Stellar Collapse: Difference between revisions
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| published = 1990 | | published = 1990 | ||
| journal = [[Apeiron]] | | journal = [[Apeiron]] | ||
| volume = | | volume = 1 | ||
| number = | | number = 7 | ||
| num_pages = 12 | | num_pages = 12 | ||
| pages = 4-7 | | pages = 4-7 | ||
Revision as of 09:29, 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.