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In differential geometry, the curvature form describes of a on a . The Riemann curvature tensor in Riemannian geometry can be considered as a special case.


Definition
Let G be a with \mathfrak g, and PB be a . Let ω be an Ehresmann connection on P (which is a \mathfrak g-valued one-form on P).

Then the curvature form is the \mathfrak g-valued 2-form on P defined by

\Omega=d\omega + {1 \over 2}\omega = D \omega.

(In another convention, 1/2 does not appear.) Here d stands for exterior derivative, \cdot is defined in the article "Lie algebra-valued form" and D denotes the exterior covariant derivative. In other terms,since \omega(X, Y) = \frac{1}{2}(\omega(X), - \omega(Y),). Here we use also the \sigma=2 Kobayashi convention for the exterior derivative of a one form which is then d\omega(X, Y) = \frac12(X\omega(Y) - Y \omega(X) - \omega(X,))

\,\Omega(X, Y)= d\omega(X,Y) + {1 \over 2}\omega(X),\omega(Y)
where X, Y are tangent vectors to P.

There is also another expression for Ω: if X, Y are horizontal vector fields on P, thenProof: \sigma\Omega(X, Y) = \sigma d\omega(X, Y) = X\omega(Y) - Y \omega(X) - \omega(X,) = -\omega(X,).

\sigma\Omega(X, Y) = -\omega(X,) = -X, + hX,
where hZ means the horizontal component of Z, on the right we identified a vertical vector field and a Lie algebra element generating it (fundamental vector field), and \sigma\in \{1, 2\} is the inverse of the normalization factor used by convention in the formula for the exterior derivative.

A connection is said to be flat if its curvature vanishes: Ω = 0. Equivalently, a connection is flat if the structure group can be reduced to the same underlying group but with the discrete topology.


Curvature form in a vector bundle
If EB is a vector bundle, then one can also think of ω as a matrix of 1-forms and the above formula becomes the structure equation of E. Cartan:

\,\Omega = d\omega + \omega \wedge \omega,

where \wedge is the . More precisely, if {\omega^i}_j and {\Omega^i}_j denote components of ω and Ω correspondingly, (so each {\omega^i}_j is a usual 1-form and each {\Omega^i}_j is a usual 2-form) then

\Omega^i_j = d{\omega^i}_j + \sum_k {\omega^i}_k \wedge {\omega^k}_j.

For example, for the of a Riemannian manifold, the structure group is O( n) and Ω is a 2-form with values in the Lie algebra of O( n), i.e. the antisymmetric matrices. In this case the form Ω is an alternative description of the curvature tensor, i.e.

\,R(X, Y) = \Omega(X, Y),

using the standard notation for the Riemannian curvature tensor.


Bianchi identities
If \theta is the canonical vector-valued 1-form on the , the torsion \Theta of the \omega is the vector-valued 2-form defined by the structure equation

\Theta = d\theta + \omega\wedge\theta = D\theta,

where as above D denotes the exterior covariant derivative.

The first Bianchi identity takes the form

D\Theta = \Omega\wedge\theta.

The second Bianchi identity takes the form

\, D \Omega = 0

and is valid more generally for any in a .

The Bianchi identities can be written in tensor notation as: R_{abmn;\ell} + R_{ab\ell m;n} + R_{abn\ell;m} = 0.

The contracted Bianchi identities are used to derive the in the Einstein field equations, a key component in the general theory of relativity.


Notes
  • Shoshichi Kobayashi and (1963) Foundations of Differential Geometry, Vol.I, Chapter 2.5 Curvature form and structure equation, p 75, Wiley Interscience.


See also
  • Connection (principal bundle)
  • Basic introduction to the mathematics of curved spacetime
  • Contracted Bianchi identities
  • Einstein field equations
  • General theory of relativity
  • Chern-Simons form
  • Curvature of Riemannian manifolds

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