Introducing Distance and Measurement in General Relativity: Changes for the Standard Tests and the Cosmological Large-Scale: Difference between revisions
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{{Infobox paper | {{Infobox paper | ||
| title = Introducing Distance and Measurement in General Relativity: Changes for the Standard Tests and the Cosmological Large-Scale | | title = Introducing Distance and Measurement in General Relativity: Changes for the Standard Tests and the Cosmological Large-Scale | ||
| url = [https://web.archive.org/web/20100927172524/http://ptep-online.com/index_files/2005/PP-03-07.PDF Link to paper (Internet Archive)] | |||
| author = [[Stephen John Crothers]] | | author = [[Stephen John Crothers]] | ||
| keywords = [[Distance]], [[Measurement]], [[General Relativity]], [[Cosmology]] | | keywords = [[Distance]], [[Measurement]], [[General Relativity]], [[Cosmology]] | ||
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| pages = 41-47 | | pages = 41-47 | ||
}} | }} | ||
'''Read the full paper''' [https://web.archive.org/web/20100927172524/http://ptep-online.com/index_files/2005/PP-03-07.PDF here] ''(archived copy — the original link is no longer available)'' | |||
==Abstract== | ==Abstract== | ||
Revision as of 08:29, 20 July 2026
| Scientific Paper | |
|---|---|
| Title | Introducing Distance and Measurement in General Relativity: Changes for the Standard Tests and the Cosmological Large-Scale |
| Read in full | Link to paper (Internet Archive) |
| Author(s) | Stephen John Crothers |
| Keywords | Distance, Measurement, General Relativity, Cosmology |
| Published | 2005 |
| Journal | Progress In Physics |
| Volume | 3 |
| Pages | 41-47 |
Read the full paper here (archived copy — the original link is no longer available)
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.