Authors: Tony Bermanseder
The experimental data collected by the various supernova observers, and under utility of the Hubble Space Telescope to track the brightness variations of discovered supernovae type Ia, now converged in 1998 to the conclusion, that distant supernovae are between 20% and 30% dimmer than expected and as a consequence of their measured redshift they appear to be further away than theory permits. An interpretation of this discovery implies, that the universe's expansion is accelerating; the measured redshift depicting a distance further away for a dimmer brightness than anticipated by theory. Closer analysis of the redshift data shows an expected distribution of luminosity, calibrated to their distances in the Chilean Cala-Tololo data, up to a redshift of about 0.11 and with a redshift-gap until a redshift of 0.3; after which the 'High-Z's' begin to show the 'curving away' from a predicted decelerating expansion rate in concordance with an Euclidean flat universe of Einsteinian General Relativity. The highest redshift recorded in 1998 was that of 'supernova Iae' at (z=1.1) by the 'High-Z-Team'. Why is there a redshift gap between z=0.11 and z=0.30 approximately? Does this imply a scarcity of supernovas in this redshift interval or is there a cosmological reason for this gap? Is this cosmological reason at the core of the Dark Energy implication and the 'factuality' of an accelerating universe? This treatise shall elucidate the cosmological nature of Dark Energy and the inferred accelerating cosmology of an accelerating universe, stipulated to begin some 5-6 Billion years ago and as a change from a measured deceleration from light speed in the early universe.
Comments: 40 Pages.
[v1] 2019-05-18 18:07:48
Unique-IP document downloads: 19 times
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