jostpuur said:
Are you sure you accomplished this?
Yes, but keep in mind that I was talking about isometries in the sense of differential geometry, not in the sense of normed vector spaces. I included the proof in post #21.
jostpuur said:
So this problem became solved in the other Mazur-Ulamn thread.
Unfortunately no. Micromass' suggestion to use spacetime's exponential map is still the most promising approach. I haven't verified the details yet. I still don't even know how to define the exponential map of a Lorentzian manifold like Minkowski spacetime.
The technique that micromass suggested for Hilbert spaces works for Minkowski spacetime as well. It can be used to prove things like this: If ##\Lambda:\mathbb R^4\to\mathbb R^4## is a surjective map such that ##g(\Lambda(x),\Lambda(y))=g(x,y)## for all ##x,y\in\mathbb R^4##, then ##\Lambda## is linear and its matrix representation with respect to the standard basis satisfies ##\Lambda^T\eta\Lambda=\eta##. But that's not the problem I was having difficulties with.
If I could prove that "##\phi## is an isometry" implies something like the assumption in the theorem I just stated, then I'm pretty much done. Unfortunately all I was able to prove by using the definitions in a straightforward way was that the Jacobian satisfies a condition like the one I want the function itself to satisfy.
jostpuur said:
But this discussion also introduced a new problem which is that if the mapping has an infinitesimal isometry property, then the isometry property extends to finite regions and possibly the whole space. Did this become solved too? I didn't understand how it happened.
I don't understand what you're referring to here, or what an infinitesimal isometry property is. Hm, "infinitesimal" often refers to things related to the tangent space. So maybe you meant something like an isometry in the sense of normed vector spaces, i.e. a condition like ##g(\Lambda(x)-\Lambda(y),\Lambda(x)-\Lambda(y))=g(x-y,x-y)##? The problem I asked about in #1 doesn't start with a condition like that. It starts with the condition that ##\phi:\mathbb R^4\to\mathbb R^4## is such that ##\phi^*g=g##, where ##\phi^*## denotes the pullback map. It's defined by ##\phi^*g_{\phi(p)}(u,v)=g_p(\phi_*u,\phi_*v)##, where ##\phi_*## is the pushforward map, defined by ##\phi_*v(f)=v(f\circ\phi)##. I'm using all these definitions in post #21.