On The Possibility Of Relativistic Shock-Wave Effects In Observations of Quasar Luminosity

Mathematics – Logic

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Scientific paper

A growing number of conflicts within the Standard Model call into question the fundamental interpretation of the Doppler component of the Hubble Expansion Law and the nature of events in spacetime associated with conventional coordinates of the line element attached to the observer. We postulate that nonlinear effects associated with the propagation of light in a gravitational field can produce shock waves at cosmological distances approaching the limit of observation. These gravitational shock waves are manifest observationally in the spectrum of QSO's and Supernova as a continuous array of light booms' produced by superluminal boosts associated with continuous coordinate transformations relative to a distant observer. This model suggests that QSOS are most likely a form of Seifert spiral galaxies with active galactic nuclei (AGN) in the vicinity of the observational limit of the Hubble radiius.

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