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In the context of General Relativity, the democratic principle allows quick, order-of-magnitude calculations for the strength of gravitomagnetic effects such as frame-dragging. While the principle is fairly intuitive, it does not have a rigorous mathematical definition. ''John Wheeler (1990) on the practical application of Mach's principle to experiment (pp.232-233):'' :: "It is not necessary to enter into the mathematics of the theory to state its simple consequence ... Each mass has an "inertia-contributing" power, a voting power, equal to its mass, there, divided by the distance from ''there'' to ''here''. " According to the general principle of relativity, rotation is a ''relative'' property, and a state of motion that a satellite senses as being "absolutely non-rotating" is a ''local'' state, dictated partly by the relative rotation of the background stars, but also partly by the rotation of the body that the satellite orbits. Applying the democratic principle, we can calculate the influence of these two rotations on the satellite by calculating the relative contributions of these two collections of massenergy to the background gravitational field strength at the satellite's location, and then weighting their contributions on the satellite's "sense of rotation" accordingly. ==See also== * Mach's principle * Gravitoelectromagnetism * General relativity 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Democratic principle」の詳細全文を読む スポンサード リンク
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