I'm trying to write the definition of arc length on a Riemannian manifold using fancy differential geometry language, mostly as a way to become familiarized with this language. Of course, writing this definition using just calculus is trivial.
Let $(M,g)$ be a Riemannian manifold, and $\alpha : I \to M$ a regular curve on it. (Think of $I$ as an abstract interval with a smooth structure, but no preferred coordinate.) Given a coordinate $t$ on $I$, the pullback metric $\alpha^\star g$ is represented by the $1 \times 1$ matrix whose lone entry is the squared length of the tangent vector field $v : I \to TI$ with coordinate $dt(v) = 1$. If the endpoints of $I$ have coordinate $t = a$ and $t = b$, the arc length of $\alpha$ is
$$\mathcal L(\alpha) = \int_a^b \sqrt {(\alpha^\star g) (v, v)} \, dt = \int_a^b \sqrt {g_{\alpha(t)}(d\alpha_t(v), d\alpha_t(v))} \, dt$$
I find this definition unsatisfying, because I needed to introduce $t$ and $v$ just to be able to state it, even though the associated geometric concept is independent of $t$ and $v$. Is there a coordinate-free way to state this definition?
Then for $\mathcal G \subset \mathcal K$ whose elements are all pairwise disjoint and whose union equals $\gamma$:
– user12262 Jan 07 '22 at 09:03