I get that this is a math question; however I find the tetrad/verbein formulation of things to be much more known among physicists.
Looking at the metric tensor components $g_{\mu\nu}$ in terms of tetrads we have then:
$$g_{\mu\nu}=e_{\mu}^{a}e_{\nu}^{b}\eta_{ab}$$
Where here $\eta_{ab}$ are components of the Minkowski metric.
We can compare that with the induced metric $g_{\mu\nu}$ of some curved space embedded in another space as:
$$g_{\mu\nu}=\frac{\partial X^{a}}{\partial\phi^{\mu}}\frac{\partial X^{b}}{\partial\phi^{\nu}}g_{ab}$$
where $g_{ab}$ is the metric of the embedding space. this equation is referred to as the pullback by a diffeomorphism.
Or for another example we can take a vector on our coordinate basis (Greek indices) and write its components in terms of vector components in our Lorentzian basis (latin indices):
$$v^{\mu}=e_{a}^{\mu}v^{a}$$
The inverse tetrad then seems to be playing the part of a pushforward. Is that correct?
I'm mostly interested in writing the metric of a spacetime and associated quantities in terms of the embedding space ( say $S^{3}\times\mathbb{R}\subset\mathbb{R}^{4,1}$ for example) Can I then import the tools of the pushforward-pullback yet still utilize the tetrad formalism in GR (just using more general metrics than the Minkowskian)?
Note that because the embedding space is higher dimensional, the tetrads would no longer be square when viewed as matrices. I would very much appreciate input or books utilizing this approach.
Note: This question is closely related but much more general than another question here
Also similar but again, more general than a question here.
EDIT:
In response to an answer below I just wanted to be really specific. Looking again at the component form of the pullback operation:
$$g_{\mu\nu}=\frac{\partial\phi^{i}}{\partial x^{\mu}}\frac{\partial\phi^{j}}{\partial x^{\nu}}g_{ij}$$
where Greek indices indicate one space and latin the other. If we specify then that we're operating our pullback on Minkowski space we get:
$$g_{\mu\nu}=\frac{\partial\phi^{i}}{\partial x^{\mu}}\frac{\partial\phi^{j}}{\partial x^{\nu}}\eta_{ij}$$
Comparing this with the tetrad formulation we get:
$$g_{\mu\nu}=\frac{\partial\phi^{i}}{\partial x^{\mu}}\frac{\partial\phi^{j}}{\partial x^{\nu}}\eta_{ij}=e_{\mu}^{i}e_{\nu}^{j}\eta_{ij}$$
Which makes me think the tetrad formulation is just a particular choice of pullback. For different spacetime topologies it may make sense to take the pullback to some other manifold to take advantage of symmetries of the space.
I ask yet another, similarly themed question here.