The three-fold theoretical basis of the Gravity Probe B gyro precession calculation

被引:12
作者
Adler, Ronald J. [1 ,2 ,3 ]
机构
[1] Stanford Univ, Hansen Expt Phys Lab, Grav Probe B Mission, Stanford, CA 94309 USA
[2] San Francisco State Univ, Dept Phys & Astron, San Francisco, CA 94132 USA
[3] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94035 USA
关键词
Gravity Probe B; general relativity; gravito-magnetism; GENERAL-RELATIVITY; SPIN;
D O I
10.1088/0264-9381/32/22/224002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Gravity Probe B (GP-B) experiment is complete and the results are in agreement with the predictions of general relativity (GR) for both the geodetic precession, 6.6 arcsec yr(-1) to about 0.3%, and the Lense-Thirring precession, 39 marcsec to about 19%. This note is concerned with the theoretical basis for the predictions. The predictions depend on three elements of gravity theory, firstly that macroscopic gravity is described by a metric theory such as GR, secondly that the Lense-Thirring metric provides an approximate description of the gravitational field of the spinning Earth, and thirdly that the spin axis of a gyroscope is parallel displaced in spacetime, which gives its equation of motion. We look at each of these three elements to show how each is solidly based on previous experiments and well-tested theory. The agreement of GP-B with theory strengthens our belief that all three elements are correct and increases our confidence in applying GR to astrophysical phenomena. Conversely, if GP-B had not verified the predictions a major theoretical quandary would have occurred.
引用
收藏
页数:13
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