Abstract
A pedagogical derivation is given of the Lense-Thirring effect using basic notions from the motion of point particles and light rays. First, the notion of rotation is introduced using the properties of light rays only. Second, two realizations for a non- rotating propagation of space-like directions are presented: the gyroscope and the spin of elementary particles. Then the gravitational field around a rotating body is specified which is taken for determining the various effects connected with a point particle or a gyroscope: the deSitter precession (geodesic precession) and the Lense-Thirring effect (‘frame dragging’). The results are applied to the precession of gyroscopes and to the motion of satellites around the earth.
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Lämmerzahl, C., Neugebauer, G. (2001). The Lense—Thirring Effect: From the Basic Notions to the Observed Effects. In: Lämmerzahl, C., Everitt, C.W.F., Hehl, F.W. (eds) Gyros, Clocks, Interferometers...: Testing Relativistic Graviy in Space. Lecture Notes in Physics, vol 562. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-40988-2_3
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