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Web (differential geometry)
From Wikipedia, the free encyclopedia
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In mathematics, a web permits an intrinsic characterization in terms of Riemannian geometry of the additive separation of variables in the Hamilton–Jacobi equation.[1][2]
Formal definition
Summarize
Perspective
An orthogonal web (also called an orthogonal grid or Ricci grid) on a Riemannian manifold (M,g) of dimension n is a set of n pairwise transversal and orthogonal foliations of connected submanifolds of codimension 1.[3] Note that two submanifolds of codimension 1 are orthogonal iff their normal vectors are orthogonal, and that in the case of a nondefinite metric, orthogonality does not imply transversality.
Remark
Since vector fields can be visualized as stream-lines of a stationary flow or as Faraday’s lines of force, a non-vanishing vector field in space generates a space-filling system of lines through each point, known to mathematicians as a congruence (i.e., a local foliation). Ricci’s idea was to fill an n-dimensional Riemannian manifold with n congruences orthogonal to each other, i.e., a local orthogonal grid.
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Differential geometry of webs
A systematic study of webs was started by Blaschke in the 1930s. He extended the same group-theoretic approach to web geometry.
Classical definition
Let be a differentiable manifold of dimension N=nr. A d-web W(d,n,r) codimension r in an open set is a set of d foliations of codimension r which are in general position.
In the notation W(d,n,r) the number d is the number of foliations forming a web, r is the web codimension, and n is the ratio of the dimension nr of the manifold M and the web codimension. Of course, one may define a d-web of codimension r without having r as a divisor of the dimension of the ambient manifold.
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See also
Notes
References
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