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It is also known as the Laplace vector, [13] [14] the Runge–Lenz vector [15] and the Lenz vector. [8] Ironically, none of those scientists discovered it. [ 15 ] The LRL vector has been re-discovered and re-formulated several times; [ 15 ] for example, it is equivalent to the dimensionless eccentricity vector of celestial mechanics .
If is a vector (a tensor of first degree), the gradient is a covariant derivative which results in a tensor of second degree, and the divergence of this is again a vector. The formula for the vector Laplacian above may be used to avoid tensor math and may be shown to be equivalent to the divergence of the Jacobian matrix shown below for the ...
In mathematics and physics, Laplace's equation is a second-order partial differential equation named after Pierre-Simon Laplace, who first studied its properties.This is often written as = or =, where = = is the Laplace operator, [note 1] is the divergence operator (also symbolized "div"), is the gradient operator (also symbolized "grad"), and (,,) is a twice-differentiable real-valued function.
The Laplace–Beltrami operator acting on a function is given by the ... Note that this transformation formula is for the mean curvature vector, ...
In the anisotropic case where the coefficient matrix A is not scalar and/or if it depends on x, then an explicit formula for the solution of the heat equation can seldom be written down, though it is usually possible to consider the associated abstract Cauchy problem and show that it is a well-posed problem and/or to show some qualitative ...
The Hodge Laplacian, also known as the Laplace–de Rham operator, is a differential operator acting on differential forms. (Abstractly, it is a second order operator on each exterior power of the cotangent bundle .)
However, the converse is not true; not every vector field that satisfies Laplace's equation is a Laplacian vector field, which can be a point of confusion. For example, the vector field v = ( x y , y z , z x ) {\displaystyle {\bf {v}}=(xy,yz,zx)} satisfies Laplace's equation, but it has both nonzero divergence and nonzero curl and is not a ...
The apsides are the two points of closest and furthest distance of the orbit (the periapsis and apoapsis, respectively); apsidal precession corresponds to the rotation of the line joining the apsides. It also corresponds to the rotation of the Laplace–Runge–Lenz vector, which points along the line of apsides.