Time dependent gravitational potential in the universe and some consequences

被引:8
作者
Trencevski, K [1 ]
机构
[1] Fac Nat Sci & Math, Skopje 1000, Macedonia
关键词
Hubble constant; gravitational potential; orbital period; pioneer spacecraft;
D O I
10.1007/s10714-005-0039-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, assuming a linear change of the gravitational potential V in the universe, i.e. Delta V = - c(2)H 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 a(P) 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 - H Theta/3e pi, while the angle from the aphelion to the perihelion is pi + H Theta/3e pi, where Theta is the orbital period. There is no perihelion precession caused by the time dependent gravitational potential V. The quotient of two consecutive orbital periods Theta(1) and Theta(2) is equal to Theta(2): Theta(1) = 1+ Theta H/3. This formula is tested for the pulsars B1885+ 09 and B1534+12, and the results are good.
引用
收藏
页码:507 / 519
页数:13
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