Recently in more technical settings (I was learning algebraic QFT), I encountered the term "real analytic" manifolds (Lorentzian manifolds, to be precise). This is in contrast to smooth manifolds, the same way real analytic functions are not the same as smooth ($C^\infty$) functions.
What I have trouble wrapping my head around are "simple" examples of analytic Lorentzian manifolds that differ from standard smooth Lorentzian manifolds. This issue is related to another post here, but I guess I am looking for something more concrete (and possibly simpler). I can frame this in two ways:
Are the standard examples in general relativity considered real-analytic manifolds? The ones I encounter most of the time---Minkowski, Schwarzschild, FRW spacetimes, seem to be the case: the Schwarzschild geometry has $f(r)=1-2M/r$. The FRW with good enough scale factors (like $a(\eta)=-1/(H\eta)$ for de Sitter case) is also real-analytic on $\eta<0$. I believe the same goes for the entire Kerr-Newman family and its maximal extension. In the Stackexchange post above, the argument seems to be a matter of talking about "the" maximal analytic extension, but if I just want to talk about the exterior of Schwarzschild or exterior of a star, for example, is real-analyticity really too strong? Another example I can probably think of is "gravitational shockwaves" (e.g., Aichelburg-Sexl metric) where the metric is not real-analytic (it is distributional, I guess). Does that mean all spacetimes whose metric can be written in terms of elementary real functions automatically real-analytic then?
If the spacetime is real-analytic, does the test fields on top of it have to be? For example, must hyperbolic wave equation be "real-analytic" (e.g., with real-analytic potentials) if the metric is real analytic? It looks to me that usually the fields living on some spaces does not need to inherit the properties of the background geometry, but I don't know.