Titlebook: Beyond Einstein; Perspectives on Geom David E. Rowe,Tilman Sauer,Scott A. Walter Book 2018 Springer Science+Business Media, LLC, part of Sp

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Heat Transfer to Structural Elements,first led to his infamous “hole argument”, a stumbling block that persuaded him early on that generally covariant field equations for gravitation could never be found. After his breakthrough to general covariance in the fall of 1915, the resolution came in form of the “point-coincidence argument.” H

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Wayne Martino,Maria Pallotta-Chiarollifinitely thin mass shell. Einstein’s impact on the subsequent work of Thirring and Lense from 1918 on the induction of gravitational dragging forces by accelerated (rotating) masses is revealed. Generalizations to strong fields were performed not earlier than in 1966 by Brill and Cohen. Extensions t

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irreparable

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Alan Ovens,Dawn Garbett,Derek Hutchinsonade a surprising comeback, however, in the last third of the 20th century in several different contexts: scalar-tensor theories of gravity, foundations of space-time theories, foundations of quantum mechanics, elementary particle physics, and cosmology. It seems that Weyl geometry continues to offer

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Ernest R. House,Stephen D. Lapanerizes the simplest closed three-manifold (the three-sphere). The paper discusses the unexpected irony whereby techniques from analysis and mathematical physics to which topology had contributed so much, would one century later repay the favor by being used to solve the most famous purely topologica