H, Peik E 2001 Phys. Rev. A 63 051802

    [30]

    Hosaka K, Webster S A, Stannard A, Walton B R, Margolis H S, Gill P 2009 Phys. Rev. A 79 033403

    [31]

    Lorini L, Ashby N, Brusch A, Diddams S, Drullinger, Eason E, Fortier T, Hastings P, Heavner T, Hume D,Itano W, Jefferts S, Newbury N, Parker T, Rosenband T, Stalnaker J, Swann W, Wineland D, Bergquist J 2008 Eur. Phys. J. Special Topics 163 19

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  • 收稿日期:  2011-09-01
  • 修回日期:  2012-05-28
  • 刊出日期:  2012-05-05

199Hg+光频标的黑体辐射频移

  • 1. 国防科学技术大学理学院, 长沙 410073
    基金项目: 

    国家自然科学基金(批准号: 10904174)和湖南省自然科学基金(批准号: 11JJ2004)资助的课题.

摘要: 光学频率标准会受到环境温度的黑体辐射影响发生频移,进而影响其准确度. 本文估算了199Hg+的超精细能级5d106s2S1/2 (F=0)和5d96s2 2D5/2 (F=2)的极化率,得到了室温(300 K)下黑体辐射引起的相对频移为-5.410-17, 最后讨论了低温环境下黑体辐射对199Hg+光频标的影响.

English Abstract

参考文献 (31)

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