小样他闲聊
发表于 2025-3-23 13:46:30
http://reply.papertrans.cn/79/7813/781209/781209_11.png
积极词汇
发表于 2025-3-23 16:08:01
http://reply.papertrans.cn/79/7813/781209/781209_12.png
Conquest
发表于 2025-3-23 18:27:59
http://reply.papertrans.cn/79/7813/781209/781209_13.png
ethnology
发表于 2025-3-23 22:35:39
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.
杀人
发表于 2025-3-24 05:21:23
http://reply.papertrans.cn/79/7813/781209/781209_15.png
helper-T-cells
发表于 2025-3-24 10:17:39
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.
繁重
发表于 2025-3-24 14:37:50
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.
不能和解
发表于 2025-3-24 15:20:02
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.
ETHER
发表于 2025-3-24 23:04:02
http://reply.papertrans.cn/79/7813/781209/781209_19.png
牲畜栏
发表于 2025-3-25 03:08:09
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