Authors: Ramzi Suleiman
Many previous attempts have been undertaken to produce a singularity-free solution to the black hole problem. This effort included many “Bardeen black hole” models, as well as quantum mechanical, and string theory models. The present paper describes a new solution based on a relativistic extension of Newton-Galileo physics, termed Information Relativity theory. For a purely gravitational, spherical black hole, the theory yields a black hole radius that equals the Schwarzschild radius, but without an interior singularity. Moreover, for a typical galaxy with a supermassive black hole residing at its center, the model produces a simple expression for the galaxy's dynamics in its dependence on redshift. According to the emerging dynamics, a galaxy's supermassive black hole is part of a binary system, together with a naked singularity at redshift z = 2 -1/2 ≈ 0.707, suspected to be a quasar with extreme velocity offsets or an active galactic nucleus (AGN). Another redshift, z ≈ 2.078, is also predicted to be associated with quasars and AGNs. The derived results are contrasted with observational data and with a recent ΛCDM model. Taken together, the produced galaxy dynamics and the aforementioned results could shed some light on the role of supermassive black holes in the evolution of the galaxies in which they reside. The success of Information Relativity in reproducing the Schwarzschild radius of black holes, together with previous successful predictions of the phenomena of light bending, gravitational redshift, dark matter, and dark energy, attest the possibility of constructing a simple cosmology, based only on physical variables, without the notion of space time and its geodesics.
Comments: 14 Pages.
[v1] 2017-11-25 02:31:50
Unique-IP document downloads: 34 times
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