%0 Journal Article
%T A Snapshot of a Homogeneous Spinning Universe
%A Barbaro Quintero-Leyva
%J Open Access Library Journal
%V 5
%N 9
%P 1-11
%@ 2333-9721
%D 2018
%I Open Access Library
%R 10.4236/oalib.1104895
%X <div style="text-align:justify;">
	<span style="line-height:1.5;">A snapshot of the circular speed as a function of the radius in a spin-ning-homogeneous spherical universe was obtained using a mass-dependent characteristic-acceleration in the Modified Newtonian Dynamics (MOND paradigm as a modified 2nd law of Newton) with and without considering the impact of the relativistic speed. To consider the impact of the relativistic speed the Extended Newtonian Theory (E</span><span style="line-height:1.5;">NET), previously developed by the author, was used. The corresponding kinetic energy equation for ENET is however reported in this work for the first time. The speed profile shows a non-linear trend with features that has been experimentally noted before. It was shown that the Hubble law (for circular speeds) can be inferred from the results for a distance range close to the experimental results of the Hubble telescope key project. The calculation considering the impact of the relativistic speeds yields a very distinctive tail towards the edge of the universe that has been noted before. It is striking that a spinning universe model yields (without any reference to dark matter or dark energy) observed features of a universe which, based on photometric and spectral line measurements, is currently interpreted as radially expanding at an accelerated rate.</span>
</div>
%K Celestial Mechanics
%K Newtonian Gravitation
%K Newton¡¯s 2<sup>nd</sup> Law
%K Theory of Relativity
%K Perihelion Precession
%K Cosmology
%U http://www.oalib.com/paper/5299838