Heat expansion of star-like cosmic objects induced by the cosmological expansion
arXiv:astro-ph/0201007 · doi:10.1002/1521-3994(200110)322:4<207::AID-ASNA207>3.0.CO;2-C
Abstract
The heat expansion of a star-like cosmic object, induced by the cosmological bremsheat production within a moving body, that was predicted by the Projective Unified field Theoriy of the author, is approximately treated. The difference to planet-like bodies investigated previously arises from another material constitution. The exponential-like expansion law is applied to a model with numerical values of the Sun. The results are not in contradiction to empirical facts.
7 pages, 4 figures, Latex