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

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12 J. Stachelupon by no (net) external forces moves in a straight line with constantvelocity with respect to an inertial frame <strong>of</strong> reference. o This equivalence<strong>of</strong> all inertial frames has been called the relativity principle <strong>of</strong> Newtonianmechanics. There is a three-fold infinity <strong>of</strong> inertial frames, each <strong>of</strong> which isin a state <strong>of</strong> uniform motion with respect to all the others, <strong>and</strong> in each <strong>of</strong>which Newton’s laws <strong>of</strong> mechanics are equally valid.With the ab<strong>and</strong>onment <strong>of</strong> absolute space, the concept ‘at the same place’loses its absolute significance, <strong>and</strong> must be replaced by the concept ‘at thesame place relative to some inertial frame <strong>of</strong> reference.’ pIn summary, whether or not adherents <strong>of</strong> the mechanical worldviewwere aware <strong>of</strong> it, Newtonian mechanics properly understood does requirea universal or absolute concept <strong>of</strong> time, but leads to ab<strong>and</strong>onment <strong>of</strong> theconcept <strong>of</strong> absolute position in favor <strong>of</strong> a concept <strong>of</strong> relative position withrespect to some reference frame, usually chosen to be inertial.The concepts <strong>of</strong> absolute time <strong>and</strong> relative space may be given operationalsignificance in terms <strong>of</strong> the measurement <strong>of</strong> temporal <strong>and</strong> spatialintervals with (ideal) measuring clocks <strong>and</strong> rods, respectively. For example,the temporal interval (’time’) between two events, as measured bytwo clocks is independent <strong>of</strong> the inertial frame <strong>of</strong> reference in which theclocks are at rest (<strong>and</strong> therefore, they need not both be at rest in the sameframe). On the other h<strong>and</strong>, the spatial interval (distance) between two nonsimultaneousevents, as measured by a rigid measuring rod for example, isnot absolute, but depends on the inertial frame <strong>of</strong> reference in which themeasuring rod is at rest. Since there is no preferred inertial frame <strong>of</strong> reference(no ‘absolute space’), none <strong>of</strong> these relative distances can claim thetitle <strong>of</strong> ‘the (absolute) distance’.For simultaneous events, <strong>of</strong> course, the distance between them is independent<strong>of</strong> the inertial frame in which the measuring rod is at rest: Itmakes no difference whether the rod is at rest or in motion relative to thetwo events. When one speaks <strong>of</strong> ‘the length’ <strong>of</strong> an extended object, what iso The phrase ‘with constant velocity’ implies that an appropriate definition <strong>of</strong> distantsimultaneity must be adopted when, as in the special theory <strong>of</strong> relativity, the concept<strong>of</strong> absolute time is ab<strong>and</strong>oned. When we come to consider gravitation, we shall have toexamine the phrase: ‘acted on by no (net) external forces’ more critically.p One might be tempted to generalize, <strong>and</strong> say: ‘with respect to any arbitrary frame <strong>of</strong>reference’. But in both Galilei-Newtonian <strong>and</strong> special-relativistic theories, the inertialframes maintain their privileged role: The laws <strong>of</strong> physics take their simplest form whenexpressed relative to these frames – as long as gravitation is disregarded. As we shallsee, when gravitation is taken into account, the inertial frames lose their privileged roleeven in Galilei-Newtonian theory.

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