The Gravitational Tidal Tensor, derived from the negative second spatial derivatives of the gravitational potential, describes the differential acceleration experienced by two adjacent particles in a gravitational field. This tensor is fundamental to understanding tidal effects, as it relates the change in acceleration linearly to the particle separation vector. Notably, the tensor is symmetric and, for a spherical mass distribution, its components reveal the dual nature of tidal forces: the off-diagonal terms are responsible for the shearing and stretching effects lateral to the mass center, while the diagonal terms govern the radial compression and stretching along the line of centers.
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Properties and Physical Effects of the Gravitational Tidal Tensor.mp4
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