Difference between revisions of "An Astronomy Model within an Infinite Universe"

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[[Category:Scientific Paper|astronomy model infinite universe]]
 
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[[Category:Gravity|astronomy model infinite universe]]

Latest revision as of 19:17, 1 January 2017

Scientific Paper
Title An Astronomy Model within an Infinite Universe
Author(s) Eit Gaastra, Cynthia Kolb Whitney
Keywords infinite universe, galaxies, stars, pulsars, AGN
Published 2004
Journal Proceedings of the NPA
Volume 1
Number 1
No. of pages 4
Pages 21-24

Abstract

In a Universe infinite in space and time, Population II stars may blacken, cool down, assemble hydrogen, and ignite as Population I stars, which finally blacken too, assemble hydrogen, etc. In this way, stars with very big heavy-element cores may come to existence, which may explain the intrinsic (gravitational) redshift of white dwarfs as well as the intrinsic (gravitational) redshift of bright blue stars. When celestial objects (with heavy elements) become very big, the gravitational contraction may become so high that endothermic reactions start: elements may fuse into elements higher than iron while absorbing low temperature (CBR) radiation, which may explain pulsars. When celestial objects become extremely big, then a reaction may start that turns elements higher than iron into very small elements, mainly HII and electrons, which then may explain radio loud activity by AGNs. Shrunken remnants of old galaxies may become the nuclei of new galaxies as well as the nuclei of AGNs. The cause of solar system formation may by objects (future planets) that travel through interstellar space, attracted to stars.