4 Unified Field Theory and Quantum Mechanics
Obviously, Einstein did not trust an investigation like the experimental physicist Osborn’s (1917 – 2003) trying to show by ideal measurements that the notion of curvature can be applied only “in the large” where “the domain of largeness is fundamentally determined by the momentum of the test particle with which the curvature is measured” – due to limitations from quantum mechanics [465]. Osborn’s feeling obviously was shared by the majority of elementary particle physicists, in particular by F. Dyson:“The classical field theory of Einstein – electromagnetic and gravitational together – give us a satisfactory explanation of all large-scale physical phenomena. […] But they fail completely to describe the behavior of individual atoms and particles. To understand the small-scale side of physics, physicists had to invent quantum mechanics and the idea of the quantum field.” ([137*], p. 60)
Nevertheless, there were other physicists like Einstein for whom no divide between classical and quantum field existed, in principle.
4.1 The impact of Schrödinger’s and Dirac’s equations
In the introduction to Section 7 of Part I, a summary has been given of how Einstein’s hope that
quantum mechanics could be included in a classical unified field theory was taken up by other
researchers. A common motivation sprang from the concept of “matter wave” in the sense of a
wave in configuration space as extracted from Schrödinger’s and Dirac’s equations. Henry
Thomas Flint whom we briefly met
in Section 7.1 of Part I, was one of those who wanted to incorporate quantum theory into a
relativistic field theory for gravitation and electrodynamics. In Flint’s imagination, the content
of quantum mechanics was greatly condensed: it already would have been reproduced by the
generation of a suitable relativistic wave equation for the wave function as a geometric
object in an appropriate geometry. This might be taken as an unfortunate consequence of the
successes of Schrödinger’s wave theory. In the first paper of a series of three, Flint started with a
5-dimensional curved space with metric
and an asymmetric connection:

![k k Δ [ij] = S ij](article619x.gif)
















As a preparation for the second paper in the series mentioned [205], a link to matrix theory as developed by Schrödinger was given through replacement of the metric “by more fundamental quantities”, the 5 by 5 matrices








In the third paper of 1935 [206*], Flint took up the idea of “matrix length”










“In connection with the equation of the electron path we have the suggestion that
respond to the certainty of finding the electron on the track” ([206*], same page).
His conclusion, i.e., that quantum phenomena correspond to geometrical conceptions, and that the
complete geometrical scheme includes quantum theory, gravitation, and electromagnetism could not hide
that all he had achieved was to build a set of classical relativistic wave equations decorated with an . In
a further paper of 1938, in the same spirit, Flint arrived at a geometrical “quantum law” built after the
vanishing of the curvature scalar from which he obtained the Dirac equation in an external electrical field
[207].
During the second world war, Flint refined his research without changing his basic assumption
[208, 209, 210], i.e., “that the fundamental equation of the quantum theory, which is the quantum equation
for an electron in a gravitational and electromagnetic field, can be developed by an appeal to simple
geometric ideas.” His applications to “field theories of the electron, positron and meson” [211] and to
“nuclear field theories” [212] follow the same line. No progress, either for the understanding of quantum
mechanics nor for the construction of a unified field theory, can be discovered. Flint’s work was not
helped by contributions of others [6, 3]. After World War II, Flint continued his ideas with a
collaborator [214*]; in the meantime he had observed that Mimura also had introduced matrix
length in 1935. As in a previous paper, he used the method by which Weyl had derived his first
gauge theory combining gravitation and electromagnetism. Strangely enough, Weyl’s later main
success, the re-direction of his idea of gauging to quantum mechanics was not mentioned by Flint
although he was up to show that “equations of the form of Dirac’s equation can be regarded as
gauge-equations”([214], p. 260). Under parallel transport, the matrix length of a vector
is
assumed to change by
, where
is an operator (a matrix) corresponding to
the 5-vector
. Flint still was deeply entrenched in classical notions when approaching the
explanation of the electron’s rest mass: it should contain contributions from the electromagnetic
and mesonic fields. The mathematician J. A. Schouten conjectured that “[t]he investigations
of H. T. Flint are perhaps in some way connected with conformal meson theory […]” ([539*],
p. 424).
That Flint was isolated from the physics mainstream may be concluded also from the fact that his papers are not cited in a standard presentation of relativistic wave-equations [84]. We dwelled on his research in order to illuminate the time lag in the absorption of new physics results among groups doing research, simultaneously. In this theme, we could have included the “tensor rear guard” (Fisher, Temple, etc.) who believed to be able to get around spinors.
4.2 Other approaches
We come back to a paper by M. Born which was referred to already in Section 3.3.2, but under a different
perspective. In view of the problems of quantum field theory at the time with infinite self-energy of the
electron, the zero-point energies of radiation fields adding up to infinity etc., Max Born preferred to unify
quantum theory and “the principle of general invariance”, i.e., inertial fields rather than include the
gravitational field. The uncertainty relations between coordinates and momenta served as a motivation for
him to assume independent and unrelated metrics in configuration and
in
momentum space [39*]. As field equations in momentum space he postulated the Einstein field
equations for a correspondingly calculated Ricci-tensor (as a function of momenta)
:











4.3 Wave geometry
A group of theoreticians at the Physical Institute of Hiroshima University in Japan in the second half of the 1930s intensively developed a program for a unified field theory of a new type with the intention of combining gravitation and quantum theory. Members of the group were Yositaka Mimura, Tôyomon Hosokawa, Kakutarô Morinaga, Takasi Sibata, Toranosuke Iwatsuki, Hyôitirô Takeno, and also Kyosi Sakuma, M. Urabe, K. Itimaru. The research came to a deadly halt when the first atom bomb detonated over Hiroshima, with the hypo-center of the explosion lying 1.5 km away from the Research Institute for Theoretical Physics.66 After the second world war, some progress was made by the survivors. The theory became simplified and was summarized in two reports of the 1960s [427*, 428*].
In an introductory paper by Mimura, the new approach was termed “wave geometry” [425*]. His intention was to abandon the then accepted assumption that space-geometry underlying microscopic phenomena (like in elementary particle physics), be the same as used for macroscopic physics. Schrödinger had argued in this sense and was cited by Mimura [541]. Einstein’s original hope that space-time must not exist in the absence of matter, unfulfilled by general relativity, became revived on the level of “microscopic physics”: “[…] the microscopic space exists only when an elementary particle exists. In this sense, where there is no elementary particle, no ‘geometry’ exists” ([425*], p. 101). Also “[…] according to our new theory, geometry in microscopic space differs radically from that of macroscopic […]” ([425], p. 106).67 “wave geometry” must not be considered as one specific theory but rather as the attempt for a theory expressing the claimed equivalence of geometry and physics.
The physical system, “the space-time-matter” manifold, was to be seen as a (quantum mechanical) state
, a 4-component (Dirac) spinor; “distance” in microscopic space became defined as an eigenvalue of a
linear distance operator. In order to find this operator, by following Dirac, a principle of linearization was
applied:










![Γ i := 14[hsr∂ihrt − {sti}g]γtγs](article699x.gif)











In 1938, T. Hosokawa even had extended wave geometry to Finsler geometry and applied to Milne’s cosmological principle [287*].
With its results obtained until 1945, wave geometry could not compete with quantum field
theory. After the war, the vague hope was expressed that in a “supermicroscopic” space-time,
elementary particle theory could be developed and that “the problem of internal space’ of elementary
particles may be interwoven with some ‘hidden’ relations to the structure of space-time.”([428*],
p. 41.) Clearly, the algebra of -matrices which is all what is behind the distance operator,
was an insufficient substitute for the algebra of non-commuting observables in quantum field
theory.