There has been a renewed interest in the recent years in the possibility of deviations from the predictionsof Newton’s “inverse-square law” of universal gravitation.One of the reasons for renewing this interest lies in various theoretical attempts to construct a unified elementary particle theory, in which there is a natural prediction of new forces over macroscopic distances. Therefore the existence of such a force would only coexist with gravity, and in principle could only be detected as a deviation from the inverse square law, or in the “universality of free fall” experiments.New experimental techniques such that of Sagnac interferometry can help explore the range of the Yukawa correction λ ≥ 10^14 m where such forces might be present. It may be,that future space missions might be operating in this range which has been unexplored for very long time. To study the effect of the Yukawa correction to the gravitational potential and its corresponding signal delay in the vicinity of the Sun, we use a spherically symmetric modified space time metric where the Yukawa correction its added to the gravitational potential. Next, the Yukawa correction contribution to the signal delay is evaluated. In the case where the distance of closest approach is much less than the range λ, it results to a signal time delay that satisfies the relation t (b <λ)∼=37.7t (b = λ).
Comments: 4 Pages. NA
[v1] 2012-10-13 22:54:43
Unique-IP document downloads: 0 times
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.