Geodesic Lines in Fields of Velocity

Abstract

This work is a purely syntactic geometric exploration of some few elements, which are our axioms, that in last instance it is the set of differential equations whose solutions give the geodesic lines of the Schwarzschild spacetime. We observe that non new physics principles or postulates will be introduced in this work. We only link the Bohr's atoms model with the Einstein's relativity through of a common geometric syntax. To obtain this common syntax, we will define the {\it extended Lorentz group}, which is defined to preserve the volume form of the Minkowski spacetime. The Schwarzschild spacetime will be defined as a manifold associated to a set of radial fields of velocities within of the four-dimensional Minkowski vectorially space form. Our procedure includes a comparison of the Newtonian and the Schwarzschild times along geodesic lines. Our constructions have strong influence of the Einstein paper about the energy content produced by fields, as well as by the Schr\"odinger digression about the annihilation of matter. We define the orbital associated to the Kepler's laws as a set of elliptical orbits, which have equal eccentricity and equal major semi-axis. Then identifying the eccentricity with the relativistic velocity we will obtain a thermodynamic equivalence between the increasing of mass in kinetic form in special relativity theory and an adiabatic process with degree of freedom equal to 2. The eccentricity will be the needed velocity to move the revolution ellipsoid and so to obtain a contraction of its major axis such that it converts into a sphere with radius given by the minor semi-axis. Therefore we can associate to the each class of equal eccentricity orbital an unique timelike unit vector, which is called {\it the observer} of class.