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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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發(fā)表于 2025-3-21 20:07:30 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
期刊全稱Beyond Einstein
期刊簡稱Perspectives on Geom
影響因子2023David E. Rowe,Tilman Sauer,Scott A. Walter
視頻videohttp://file.papertrans.cn/186/185175/185175.mp4
發(fā)行地址Presents work by leading experts in Einstein studies along with eminent physicists and mathematicians.Explores recent developments and applications in the general theory of relativity in their histori
學(xué)科分類Einstein Studies
圖書封面Titlebook: Beyond Einstein; Perspectives on Geom David E. Rowe,Tilman Sauer,Scott A. Walter Book 2018 Springer Science+Business Media, LLC, part of Sp
影響因子.This volume explores the interplay between mathematical and physical research and the interactions of twentieth-century scientists within their academic communities. Beginning with Einstein’s general theory of relativity, the authors investigate a series of dramatic discoveries and rival theories in physics that influenced the development of modern differential geometry. Other sections recount the numerous methods, like the resurgence of Weyl geometry, used by geometers to solve the problems revealed by those same innovations in space-time physics. The effect of general relativity on astronomy is also addressed, namely how astronomers worked through new theories like inflationary cosmology and Phoenix models..By including recent historical research and coupling this work with many disciplines’ unique perspectives, this text provides a rich picture of general relativity and cosmology over the course of the twentieth century. The increased study on the documentation of Einstein’s early scientific work has clarified the history of science for that time and profoundly altered the way scientists view their own work, as this interdisciplinary volume demonstrates..
Pindex Book 2018
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Hilbert on General Covariance and Causalityfirst 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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Putting General Relativity to the Test: Twentieth-Century Highlights and Twenty-First-Century Prosperinciple, which underlies the concept that gravitation is synonymous with spacetime geometry and must be described by a metric theory. Solar system experiments that test the weak-field, post-Newtonian limit of metric theories strongly favor general relativity. Binary pulsars test gravitational-wave
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Rotating Hollow and Full Spheres: Einstein, Thirring, Lense, and Beyondfinitely 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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發(fā)表于 2025-3-22 12:58:07 | 只看該作者
Relativistic Lighthouses: The Role of the Binary Pulsar in Proving the Existence of Gravitational Wace that gravitational waves existed which was made possible over 40 years ago by the discovery of the first binary pulsar by Joe Taylor and Russell Hulse. This paper examines the theoretical controversies over how best to interpret measurements of the orbital decay of this remarkable system. Ultimat
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The Rise and Fall of the Fifth Forceed the gravitational potential from .?=??...∕. to .?=?(?...∕.)[1?+?..] where ., the strength of the interaction, was approximately one percent and the range of the force . was approximately 100 meters. This additional term was known as the Fifth Force. This suggestion was based on tantalizing eviden
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Inflation and the Origins of Structureig bang cosmology. Yet one of the most important consequences of inflation was only widely recognized a few years later: inflation provides a mechanism for generating small departures from uniformity, needed to seed formation of subsequent structures, by “freezing out” vacuum fluctuations to form cl
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