Holonomic basis
In mathematics and mathematical physics, a coordinate basis or holonomic basis for a differentiable manifold M is a set of basis vector fields {eα} defined at every point P of a region of the manifold as
where s is the infinitesimal displacement vector between the point P and a nearby point Q whose coordinate separation from P is δxα along the coordinate curve xα (i.e. the curve on the manifold through P for which the local coordinate xα varies and all other coordinates are constant).[1]
It is possible to make an association between such a basis and directional derivative operators. Given a parameterized curve C on the manifold defined by xα(λ) with the tangent vector u = uαeα, where uα = dxα/dλ, and a function f(xα) defined in a neighbourhood of C, the variation of f along C can be written as
Since we have that u = uαeα, the identification is often made between a coordinate basis vector eα and the partial derivative operator ∂/∂xα, under the interpretation of all vector relations as equalities between operators acting on scalar quantities.[2]
A local condition for a basis {ek} to be holonomic is that all mutual Lie derivatives vanish:[3]
A basis that is not holonomic is called a non-holonomic or non-coordinate basis.
It is in general not possible to find a coordinate basis that is orthonomal in any open region U of a manifold M, with an obvious exception of the real coordinate space Rn considered as a manifold with the Euclidean metric δij ei ⊗ ej at every point.[4]
References
- ↑ M. P. Hobson; G. P. Efstathiou; A. N. Lasenby (2006), General Relativity: An Introduction for Physicists, Cambridge University Press, p. 57
- ↑ T. Padmanabhan (2010), Gravitation: Foundations and Frontiers, Cambridge University Press, p. 25
- ↑ Roger Penrose; Wolfgang Rindler, Spinors and Space–Time: Volume 1, Two-Spinor Calculus and Relativistic Fields, Cambridge University Press, pp. 197–199
- ↑ Bernard F. Schutz (1980), Geometrical Methods of Mathematical Physics, Cambridge University Press, p. 69, ISBN 9780521298872