An absolute calibration system for millimeter-accuracy APOLLO measurements

被引:14
作者
Adelberger, E. G. [1 ]
Battat, J. B. R. [2 ]
Birkmeier, K. J. [3 ]
Colmenares, N. R. [4 ]
Davis, R. [4 ]
Hoyle, C. D. [5 ]
Huang, L. R. [2 ]
McMillan, R. J. [6 ]
Murphy, T. W., Jr. [4 ]
Schlerman, E. [2 ]
Skrobol, C. [3 ]
Stubbs, C. W. [7 ]
Zach, A. [3 ]
机构
[1] Univ Washington, Ctr Expt Nucl Phys & Astrophys, Box 354290, Seattle, WA 98195 USA
[2] Wellesley Coll, Dept Phys, 106 Cent St, Wellesley, MA 02481 USA
[3] TOPTICA Photon AG, Lochhamer Schlag 19, D-82166 Graefelfing Munich, Germany
[4] Univ Calif San Diego, Ctr Astrophys & Space Sci, 9500 Gilman Dr, La Jolla, CA 92093 USA
[5] Humboldt State Univ, Dept Phys & Astron, One Harpst St, Arcata, CA 95521 USA
[6] Apache Point Observ, 2001 Apache Point Rd, Sunspot, NM 88349 USA
[7] Harvard Univ, Dept Phys, 17 Oxford St, Cambridge, MA 02318 USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
lunar laser ranging; experimental gravity; calibration; frequency standard; SESAM laser; LASER-RANGING OPERATION; EQUIVALENCE PRINCIPLE; MOON; RELATIVITY;
D O I
10.1088/1361-6382/aa953b
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Lunar laser ranging provides a number of leading experimental tests of gravitation-important in our quest to unify general relativity and the standard model of physics. The apache point observatory lunar laser-ranging operation (APOLLO) has for years achieved median range precision at the similar to 2 mm level. Yet residuals in model-measurement comparisons are an order-of-magnitude larger, raising the question of whether the ranging data are not nearly as accurate as they are precise, or if the models are incomplete or ill-conditioned. This paper describes a new absolute calibration system (ACS) intended both as a tool for exposing and eliminating sources of systematic error, and also as a means to directly calibrate ranging data in situ. The system consists of a high-repetition-rate (80 MHz) laser emitting short (<10 ps) pulses that are locked to a cesium clock. In essence, the ACS delivers photons to the APOLLO detector at exquisitely well-defined time intervals as a 'truth' input against which APOLLO's timing performance may be judged and corrected. Preliminary analysis indicates no inaccuracies in APOLLO data beyond the similar to 3 mm level, suggesting that historical APOLLO data are of high quality and motivating continued work on model capabilities. The ACS provides the means to deliver APOLLO data both accurate and precise below the 2 mm level.
引用
收藏
页数:19
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