Category: General Relativity
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In this article, we will calculate the Euclidian metric tensor for a surface of a sphere in spherical coordinates by two ways, as seen in the previous article Generalisation of the metric tensor

Spherical coordinates (r, θ, φ) as commonly used in physics: radial distance r, polar angle θ (theta), and azimuthal angle φ (phi). Source Wikipedia


Deducing the metric by the line element

In this Euclidian three-dimensionnal space, the line element is given by:

dl2 = dr2 + r22 + r2sin2θdΦ2

If we set the polar coordinate r to be some constant R we lose the dr term (because r is now constant) and the line element now becomes: 

dl2 = R22 + R2sin2θdΦ2

which describes a two-dimensional surface using the two polar coordinates (θ, Φ)

Or we know from the previous article that this line element could be written as:

dl2 = gijdxidyj

We can deduce immediately that the metric and inverse metric for this surface, using coordinates x0=θ and x1=Φ, are:


This was the easy part. Let's try to calculate the same metric by using  the formula of the coordinates derivatives product.

Calculating the metric by the Cartesian  coordinates derivatives product

We should recall that we also defined the metric tensor as the product of derivatives to another coordinate system (in the previous article, it was from a Minkowski inertial referential)

 Or the cartesian coordinates and spherical coordinates are linked together by the following equations:


At this point we can confirm that by both the space  line element and the product of coordinates derivatives, we have found exactly the same components for the metric of a two-dimensional surface of a sphere in polar coordinates