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"On the History of Unified Field Theories. Part II. (ca. 1930 – ca. 1965)"
Hubert F. M. Goenner 
Abstract
1 Introduction
2 Mathematical Preliminaries
3 Interlude: Meanderings – UFT in the late 1930s and the 1940s
4 Unified Field Theory and Quantum Mechanics
5 Born–Infeld Theory
6 Affine Geometry: Schrödinger as an Ardent Player
7 Mixed Geometry: Einstein’s New Attempt
8 Schrödinger II: Arbitrary Affine Connection
9 Einstein II: From 1948 on
10 Einstein–Schrödinger Theory in Paris
11 Higher-Dimensional Theories Generalizing Kaluza’s
12 Further Contributions from the United States
13 Research in other English Speaking Countries
14 Additional Contributions from Japan
15 Research in Italy
16 The Move Away from Einstein–Schrödinger Theory and UFT
17 Alternative Geometries
18 Mutual Influence and Interaction of Research Groups
19 On the Conceptual and Methodic Structure of Unified Field Theory
20 Concluding Comment
Acknowledgements
References
Footnotes
Biographies
Note the altered notation with regard to Eqs. (3) and (4) in Part I of this article, where the notation of [632*] has been used. Here, we take over the notation of A. Lichnerowicz ([371*], p. 255). The correspondences are ik ik ik ik γik ∼ hik, ϕik ∼ kik, h ∼ l , f ∼ m The inverses are defined with the same kernel letter. Also, in physical applications, special conditions for h and k might be needed in order to guarantee that g is a Lorentz metric. Equation (3*) reflects Hlavatý’s notation, too.