Second covariant derivative

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In the math branches of differential geometry and vector calculus, the second covariant derivative, or the second order covariant derivative, of a vector field is the derivative of its derivative with respect to another two tangent vector fields.

Definition

Formally, given a (pseudo)-Riemannian manifold (M, g) associated with a vector bundle EM, let ∇ denote the Levi-Civita connection given by the metric g, and denote by Γ(E) the space of the smooth sections of the total space E. Denote by T*M the cotangent bundle of M. Then the second covariant derivative can be defined as the composition of the two ∇s as follows: [1]

Γ(E)Γ(T*ME)Γ(T*MT*ME).

For example, given vector fields u, v, w, a second covariant derivative can be written as

(u,v2w)a=ucvbcbwa

by using abstract index notation. It is also straightforward to verify that

(uvw)a=uccvbbwa=ucvbcbwa+(uccvb)bwa=(u,v2w)a+(uvw)a.

Thus

u,v2w=uvwuvw.

When the torsion tensor is zero, so that [u,v]=uvvu, we may use this fact to write Riemann curvature tensor as [2]

R(u,v)w=u,v2wv,u2w.

Similarly, one may also obtain the second covariant derivative of a function f as

u,v2f=ucvbcbf=uvfuvf.

Again, for the torsion-free Levi-Civita connection, and for any vector fields u and v, when we feed the function f into both sides of

uvvu=[u,v]

we find

(uvvu)(f)=[u,v](f)=u(v(f))v(u(f))..

This can be rewritten as

uvfvuf=uvfvuf,

so we have

u,v2f=v,u2f.

That is, the value of the second covariant derivative of a function is independent on the order of taking derivatives.

Notes

  1. Parker, Thomas H. "Geometry Primer" (PDF). Retrieved 2 January 2015., pp. 7
  2. Jean Gallier and Dan Guralnik. "Chapter 13: Curvature in Riemannian Manifolds" (PDF). Retrieved 2 January 2015.