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Titlebook: Quantum Geometry; A Framework for Quan Eduard Prugove?ki Book 1992 Springer Science+Business Media Dordrecht 1992 Minkowski space.cosmology

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樓主: Helmet
11#
發(fā)表于 2025-3-23 13:46:30 | 只看該作者
12#
發(fā)表于 2025-3-23 16:08:01 | 只看該作者
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發(fā)表于 2025-3-23 18:27:59 | 只看該作者
14#
發(fā)表于 2025-3-23 22:35:39 | 只看該作者
Historical and Epistemological Perspectives on Developments in Relativity and Quantum Theory, the experimentalists’ conscious or subconscious biases. Hence, the outcome is prone to various kinds of errors, ranging from systematic ones, due to the faulty design of apparatus or erroneous analysis of the raw data, to the subtle ones, due to misinterpretation or unwarranted extrapolation.
15#
發(fā)表于 2025-3-24 05:21:23 | 只看該作者
16#
發(fā)表于 2025-3-24 10:17:39 | 只看該作者
Relativistic Quantum Geometries for Spin-0 Massive Fields,ed in Sec. 7.6. Hence, the last word on this subject has to go to the acknowledged founder of relativistic quantum field theory as well as of relativistic quantum mechanics, P.A.M. Dirac, whose insightful and uncompromisingly forthright assessments of these two disciplines have greatly inspired the present work.
17#
發(fā)表于 2025-3-24 14:37:50 | 只看該作者
Quantum Geometries for Electromagnetic Fields,due to the absence of rest frames for such objects. This means the notion of proper time is meaningless for zero-mass particles, and that such particles can be localized only in relation to frames constructed out of massive particles.
18#
發(fā)表于 2025-3-24 15:20:02 | 只看該作者
Geometro-Stochastic Quantum Gravity,covariance feature of CGR reflects the fact that the . fundamental observable entities in CGR are spacetime coincidences (Norton, 1987), which are represented by the points of a Lorentzian manifold. In Einstein’s own words: “..” (Einstein, 1916, 1952, p. 117) — emphasis added.
19#
發(fā)表于 2025-3-24 23:04:02 | 只看該作者
20#
發(fā)表于 2025-3-25 03:08:09 | 只看該作者
The Fibre Bundle Framework for Classical General Relativity, manifold (., .) — i.e., by a 4-dimensional manifold . carrying a Lorentzian metric . — which in the presence of gravitational sources would display non-zero curvature. The mathematical description of such manifolds and of associated tensor structures that was available to Einstein in the second dec
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