Difference between revisions of "Light Speed as a Function of Gravitational Potential"
Jump to navigation
Jump to search
(Imported from text file) |
(Imported from text file) |
||
| Line 12: | Line 12: | ||
==Abstract== | ==Abstract== | ||
| − | '''Summary: '''Beckmann makes the case that light speed is constant with respect to the gravitational field. His model, however, does not specify how the speed varies with such things as the mass of the locally dominant body and its distance from the point of interest. In the present paper, we derive the result from the conservation of energy, and use it to predict the reflection of starlight. The results agree with those of General Relativity Theory, and more importantly with measurement.[[Category:Scientific Paper]] | + | '''Summary: '''Beckmann makes the case that light speed is constant with respect to the gravitational field. His model, however, does not specify how the speed varies with such things as the mass of the locally dominant body and its distance from the point of interest. In the present paper, we derive the result from the conservation of energy, and use it to predict the reflection of starlight. The results agree with those of General Relativity Theory, and more importantly with measurement. |
| + | |||
| + | [[Category:Scientific Paper|light speed function gravitational potential]] | ||
[[Category:Gravity]] | [[Category:Gravity]] | ||
[[Category:Relativity]] | [[Category:Relativity]] | ||
Revision as of 10:38, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Light Speed as a Function of Gravitational Potential |
| Author(s) | Howard C Hayden |
| Keywords | light speed, gravitational potential, GRT, mass, distance, point of interest, atarlight |
| Published | 1990 |
| Journal | Galilean Electrodynamics |
| Volume | 1 |
| Number | 2 |
| Pages | 15-17 |
Abstract
Summary: Beckmann makes the case that light speed is constant with respect to the gravitational field. His model, however, does not specify how the speed varies with such things as the mass of the locally dominant body and its distance from the point of interest. In the present paper, we derive the result from the conservation of energy, and use it to predict the reflection of starlight. The results agree with those of General Relativity Theory, and more importantly with measurement.
