Stellar Collapse: Difference between revisions
Add to Category:Emission Theory |
Correct num_pages from the actual PDF |
||
| Line 8: | Line 8: | ||
| volume = [[1]] | | volume = [[1]] | ||
| number = [[7]] | | number = [[7]] | ||
| num_pages = | | num_pages = 12 | ||
| pages = 4-7 | | pages = 4-7 | ||
}} | }} | ||
Revision as of 09:04, 21 July 2026
| Scientific Paper | |
|---|---|
| Title | Stellar Collapse |
| Read in full | Link to paper |
| Author(s) | Richard A Waldron |
| Keywords | stellar collapse, ballistic theory of light |
| Published | 1990 |
| Journal | Apeiron |
| Volume | 1 |
| Number | 7 |
| No. of pages | 12 |
| Pages | 4-7 |
Read the full paper here
Abstract
The phenomenon of stellar collapse is considered from the viewpoint of the neo-Newtonian ballistic theory of light. The restrictions of the special theory of relativity are thus removed. The theory predicts that a collapsing star will expand again, and continue to alternately expand and collapse at a rate depending on the mass and greatest radius of the star. On each cycle material will be lost, including photons which appear to distant observers as the emissions of a pulsar. It is concluded that pulsars are oscillating stars, that these eventually "evaporate" away completely, and that there is no such object as a black hole.