Suppose we have a Riemannian manifold $(M^n,g)$ and consider geodesic normal coordinates $x_1,\dots,x_n$ about $p$ in some neighbourhood $U.$ By shrinking $U$ as necessary, we will moreover assume it is geodesically convex.
To fix notation, write $e_i = \partial_{x_i}|_p$ which forms an orthonormal basis of $T_pM.$ Then if $x \in B_r$ for $r$ sufficiently small, we can identify this as a point in $M$ by $\exp_p(\sum x_ie_i)$ (this is really the local coordinates written out explicitly). The metric $g$ with respect to these coordinates will be denoted by $g_{ij}$ and its inverse by $g^{ij}.$
Question: Is it true that $x_i = g^{ij}(x)x_j$ for all $x \in B_r$?
Note in the above I am using the summation convention, so $j$ is summed over from $1, \dots, n.$ Also I am identifying $B_R$ with a neighbourhood of $p$ via the expoential map, as is the usual convention when working with local coordinates.
I am reading a paper which seems to suggest this, appealing to Gauss' lemma. From the perspective of the paper this is a minor point and hence was glossed over, but it would be useful for me if it's true.
Some ideas: If I let $y_i = g^{ij}x_j,$ I can view $y$ as an element of $T_pM$ similarly to $x.$ Then I can consider how $y$ transforms with respect to geodesic polar coordinates. I suspect you can then show by Gauss' lemma that $|x|^2 = |y|^2$ and combine it with the calculation $\langle x, y\rangle_g = g_{ij}x_ig^{jk}x_k = |x|^2,$ but I can't see the change of coordinates giving anything nice.
Recall Gauss lemma : If $g(0)(V,W)=0$, then $g(tV)(V,W)=0$.
Hence If $V=\sum_i\ x_ie_i,\ W=x_2e_1-x_1e_2$, then $$ x_2g_{1j}x_j =x_1g_{2j}x_j$$
so that $g_{ij}x_j=cx_i$ for some $c$.
Further, $g(V,V)=\sum_i\ x_i^2$ so that $c=1$.