Scalar potential model of redshift and discrete redshift
Abstract
On the galactic scale the universe is inhomogeneous and redshift is occasionally less than zero. A scalar potential model (SPM) that links the galaxy scale to the cosmological scale of the Hubble Law is postulated. Several differences among galaxy types suggest that spiral galaxies are Sources and that early type, lenticular, and irregular galaxies are Sinks of a scalar potential field. The morphology-radius and the intragalactic medium cluster observations support the movement of matter from Source galaxies to Sink galaxies. A cell structure of galaxy groups and clusters is proposed to resolve a paradox concerning the scalar potential like the Olber's paradox concerning light. For the sample galaxies, the ratio of the luminosity of Source galaxies to the luminosity of Sink galaxies approaches . An equation is derived from sample data, which is anisotropic and inhomogeneous, relating of and the distance to galaxies. The calculated has a correlation coefficient of 0.88 with the measured for a sample of 32 spiral galaxies with calculated using Cepheid variable stars. The equation is consistent with observations of close galaxies. At low cosmological distances, the equation reduces to , where is a constant, positive value. The equation predicts from galaxies over 18 Gpc distant approaches a constant value on the order of 500. The SPM of provides a physical basis for the of particle photons. Further, the SPM qualitatively suggests the discrete variations in , which was reported by W. G. Tifft, 1997, Astrophy. J. 485, 465 and confirmed by others, are consistent with the SPM.
Keywords
Cite
@article{arxiv.astro-ph/0602344,
title = {Scalar potential model of redshift and discrete redshift},
author = {John C. Hodge},
journal= {arXiv preprint arXiv:astro-ph/0602344},
year = {2009}
}
Comments
36 pages, 17 figures, Article in press New Astronomy