A.T. said:
@lriuui0x0 Is this what you had in mind?
What I originally had in mind is below:
So we have an affine spacetime ##N^4##, the associated vector space ##V^4##, with the simultaneity subspace ##V^3##. An oberserver in my mind is the combination of a smooth worldline ##\gamma: \mathbb{R} \to N^4## and a smooth orthonormal basis assignment in ##\mathbf{e}_1, \mathbf{e}_2, \mathbf{e}_3: \mathbb{R} \to V^3##. The Galilean transformation transforms this worldline and the basis assignment. It will be an affine map ##f: N^4 \to N^4##, with associated linear map ##g: V^4 \to V^4##, and ##g## can be applied to the orthonormal basis vector to let the observer "look at different direction".
Please help check if the above idea of transforming an observer makese sense!
For transforming among inertial observers, it will conceptually look like:
(The three big coordinate arrows was just there to make the drawing look better, they're not part of the entities under discussion).
I think this transformation has nothing specific to the observer being inertial, right? It can be similarly be applied to non-inertial observers, like:
The Newton's equation will have a particular form on the left, involving ficticious forces. My original question is will it be of the same form on the right? Based on the calculation above, ##\mathbf{a}_2 = \mathbf{a}_1##. Or at least ##\mathbf{a}_2 = R(\mathbf{a}_1)## with ##R## being a rotation, if we take the general transformation ##(x, t) \mapsto (Rx + vt + d, t + s)##. So I think the fictious force doesn't change apart from a rotation?
But there's also the question if the real force changes its form or not. I was thinking for gravity and Columb's force, since they depend on only the distance of particles, they will not change its form under Galilean transformation, at least if you start with an inertial observer. But I also want to confirm this and also what about non-inertial observer? If they don't change form, then can we conclude that the entire Newton's equation doesn't change form either?