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Bibliographic Details
Main Author: Wipfler, Karl Heinz
Format: Recurso digital
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Published: Zenodo 2026
Online Access:https://doi.org/10.5281/zenodo.18405343
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  • <p>This paper derives the neutrino mass <span><span><span><span><span><span>m</span><span><span><span><span><span><span><span>ν</span></span></span></span><span></span></span></span></span></span></span></span></span></span> not as a statistical fit but as a necessary consequence of field tension and the 137-resonance. Based on the arrival time data from supernova SN1987A, Karl Heinz Wipfler demonstrates that previous uncertainties in neutrino physics result from using a "slowed" speed of light. Through TFD normalization to <span><span><span><span><span><span>c</span><span><span><span><span><span><span><span>0</span></span></span></span><span></span></span></span></span></span><span>=</span></span><span><span>300</span><span>,</span><span>000</span></span></span></span></span> km/s and the application of the field amplitude <strong><span><span><span><span><span>A</span><span>=</span></span><span><span><span>m</span><span><span><span><span><span><span><span>1/2</span></span></span></span></span></span></span></span></span></span></span></span></strong>, a precise anchor value of 0.041 eV is obtained. This value is fully compatible with current KATRIN measurement data (<span><span><span><span><span><</span></span><span><span>0.45</span></span></span></span></span> eV) and resolves the discrepancy between cosmology and particle physics without free parameters.</p>