Physicists usually talk about reference frames and more specially inertial reference frames. This is particularly important in Mechanics and Relativity. Now, from the Physics standpoint there's no doubt on what is a reference frame: it is a point of view to observe a phenomenon. From the Math standpoint, however, usually books speak very loosely about reference frames.
There are many things that books imply without ever making it explict. Some of those things are:
- Sometimes reference frames seems to be considered simply as coordinate systems on spacetime
- But sometimes, books seems to stress that they are "sets of axes", so only cartesian coordinates on flat spacetime would be reference frames
- Usually reference frames seems to be able to move around, but coordinate systems (on Differential Geometry sense) can't do this
Now, these are just some of the concerns. Never it is made clear what really a reference frame is mathematically and this is annoying me for a long time. Some mechanics books do even worse: they make it seems that a reference frame is just a question of interpreting the equations correctly.
Just making the last point clearer: in Differential Geometry one coordinate system is suited for a particular subset, so it doen't make sense to try moving one coordinate system around. This could only work in $\mathbb{R}^n$.
Also, for any manifold $M$ we can consider the bundle of frames $F(M)$ which is the bundle whose fiber at $a \in M$ is homeomorphic to $GL(n,\mathbb{R})$ representing all the possible bases for the tangent space at $a$. Because of the name (bundle of frames) I thought this could relate to physicists' reference frames.
So, what is really in a rigorous mathematical language a reference frame? And in using that definition, what will be then one inertial reference frame?
Here is how Sachs and Wu do it in General Relativity for Mathematicians (1977).
They start by defining a spacetime to be a connected 4-dimensional, oriented, and time-oriented Lorentzian manifold $(M,g)$ together with the Levi-Civita connection $D$ of $g$ on $M$.
Then they define an observer in $M$ to be a future-pointing timelike curve $\gamma$ such that $|\gamma_*|=1$. (This latter condition is just for convenience.)
Finally, they define a reference frame on a spacetime $M$ to be a vector field, each of whose integral curves is an observer.
The inertial frames are then those that are parallel, i.e. constant with respect to the covariant derivative. Intuitively, those are the frames that aren't "accelerating." (This is also related to Killing vector fields.)
But on Einstein-de Sitter spacetime, for example, there ARE no parallel reference frames: that's why inertial frames don't make sense, in general, in relativity. Asking for a parallel frame is a strong constraint on the metric.