rpt said:
Whether it is Minkowski space or otherwise, the space to have a precise quantifiable meaning, we should be able to accurately define the meaning of distance. In doing so we have to use the abstract mathematical idea called "point" which does not really exist.
Point is only an abstract mathematical idea in the mind. Without reconciling this issue we accept that the space really exist. This is the main problem I have in understanding space.
Physics is not about exact points, distances or anything else, but about approximations valid at the level of measurement accuracies.
It is enough to have an approximate notion of point and distance, and to verify that these approximately satisfy the properties demanded from the ideal points and distances the theory speaks about. And this is amply satisfied.
A far away star is an excellent example of an approximate point - it appears pointlike in all our experiments.
According to established physics, a real observer is a macroscopic
object with the capacity to record information. The recording process
is described by means of irreversible thermodynamics. In particular,
observers can be described to good accuracy classically, in terms of
their associated macroscopic observables. These are expectation values
of corresponding aggregated microscopic variables, behaving essentially
classically according to Ehrenfest's theorem. Large objects such as
stars can similarly be described by their associated macroscopic
observables. The position of an observer and the objects it observes changes
in time, defining their trajectories = world lines (apart from a global Poincare
transformation). This change is (on the macroscopic description level
appropriate for observers) continuous. (The world lines get fuzzy as one
focusses on smaller and smaller details, and become undetermined in
principle when the scale is reached where quantum effects dominate.
Indeed, the Heisenberg uncertainty principle forbids well-defined
trajectories of arbitrary accuracy.)
Suppose that the observer is the Mount Palomar observatory at a given time t. The observer's past light cone cuts out from 4-space a 3-dimensional manifold, which intersects the world lines of the objects observed at definite points (within the accuracy of the whole construction) - the positions x(t) of the visible stars at time t. This is indeed consistent with how astronomical positions are determined.
All this has a precise quantifiable meaning, to the accuracy needed to compare with experiments.