Varying Newton Gravitational “Constant” Cosmology - presented by Dr.-Ing. Clovis Jacinto de Matos

Varying Newton Gravitational “Constant” Cosmology

Dr.-Ing. Clovis Jacinto de Matos

CM
Slide at 08:19
G fluctuations in function of galactic redshift 0.12 data fitted curve The relative fluctuation of G near Active prediction bounds Galactic Nuclei depends on the AGN 3C120 bolometric luminosity Lbol and mass flow 0,08 accretion rate M according to: 0.06 AG/G = 2 Lbol/c2M in the limit Lbol << c2 M. 0.04 A Gaussian law for the relative variation of G 0.02 with respect to the cosmological redshift Z is proposed as being: -0.02 AG/GN = +0.09334 e - -((z-0.09026)/0.03829)2 0.01 0.02 0,03 0.04 0.05 0.06 0,07 0,08 0,09 Distance from Earth in redshift Z
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Summary (AI generated)

The fluctuations of the Schwarzschild horizon, assuming that 100% of the accretion rest mass is converted into energy, indicate that the relative fluctuation of the gravitational constant ( G ) near a black hole's horizon is directly proportional to the volumetric luminosity of the accretion disk and inversely proportional to the accretion mass rate.

When applying this relationship to observed black holes in Active Galactic Nuclei (AGN) across various redshifts, we observe a Gaussian distribution for the relative variation of ( G ) in relation to the galactic redshift ( z ), as illustrated in the bottom left of the slide. This distribution represents the best statistical fit for the calculated ( \delta G / G ). The analysis is based on observational data from multiple AGN at varying redshifts, indicating their distances from Earth.