Abstract
The first part of the 20th century saw the most revolutionary breakthroughs in the history of theoretical physics, the birth of general relativity and quantum field theory. The seemingly nearly completed description of our world by means of classical field theories in a simple Euclidean geometrical setting experienced major modifications: Euclidean geometry was abandoned in favor of Riemannian geometry, and the classical field theories had to be quantized. These ideas gave rise to today’s theory of gravitation and the standard model of elementary particles, which describe nature better than anything physicists ever had at hand. The dramatically large number of successful predictions of both theories is accompanied by an equally dramatically large number of problems.
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Bick, E., Steffen, F. Introduction and Overview. In: Bick, E., Steffen, F.D. (eds) Topology and Geometry in Physics. Lecture Notes in Physics, vol 659. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-31532-2_1
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DOI: https://doi.org/10.1007/978-3-540-31532-2_1
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