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In the description of \emph{relative} motion in accelerated systems and gravitational fields, inertial and tidal accelerations must be taken into account, respectively. These involve a critical speed that in the first approximation can be simply illustrated in the case of motion in one dimension. For one-dimensional motion, such first-order accelerations are multiplied by , where is the critical speed. If the speed of relative motion exceeds , there is a sign reversal with consequences that are contrary to Newtonian expectations.

生成讲解博客的中文版本

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