Total scalar curvature: Difference between revisions

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The '''total scalar curvature''' of <math>M</math> is defined as the integral over the volume of the [[scalar curvature]] over the manifold. That is, if <math>R</math> denotes the scalar curvature and <math>d\mu</math> the volume element, we have that:
The '''total scalar curvature''' of <math>M</math> is defined as the integral over the volume of the [[scalar curvature]] over the manifold. That is, if <math>R</math> denotes the scalar curvature and <math>d\mu</math> the volume element, we have that:


<math> r = \frac{\int R d\mu}</math>
<math> r = \int R d\mu</math>


Here, the volume element <math>d\mu</math> is the natural choice of volume-element arising from the Riemannian metric.
Here, the volume element <math>d\mu</math> is the natural choice of volume-element arising from the Riemannian metric.

Revision as of 19:07, 22 May 2007

This article defines a notion of curvature for a differential manifold equipped with a Riemannian metric

This article defines a scalar value (viz, a real number) associated with a Riemannian manifold. This real number depends both on the underlying differential manifold and the Riemannian metric

Definition

Given data

A compact connected differential manifold M with a Riemannian metric g.

Definition part

The total scalar curvature of M is defined as the integral over the volume of the scalar curvature over the manifold. That is, if R denotes the scalar curvature and dμ the volume element, we have that:

r=Rdμ

Here, the volume element dμ is the natural choice of volume-element arising from the Riemannian metric.

Note that if we divide by the total volume, we get the average scalar curvature.

Further information: average scalar curvature