Enrico said:
[...] But what if one wants to define spacetime before deriving the (special) relativistic metric?
You've already been told that the underlying mathematical concept for spacetime is that of "manifold", but you still seem dissatisfied. So let's look a bit more carefully at what "manifold" means.
In the Wikipedia page about
manifolds it says:
Wikipedia said:
In
mathematics, a
manifold is a
topological space that locally resembles
Euclidean space near each point. More precisely, an n-dimensional manifold, or
n-manifold for short, is a topological space with the property that each point has a neighborhood that is
homeomorphic to an open subset of n-dimensional Euclidean space.
Carroll mentions "topology" in his introductory treatment, but doesn't delve into what that really means.
If you want more a thorough "formal" definition of spacetime as a manifold, you'll need to learn some basics about general (pre-metric) topology. (Try the Schaum Outline book on "General Topology" -- it presents a lot of material concisely.)
Intuitively, a "topology" (on a set of points) is a recipe for specifying a concept of "nearness" of points which does not necessarily involve a metric. This is done by specifying which collections of points in the set are to be called "open sets", as well as a few axioms those open sets must satisfy. I.e., specifying the "open" sets is equivalent to specifying a "topology". A set of points such that particular subsets therein are specified as "the" open sets (and satisfying the axioms of general topology) is called a "topological space".
A topological space need not be equipped with a metric. Indeed, there exist topologies which do not come with any notion of metric, and one talks about
Separation Axioms which make various (successively more restrictive) notions of "nearness" precise. E.g., in physics, we typically use topological spaces satisfying the Hausdorff separation axiom, hence are called "Hausdorff" spaces.
The concept of "topological spaces" is therefore more fundamental (mathematically) than "metric spaces" or "manifolds". Metric spaces are essentially topological spaces whose specification of "open sets" is in terms of a metric. E.g., a Euclidean space like ##R^n##, where the open sets are
open balls in ##R^n##.
A manifold is just a topological space which is locally homeomorphic to Euclidean space. "Homeomorphic" means that the topologies of the two spaces can be mapped into each other bijectively and continuously. That's what the Wikipedia page means when it says that a manifold "locally resembles Euclidean space near each point". (Where others have used the term "isomorphic" earlier in this thread, it's perhaps more precise to say "homeomorphic".)
The generic concept of "spacetime" is then a manifold equipped with an
additional pseudo-metric (i.e., Lorentzian pseudo-metric). Thus it has both an unphysical, but mathematical, Euclidean metric (which is positive-definite, hence useful for defining open balls and hence the topology), as well as the physical Lorentzian pseudo-metric (which is unsuitable for defining an open ball topology since it is not positive definite). Some neighbouring points on the manifold have finite nonzero Euclidean distance separation, but zero Lorenztian distance (e.g., on a lightlike path).
HTH.