Total scalar curvature

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 $d\mu$ the volume element, we have that:

Failed to parse (syntax error): {\displaystyle r = \frac{\int R d\mu}}

Here, the volume element $d\mu$ 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