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Propagation of signals in spaces with affine connections and metrics as models of spacetime

机译:信号在带仿射连接和度量的空间中的传播作为时期的模型

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The propagation of signals in spacetime is considered on the basis of the notion of null (isotropic) vector field in spaces with affine connections and metrics [((L) over bar (n), g) spaces] as models of space or spacetime. The Doppler effect is generalized for these types of spaces. The notions of aberration, standard (longitudinal) Doppler effect, and transverse Doppler effect are introduced. On their grounds, the Hubble effect appears as Doppler effect with explicit forms of the centrifugal (centripetal) and Coriolis velocities and accelerations in spaces with affine connections and metrics. Doppler effect, Hubble effect, and aberration could be used in mechanics of continuous media and in other classical field theories in the same way as the standard Doppler effect is used in classical and relativistic mechanics.
机译:基于具有仿射连接和度量的空间中的空隙(各向同性)矢量场的概念来考虑信号的传播,以带仿射连接和度量的空间[((l)栏(n),g)空间,作为空间或时空的模型。 多普勒效应是广泛的,用于这些类型的空间。 引入了像差,标准(纵向)多普勒效应和横向多普勒效应的概念。 在理由上,哈勃效果表现为多普勒效应,具有与仿射连接和指标的空间中的离心(离心机)和科里奥利速度和加速度。 多普勒效应,哈勃效应和像差可用于连续介质的力学和其他经典田间理论,与标准多普勒效应在经典和相对论的力学中使用相同的方式。

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