Titlebook: At the Frontier of Spacetime; Scalar-Tensor Theory Torsten Asselmeyer-Maluga Book 2016 Springer International Publishing Switzerland 2016 B

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Fundamental Theories of Physicshttp://image.papertrans.cn/b/image/163901.jpg

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Resistance: London, France, Algeria,c instabilities around constant curvature space-times in four dimensions. Specifically, this includes the Minkowski, de Sitter and anti-de Sitter backgrounds. We will first argue in details how starting from a general covariant action for the metric one arrives at an “equivalent” action that at most

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,The Fall of the Fourth Republic: 1951–1958, of such a boson cloud would lead to a . (BS) as a new type of a compact object. Similarly as for white dwarfs and neutron stars (NSs), there exist a limiting mass, the Kaup limit, below which a BS is . against complete gravitational collapse to a black hole (BH). Depending the self-interaction of t

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https://doi.org/10.1057/9781137315458dilatonic) Brans–Dicke theory only for the exponential potential ., which corresponds to the quadratic potential . in terms of the original Brans–Dicke field ., or for potentials which approach to . at the stable point. I find bounds on the Brans–Dicke coupling constant ., which are consistent with

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https://doi.org/10.1057/9781137315458nding the tensor-based theory by a scalar field. But experimental support has not materialized. Nevertheless the model continues to generate interest and new research. The reasons for the current activity is described in this essay, which is dedicated to Carl Brans on his eightieth birthday.

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,Unreliable Allies: Empire, 1952–1958,with the publication of a 10-page paper in Physical Review. An extension of Einstein’s general relativity, it generated great interest and was the subject of enormous effort to test its implications experimentally. We examine the history and impact of the experimental tests of this theory.

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