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Spacetime, Invariance, Covariance

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Abstract

The papers collected in this chapter concern the physical structure of space, time and spacetime. Problems connected with invariance properties of physical theories based on invariance properties of their corresponding spacetime theories are well-known, e.g. the Galileo invariance of Newton’s dynamics, the Lorentz invariance of classical electrodynamics and the general covariance of Einstein’s field equations. In [31], [33] and [34] problems of the formulation, the meaning and the physical content of invariance and covariance statements are dealt with. Less well-known is the question of characterizing the structure and theory of spacetime by assumptions as plausible as possible from the physical point of view. The classical case is Helmholtz’ characterization of the riemannian spaces of constant curvature by means of their group of free mobility of rigid bodies. Since today we believe in Einstein’s general theory of relativity, a more appropriate characterization should refer to the Lorentz manifolds that are the infinitesimal version of Minkowski spacetime. No such characterization seems to be known. But Hermann Weyl succeeded in 1923 in characterizing a slightly more general class of manifolds which he named after Pythagoras ([32]).

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References

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  4. First published as Scheibe 1982c. The completion of this paper was made possible by a Visiting Fellowship at the Center for Philosophy of Science at the University of Pittsburgh. The author wants to express his gratitude to the chairman and the director of the Center, Professor A. Grünbaum and Professor L. Laudan, for the kind invitation and generous hospitality.

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  75. A different analysis of the principle of general covariance can be found in Weinberg 1972, pp. 91ff

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Scheibe, E. (2001). Spacetime, Invariance, Covariance. In: Falkenburg, B. (eds) Between Rationalism and Empiricism. Springer, New York, NY. https://doi.org/10.1007/978-1-4613-0183-7_7

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  • DOI: https://doi.org/10.1007/978-1-4613-0183-7_7

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