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 with a Riemannian metric .

Definition part

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

Here, the volume element 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