Difference between revisions of "Introducing Distance and Measurement in General Relativity: Changes for the Standard Tests and the Cosmological Large-Scale"
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| − | Relativistic motion in the gravitational field of a massive body is governed by the external metric of a spherically symmetric extended object. Consequently, any solution for the point-mass is inadequate for the treatment of such motions since it pertains to a fictitious object. I therefore develop herein the physics of the standard tests of General Relativity by means of the generalised solution for the field external to a sphere of incompressible homogeneous fluid.</p></span></span>[[Category:Scientific Paper]] | + | Relativistic motion in the gravitational field of a massive body is governed by the external metric of a spherically symmetric extended object. Consequently, any solution for the point-mass is inadequate for the treatment of such motions since it pertains to a fictitious object. I therefore develop herein the physics of the standard tests of General Relativity by means of the generalised solution for the field external to a sphere of incompressible homogeneous fluid.</p></span></span> |
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| + | [[Category:Scientific Paper|introducing distance measurement general relativity changes standard tests cosmological large-scale]] | ||
[[Category:Relativity]] | [[Category:Relativity]] | ||
Revision as of 10:34, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Introducing Distance and Measurement in General Relativity: Changes for the Standard Tests and the Cosmological Large-Scale |
| Author(s) | Stephen John Crothers |
| Keywords | Distance, Measurement, General Relativity, Cosmology |
| Published | 2005 |
| Journal | Progress In Physics |
| Volume | 3 |
| Pages | 41-47 |
Abstract
Relativistic motion in the gravitational field of a massive body is governed by the external metric of a spherically symmetric extended object. Consequently, any solution for the point-mass is inadequate for the treatment of such motions since it pertains to a fictitious object. I therefore develop herein the physics of the standard tests of General Relativity by means of the generalised solution for the field external to a sphere of incompressible homogeneous fluid.
