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On the Origin of Kaluza's Idea of Unification

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We argue that the starting point of Kaluzas idea of unifying electrodynamics and gravity was the analogy between gravitation and electromagnetism which was pointed out by Einstein and Thirring. It seems that Kaluzas attention was turned to this point by the three papers on the Lense–Thirring effect and the analogy between gravitation and electromagnetism which were published a short time before Kaluzas paper was submitted. We provide here also an English translation of the third of these papers (Phys. Zeits. 19: 204, 1918).
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The Collected Papers of Albert Einstein
  • A Engel
A. Engel, The Collected Papers of Albert Einstein, Vol. 6: English Translation, Princeton University Press (1997).
  • D Wuensch
D. Wuensch, Ann. Phys. (Leipzig) 12, 519 (2003).
  • H F M Goenner
H. F. M. Goenner, Living Rev. Rel. 7, 2 (2004).
  • G Nordstrom
G. Nordstrom, Phys. Zeits. 15, 504 (1914).
  • A Einstein
A. Einstein, Phys. Zeits. 14, 1249 (1913).
The Collected Papers
  • A Beck
A. Beck, The Collected Papers of Albert Einstein, Vol. 4: English Translation, Princeton University Press (1996).
  • H Thirring
H. Thirring, Phys. Zeits. 19, 204 (1918).
  • H Thirring
  • J Lense
H. Thirring and J. Lense, Phys. Zeits. 19, 156 (1918).
  • B Mashhoon
  • F W Hehl
  • D S Theiss
B. Mashhoon, F. W. Hehl and D. S. Theiss, Gen. Rel. and Grav. 16, 711 (1984).
  • B Mashhoon
B. Mashhoon, arXiv:gr-qc/0311030
  • A Tartaglia
  • M L Ruggiero
A. Tartaglia and M. L. Ruggiero, Eur. J. Phys. 25, 203 (2004)