Overview

We consider the case of an effective river of mass flow or matter flow for which the heat flux vector is non-zero and the viscous shear is zero and also the case of non-zero viscous shear. For purposes of modeling, we will first consider a linear array of solid rotating cylindrical disks for which each disk is composed of a form of shadow matter that only interacts with the gravitation of the adjacent disks that overlap in space. Here, we will assume that there is systemic pressure in that the rotating disks have rotational velocities such that the self-induced gravitational attractive pressures of the disks are not cancelled out as a result of centripetal acceleration. We further assume a similar linear array of disks rotating in the opposite direction but where there is a non-overlapped portion which essentially mimics a linear unidirectional massive river flow. A simulated space-time-mass-energy river may be applicable to methods of superluminal travel. For example, a spacecraft traveling down such river might have a velocity of its relative velocity with respect to the river added to the effective river current velocity. It is plausible that the river velocity may be modulated to have an arbitrary group velocity and phase velocity thereby enabling effectively arbitrarilly great super-luminal river currents with respect to the background. Herein, the solutions are explained with prose so as to cover tremendously large numbers of specific solutions for each of numerous contemplated classes of solutions.

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9781518795459

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