Consider the unit hypersphere in $\mathbb{R}^n$, i.e. with the Euclidean metric, using spherical coordinates.
The metric tensor is then: $$ g_{11}=1 $$ $$ g_{ij}=\delta_{ij}\prod_{k=1}^{i-1}\sin^2(\theta_k) $$ where $\delta_{ij}$ is the Kronecker delta. The inverse metric is then: $$ g^{11}=1 $$ $$ g^{ij}=\delta_{ij}\prod_{k=1}^{i-1}\csc^2(\theta_k) $$ Notice that if any of $\theta_k=0$, then there will be a problem with $\csc(\theta_k)$. But $\theta_k=0$ seems to be a perfectly reasonable coordinate to be on.
Questions:
- (1) Why does the inverse metric fail to exist when $\theta_k=0$?
- (2) How do I fix this so that I can use the inverse metric computationally in cases where $\theta_k$ are allowed to freely vary (and vanish) as they can for $g$?
I'm hoping I'm making a silly mistake :)
(Note: this is true for $n=3$ too)