Absolute spacetime: the twentieth century ether

Details Absolute spacetime: the twentieth century ether Absolute spacetime: the twentieth century ether

1998-01-09

arxiv.org/abs/gr-qc/9801029v1

Gen.Rel.Grav.31:597-607,1999

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Contribution to Proceedings of Mexico Meeting on Gauge Theories of Gravity in honor of Friedrich Hehl

Scientific paper

10.1023/A:1026632709502

All gauge theories need ``something fixed'' even as ``something changes.'' Underlying the implementation of these ideas all major physical theories make indispensable use of an elaborately designed spacetime model as the ``something fixed,'' i.e., absolute. This model must provide at least the following sequence of structures: point set, topological space, smooth manifold, geometric manifold, base for various bundles. The ``fine structure'' of spacetime inherent in this sequence is of course empirically unobservable directly, certainly when quantum mechanics is taken into account. This issue is at the basis of the difficulties in quantizing general relativity and has been approached in many different ways. Here we review an approach taking into account the non-Boolean properties of quantum logic when forming a spacetime model. Finally, we recall how the fundamental gauge of diffeomorphisms (the issue of general covariance vs coordinate conditions) raised deep conceptual problems for Einstein in his early development of general relativity. This is clearly illustrated in the notorious ``hole'' argument. This scenario, which does not seem to be widely known to practicing relativists, is nevertheless still interesting in terms of its impact for fundamental gauge issues.

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