Hubble redshift and the Heisenberg frequency uncertainty: on a coherence (or pulse) time signature in extragalactic light
Richard Lieu

TL;DR
This paper explores the potential to detect a fundamental frequency uncertainty signature in extragalactic light, which could verify the Hubble redshift effect and its consistency with quantum principles.
Contribution
It proposes a novel observational test for the Hubble Law using the Heisenberg frequency uncertainty and pulse time signatures in cosmic light.
Findings
The characteristic time scale for CMB is about 5-15 minutes.
Short-term frequency shifts are below the Heisenberg uncertainty limit.
Observing pulse periodicity could confirm the redshift mechanism.
Abstract
In any Big Bang cosmology, the frequency of light detected from a distant source is continuously and linearly changing (usually redshifting) with elapsed observer's time , because of the expanding Universe. For small , however, the resulting shift lies beneath the Heisenberg frequency uncertainty. And since there {\it is} a way of telling whether such short term shifts really exist, if the answer is affirmative we will have a means of monitoring radiation to an accuracy level that surpasses fundamental limitations. More elaborately, had been `frozen' for a minimum threshold interval before any redshift could take place, i.e. the light propagated as a smooth but {\it periodic} sequence of wave packets or pulses, and decreased only from one pulse to the next, one would then be denied the above forbiddingly precise information…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena · Pulsars and Gravitational Waves Research
