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

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6 J. StachelFig. 2respectively. Furthermore, Newtonian gravitation theory is considered in itsmodern, four-dimensional formulation, which takes into account the equivalenceprinciple (see Sec. 11); I have adopted the name for this formulation<strong>of</strong> Newtonian theory introduced by Jürgen Ehlers – General Non-<strong>Relativity</strong>— which contrasts nicely with General <strong>Relativity</strong>. But the name should notbe taken to imply that the theory has no relativity (i.e., no symmetry group<strong>of</strong> the space-time): indeed, the chronogeometry <strong>of</strong> this class <strong>of</strong> space-timesis invariant under a wider group than that <strong>of</strong> Galilei-Newtonian space-time,as discussed in Secs. 5 <strong>and</strong> 8.The upper right-h<strong>and</strong> corner <strong>of</strong> the cube, Quantum Gravity, also callsfor further comment. It is not the name <strong>of</strong> an already-existing theory, butrather <strong>of</strong> a hope: The goal <strong>of</strong> much current research in theoretical physics isto find a theoretical framework wide enough to encompass (in some sense)both classical general relativity <strong>and</strong> (special-relativistic) quantum field theory.Unfortunately, in the current state <strong>of</strong> this subject, the edges <strong>of</strong> the cubedo not commute (see Figs. 3, 4). Starting from quantum field theory on theroad to quantum gravity <strong>and</strong> attempting to incorporate the Newtonian constantG, most particle physicists believe that one will arrive at some versionI Figure 2

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