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100 Years of Relativity Space-Time Structure: Einstein and Beyond ...

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32 J. Stachelwhich merely defines the chronogeometrical relations between events givenpriori. This is incorrect for at least two reasons. As noted earlier, withoutthe specification <strong>of</strong> a particular metric tensor field, we cannot specify theglobal topology <strong>of</strong> the base space differentiable manifold. But, even locally,there is no means <strong>of</strong> physically individuating a priori the points <strong>of</strong> a region<strong>of</strong> a bare manifold. If particles or other, non-gravitational fields are presentin the region, then their properties may suffice to individuate the points <strong>of</strong>the region. But even then, without a metric, it is generally impossible t<strong>of</strong>ully interpret the physical properties <strong>of</strong> such non-gravitational entities.If we confine ourselves to otherwise empty regions, in which only thechronogeometrical (<strong>and</strong> corresponding inertio-gravitational) field is present,then the points <strong>of</strong> such a region cannot be physically individuated by anythingbut the properties <strong>of</strong> this field. oo16. The Second Relativization <strong>of</strong> <strong>Time</strong>Among the properties <strong>of</strong> any physical event are its position in space-time:the ‘here’ <strong>and</strong> ‘now’ <strong>of</strong> the event. One cannot give meaning to the concepts‘here’ <strong>and</strong> ‘now’ <strong>of</strong> an event in otherwise empty regions <strong>of</strong> space-timewithout use <strong>of</strong> the chronogeometry (metric tensor). This leads to a secondrelativization <strong>of</strong> the concept <strong>of</strong> time in general relativity that is even moredrastic than that required by the special theory <strong>of</strong> relativity.To recall what has been said earlier: In Galilei-Newtonian kinematics,the absolute time function as a global time, the same for all rigid referenceframes, regardless <strong>of</strong> their states <strong>of</strong> motion, even when gravitation is takeninto account; <strong>and</strong> it also serves as a local time, the time elapsed betweentwo events is the same for all time-like paths between them.In special-relativistic kinematics, this unique concept <strong>of</strong> absolute timesplits into two different concepts, both <strong>of</strong> which are relativized. <strong>Time</strong> inthe global sense (the time used to compare events at different places) isrelative to the inertial frame chosen, i.e., to one member <strong>of</strong> a preferredclass <strong>of</strong> reference frames. <strong>Time</strong> in the local sense (the proper time thatelapses between events along a time-like path) is relative to the path <strong>and</strong>differs for different paths between the same two events.In both pre-relativistic <strong>and</strong> special-relativistic kinematics, the use <strong>of</strong>different frames <strong>of</strong> reference leads to different descriptions <strong>of</strong> some processundergone by a dynamical system: The expression for the initial state <strong>of</strong>oo For a more detailed discussion <strong>of</strong> this point, see Ref. 10.

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