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Time dependent gravitational potential in the universe and some consequences
Authors:Kostadin?Tren?evski  author-information"  >  author-information__contact u-icon-before"  >  mailto:kostatre@iunona.pmf.ukim.edu.mk"   title="  kostatre@iunona.pmf.ukim.edu.mk"   itemprop="  email"   data-track="  click"   data-track-action="  Email author"   data-track-label="  "  >Email author
Affiliation:(1) Faculty of Natural Sci. and Math., P.O. Box 162, 1000 Skopje, Macedonia
Abstract:In this paper, assuming a linear change of the gravitational potential V in the universe, i.e. $${rm Delta} V=-c^{2H}{rm Delta} t$$, some consequences are obtained. 1. The Hubble red shift is explained by the potential difference between the considered galaxy long time ago and the observer at this epoch. 2. The anomalous acceleration aP from the spacecraft Pioneer 10 and 11 [1] is explained. 3. The deformations of the trajectories of planets are studied. It is shown that the planetary orbits are not axially symmetric and the angle from the perihelion to the aphelion is $$pi-frac{H{rm Theta}}{3epi}$$, while the angle from the aphelion to the perihelion is $$pi+frac{H{rm Theta}}{3epi}$$, where THgr is the orbital period. There is no perihelion precession caused by the time dependent gravitational potential V. The quotient of two consecutive orbital periods THgr1 and THgr2 is equal to $${rm Theta}_2{:},{rm Theta}_1=1+frac{{rm Theta} H}{3}.$$ This formula is tested for the pulsars B1885+09 and B1534+12, and the results are good.This revised version was published online in April 2005. The publishing date was inserted.
Keywords:Hubble constant  Gravitational potential  Orbital period  Pioneer spacecraft
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