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
“...the nature of the metric field...is essentially one and therefore absolutely determined...in it the aprioristic essence of the space-time structure is expressed” (Weyl 1923b, p.45)
Scheibe 1999, VIII.3 (Newton/Cartan theory of gravitation)
Scheibe 1997b, IV. 1–3
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.
Bourbaki 1968, Ch. IV
Shoenfield 1967, Ch. 9
Bourbaki 1968, Ch. IV
ibid.
Trautman 1972, p. 85
Ludwig 1978
Stegmüller 1979
Scheibe 1979 (this vol. ch. III.11)
Trautman 1972, p. 85
Ehlers 1973
Rosen 1972
ibid.
Bourbaki 1968, Ch. IV
Iyanaga/ Kawada 1977, 92 D
ibid., 108 Z; Kobayashi/Nomizu 1963, p. 1
Ludwig 1978
ibid.
Havas 1964, Trautman 1967, Künzle 1972, Misner et al. 1973, Ch. 12
First published as Scheibe 1988e.
Weyl 1919, p. 25 ff; 1922 a; 1922 b; 1923 a; 1923 b, 7. und 8. Vorlesung; 1923 c, §19.
Weyl 1923 b, p. 45; 1949, p. 134.
Weyl 1923 b, p. 61.
Weyl 1923 b, p. 46.
Weyl 1923b, p. 46.
Weyl 1919, p. 27.
Laugwitz 1958. In this paper Laugwitz extends “Weyl’s first space problem” to the pseudo-riemannian case and prepares the ground for a similar characterization also in this case. However, he did not succeed then and has recently informed me that nobody seems to have continued his work.
Scheibe 1957, p. 172, 176.
Kobayashi and Nomizu 1963, p. 288.
Scheibe 1957, p. 192.
Klingenberg 1959, p. 301.
Cartan 1923, esp. pp. 171–174.
Kobayashi and Nomizu 1963, p. 288 f; Kobayashi and Nagano 1965, Theorem 2, p. 86; Freudenthal 1960, p. 107; 1964, p. 157 ff; 1967, p. 326.
For a modern treatment of Weyl’s geometries see Folland 1970. Our version is slightly more general than Folland’s: the conformal viewpoint is applied only locally.
More accurately stated, we have obtained the concept of a group field of a given nature Q3 where Q3 is a class of conjugate Lie-subgroups of the general linear group, see Scheibe 1957, §2. No group within Q3 is distinguished by our concept. By contrast, the concept of a G-structure requires such a distinction. However, the generalization of Weyl’s metric connection, to be given presently, also requires it.
Scheibe 1957, p. 175 Satz 1. With respect to the “historical myth” I want to destroy it should also be emphasized that, whereas an Ok-structure uniquely determines a torsionfree linear connection compatible with it, an Ok-field does not do this.
Weyl 1922 a, §1; 1922 b, V; 1923 b, 7. und 8. Vorlesung; 1923 c, §§ 17 und 19.
Weyl 1922b, p. 221 (p.344 of the Ges. Abh. II).
Weyl 1923b, p. 47, my italics.
It should be noticed that the otherwise somewhat clumsy concept of a class of linear connections related to a group field in the manner indicated has the advantage that it avoids the explicit dependency on the group G: It thus makes the whole concept of a metric dependent only on a class of conjugate groups representing the nature of the metric. This is very much in the spirit of Weyl! The following lemma (A) is in Weyl (1923 b), p. 49 f.
A second postulate used in this argument — the socalled postulate of the freedom of the metric — can be proven, cf. Weyl 1923 b, p. 49, Scheibe 1957, p. 196, Hilfssatz 1.
Cartan 1923; Freudenthal 1960.
Weyl 1923b, p. 46.
Wigner 1979, p. 16 f.
Scheibe 1982c (this vol. sect. VII.31).
Kobayashi and Nagano 1965, p. 86, theor. 1.
Weyl 1923 b, p. 45.
Weyl 1923 b, p. 49.
Weyl 1949, p. 137.
Coffa 1979, p. 277.
Weyl 1949, p. 137.
Weyl 1949, p. 134.
Künzle 1972. It is interesting that although Newton’s theory in a sense is a limiting case of Einstein’s, Weyl’s postulate does not survive the limiting process.
Weyl (1923 c), § 29
First published as Scheibe 1991f.
Einstein 1916b,sect. 3
ibid. sect. 2
ibid. sect.3
Kretschmann 1917, p. 576
Einstein 1918, p. 242
Einstein/ Infeld 1938, p.212
Einstein 1916b, sect. 2
ibid. sect. 3
Cartan 1923/4
Bourbaki 1968, Ch. IV
For the following see Scheibe 1982c (this vol. VII.31)
For details see Iyanaga/ Kawada 1977. 92 D and (a narrower concept) 108 Z.
A recent exception is Dixon 1978, pp. 42ff
Klein 1925
The Standard monograph is Schouten 1954
See Misner/ Thorne/ Wheeler 1973. What I am emphasizing is that, although the definition of, say, the concept of a vector field need not refer to coordinate Systems, the definition is based on the concept of a differentiable manifold and this concept usually is defined by using coordinate Systems.
A different analysis of the principle of general covariance can be found in Weinberg 1972, pp. 91ff
For some further thoughts on the matter see Scheibe 1982c (this vol. VII.31)
Anderson 1967 and 1971
Friedman 1973
First published as Scheibe 1994b.
Wigner 1979, 30 f.
Loc. cit., 16 f.
Dodd 1984, 41.
See, for instance, Genz und Decker 1991; Mayer-Kuckuk 1989.
For details see Bourbaki 1968, Ch. IV.
The first to have applied species of structures to physies in a systematic fashion is Ludwig in 1978, 21990.
See Scheibe 1982c (this vol. VII.31).
This is due to the von Neumann-Stone theorem, see Emch 1984, Ch. 8.3 f
See, for instance, Bethge und Schröder 1986, Ch. 5.
Einstein’s favorite view of the matter is discussed in Scheibe 1991f (this vol. VII.35).
Kant, Critique of Pure Reason, B 39.
Sommerfeld 1948.
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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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