Abstract
Condensed Neutrino Objects (CNO) are a candidate for the Dark Matter which everyone has been looking for. In this article, from Albert Einstein’s original 1911 and 1917 papers, we begin the journey from weak lensing data to neutrino signatures. New research results include an Einasto density profile that fits to a range of candidate degenerate neutrino masses, goodness-of-fit test results for our functional CNO mass/radius relationship which fits to available weak lensing data, and new results based on revised constraints for the CNO that our Local Group of galaxies is embedded in.
Highlights
[12] isto differentiate these different types and, since we spectroscopically, no measurement can be made are only interested in the mass and 4radius large objects, we describe them by setting the h of these i neutrino Fermi momentum the anti-neutrino Fermi momentum
Mathematica used to provide new results additional applicable weak lensing observational data, and using Mathematica® to provide for a number of commonly used goodness-of-fit tests for our functional form
After routinely scouring the literature for applicable galaxy cluster data with virial mass and radii estimates we present additional data in Table 4 using the following nomenclature/notes: (1) WL is weak lensing data that uses an estimated Dark Matter velocity dispersion based on tangential shear measurements
Summary
If Dark Matter is made up of boson particles, they must have an internal energy source Since these bosons would have been created at the time of the Big Bang, the expansion of the Universe would have cooled them down to very low energies. They would fall into the lowest energy state and their aggregate cloud would be hydro-statically unstable; they would end up as a Black Hole. Cosmological neutrinos and anti-neutrinos were created in the original Big Bang, in almost unlimited numbers1 If they should condense, they would make excellent Dark Matter particle candidates. The expansion of the universe is not sufficient by itself for neutrino and anti-neutrino condensation
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