The Heisenberg limit at cosmological scales
arXiv:2112.07359 · doi:10.1007/s10701-021-00531-z
Abstract
For an observation time {equal to} the universe age, the Heisenberg principle fixes the value of the smallest measurable mass at kg and prevents to probe the masslessness for any particle using a balance. The corresponding reduced Compton length to is $\lambdabar_{\rm H}$, and represents the length limit beyond which masslessness cannot be proved using a metre ruler. In turns, $\lambdabar_{\rm H}$ is equated to the luminosity distance which corresponds to a red shift . When using the Concordance-Model parameters, we get Gpc and . Remarkably, falls quite short to the radius of the {\it observable} universe. According to this result, tensions in cosmological parameters could be nothing else but due to comparing data inside and beyond . Finally, in terms of quantum quantities, the expansion constant reveals to be one order of magnitude above the smallest measurable energy, divided by the Planck constant
A different view on the Hubble tension. To appear in final form on Foundations of Physics by Springer, as follow-on of Capozziello S., Benetti M., Spallicci A.D.A.M., 2020, Found. Phys., 50, 893
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