Quantum Cosmology Explains the General Galaxy-Black Hole Correlation ()
ABSTRACT
The symmetric quantum physics of the Universe demonstrates that the massive black holes developing in the post-inflation big-bang prompt the formation of the host galaxies around them. A general correlation between the variety of galaxies and black holes develops, a specific example of which is the celebrated (but not understood) mass correlation between the host elliptical galaxies and their core black holes. The elucidations and predictions in this exposition are inclusive and far-reaching, resolving a myriad of yet unsolved problems and quandaries in the evolving Universe, among which are: how the general galaxy-black hole correlations are established; what is the role of the dark matter and energy in the formation of galaxies and stars; how the spiral galaxies with less predominant black holes are formed; how the early star forming globular cluster emerged with sparse dark matter; why some galaxy mergers give rise to the starbursts, while other mergers switch the star flourishing galaxies off into grave yards; and how could the Universe have wound up as sheets and filaments of galaxy clusters encompassing great voids.
Share and Cite:
P. Suh, "Quantum Cosmology Explains the General Galaxy-Black Hole Correlation,"
International Journal of Astronomy and Astrophysics, Vol. 2 No. 2, 2012, pp. 101-112. doi:
10.4236/ijaa.2012.22014.