万有引力常数G精确测量实验进展

刘建平; 邬俊飞; 黎卿; 薛超; 毛德凯; 杨山清; 邵成刚; 涂良成; 胡忠坤; 罗俊

doi:10.7498/aps.67.20181381

摘要

万有引力常数G是人类历史上引入的第一个基本物理学常数，其在理论物理、天体物理和地球物理等许多领域中扮演着重要角色.两百多年来，人们共测量出了200多个G值，但G的测量精度仍然是所有物理学常数中最差的，这一现象反映了测G工作本身的复杂性和困难性.本文简要概述了G值测量的意义和测G的历史，并结合自2010年以来国际上新出现的三个高精度测G实验介绍这一领域的研究进展，以及华中科技大学引力实验中心测G工作的最新动态.

关键词:

Abstract

The Newtonian gravitational constant G is the first fundamental physics constant introduced by human beings. It plays an important role in many fields, such as theoretical physics, astrophysics, and geophysics. Its precision measurement and related research is of great significance to the whole experimental physics. However, the measuring accuracy of G is the worst among all fundamental physical constants, which reflects the great complexity and difficulty in determining G. This paper briefly reviews the history of G measurement, and also introduces the current research progress in this field by a summary of the recent three precision measurements of G. At the end of the paper, the latest developments of the G measurement in the center of gravitational experiments at Huazhong University of Science and Technology are introduced.

Keywords:

作者及机构信息

1.
华中科技大学物理学院, 基本物理量测量教育部重点实验室, 引力与量子物理湖北省重点实验室, 武汉 430074;

2.
中山大学天琴引力物理研究中心, 珠海 519082

通信作者: 杨山清, ysq2011@hust.edu.cn;junluo@hust.edu.cn ; 罗俊, ysq2011@hust.edu.cn;junluo@hust.edu.cn

基金项目: 国家自然科学基金重大项目（批准号：91536223）和国家重点基础研究发展计划（批准号：2010CB832801）资助的课题.

Authors and contacts

1.
MOE Key Laboratory of Fundamental Physical Quantities Measurements, Hubei Key Laboratory of Gravitation and Quantum Physics, School of Physics, Huazhong University of Science and Technology, Wuhan 430074, China;

2.
TianQin Research Center for Gravitational Physics, Sun Yat-sen University, Zhuhai 519082, China

Corresponding author: Yang Shan-Qing, ysq2011@hust.edu.cn;junluo@hust.edu.cn ; Luo Jun, ysq2011@hust.edu.cn;junluo@hust.edu.cn

Funds: Project supported by the Major Research Plan of the National Natural Science Foundation of China (Grant No. 91536223) and the National Basic Research Program of China (Grant No. 2010CB832801).

参考文献

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施引文献

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[2]	Herrick S 1971 Astrodynamics: Orbit Determination, Space Navigation, Celestial Mechanics (Vol. I) (London: Van Nostrand Reinhold) pp127-163
[3]	Ries J C, Eanes R J, Shum C K, Watkin M M 1992 Geophys. Res. Lett. 19 529
[4]	Ezer D, Cameron A G W 1966 Can. J. Phys. 44 593
[5]	Tomilin K A 1999 Proceedings of the XXⅡ Workshop on High Energy Physics and Field Theory (CiteSeer)
[6]	Planck M 1990 Ann. Phys. 306 69
[7]	McQueen H W S 1981 Phys. Earth Planet Inter. 26 6
[8]	Dirac P A M 1937 Nature 139 323
[9]	Dirac P A M 1938 Roy. Soc. Lond. Proc. A 165 199
[10]	Dirac P A M 1974 Roy. Soc. Lond. Proc. A 338 439
[11]	Weinberg S 1989 Rev. Mod. Phys. 61 1
[12]	Brans C, Dicke R H 1961 Phys. Rev. 124 925
[13]	Hellings R W 1988 NATO Advanced Science Institute Series C 230 215
[14]	Massa C 1989 Helv. Phys. Act. 62 424
[15]	Long D R 1976 Nature 260 417
[16]	Eötvös R V, Pekar D, Fekete E 1922 Ann. Phys. (Leipz.) 68 11
[17]	Fischbach E, Sudarsky D, Szafer A, Talmadge C, Aronson S H 1986 Phys. Rev. Lett. 56 3
[18]	Fischbach E, Talmadge C 1992 Nature 356 207
[19]	Cook A H 1988 Rep. Prog. Phys. 51 707
[20]	Cavendish H 1798 Phil. Trans. R. Soc. Lond. 88 469
[21]	Gillies G T 1987 Metrologia 24(S) 1
[22]	Rothleitner C, Schlamminger S 2017 Rev. Sci. Instrum. 88 111101
[23]	Cohen E R, Taylor B N 1973 J. Phys. Chem. Ref. Data 2 663
[24]	Cohen E R, Taylor B N 1987 Rev. Mod. Phys. 59 1121
[25]	Mohr P J, Taylor B N 2000 Rev. Mod. Phys. 72 351
[26]	Mohr P J, Taylor B N 2005 Rev. Mod. Phys. 77 1
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[31]	Luther G G, Towler W R 1982 Phys. Rev. L 48 121
[32]	Karagioz O V, Izmailov V P 1996 Meas. Tech. 39 979
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[34]	Gundlach J H, Merkowitz S M 2000 Phys. Rev. Lett. 85 2869
[35]	Quinn T J, Speake C C, Richman S J, Davis R S, Picard A A 2001 Phys. Rev. Lett. 87 111101
[36]	Kleinevoß U 2002 Bestimmung der Newtonschen Gravitationskonstanten G Disertation for the Doctoral Degree (Wuppertald: University of Wuppertald)
[37]	Armstrong T R, Fitzgerald M P 2003 Phys. Rev. Lett. 91 201101
[38]	Hu Z K, Guo J Q, Luo J 2005 Phys. Rev. D 71 127505
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[40]	Luo J, Liu Q, Tu L C, Shao C G, Liu L X, Yang S Q, Li Q, Zhang Y T 2009 Phys. Rev. Lett. 102 240801
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[42]	Parks H V, Faller J E 2010 Phys. Rev. Lett. 105 110801
[43]	Quinn T J, Parks H V, Speake C C, Davis R S 2013 Phys. Rev. Lett. 111 101102
[44]	Rosi G, Sorrentino F, Cacciapuoti L, Prevedelli M, Tino G M 2014 Nature 510 518
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[46]	Schlamminger S, Holzschuh E, Kndig W 2002 Phys. Rev. Lett. 89 161102
[47]	Tu L C, Li Q, Shao C G, Hu Z K, Luo J 2011 Sci. Sin. Phys. Mech. Astron. 41 691 (in Chinese) [涂良成, 黎卿, 邵成刚, 胡忠坤, 罗俊 2011 中国科学: 物理学力学天文学 41 691]
[48]	Gillies G T, Ritter T C 1993 Rev. Sci. Instrum. 64 283
[49]	Quinn T, Speake C, Parks H, Davis R 2014 Phil. Trans. R. Soc. A 372 20140032
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[52]	Heyl P R 1930 J. Res. Natl. Bur. Stand. 5 1243
[53]	Heyl P R, Chrzanowski P A 1942 J. Res. Natl. Bur. Stand. 29 1
[54]	Kuroda, K 1995 Phys. Rev. Lett. 75 2796
[55]	Newman R D, Bantel M K 1999 Meas. Sci. Technol. 10 445
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[58]	Yang S Q, Tu L C, Shao C G, Li Q, Wang Q L, Zhou Z B, Luo J 2009 Phys. Rev. D 80 122005
[59]	Kasevich M, Chu S 1991 Phys. Rev. Lett. 67 181
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[67]	Numata K, Horowitz J, Camp, J 2007 Phys. Lett. A 370 91
[68]	Fan X D, Liu Q, Liu L X, Milyukov V, Luo J 2008 Phys. Lett. A 372 547
[69]	Gundlach J H, Adelberger E G, Heckel B R, Swanson H E 1996 Phys. Rev. D 54 R1256
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[73]	Quan L D, Xue C, Shao C G, Yang S Q, Tu L C, Wang Y J, Luo J 2014 Rev. Sci. Instrum. 85 014501
[74]	https://www.bipm.org/utils/en/pdf/CIPM/CIPM2014-Ⅱ-Decisions-EN.pdf [2014-12-10]

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