Chaffin, Eugene F. (2017) Variable Neutrino Mass, Supernovae, and Accelerated Decay. Creation Research Society Quarterly, 53 (3): 4.
Variable Neutrino Mass, Supernovae, and Accelerated Decay.pdf
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Abstract
The antineutrino flux from radioactive uranium, thorium, potassium-40, etc. on the earth’s surface is of the order of 106 antineutrinos per square centimeter per second. The flux of neutrinos from the sun is four orders of magnitude larger. Larger than that would be the cosmic background of neutrinos and the possibility of a nearby supernova. Recent physics literature contains theories in which the neutrino mass is coupled to the neutrino density via a so-called acceleron field. This acceleron field is hypothesized to resemble the Higgs field, and to change strength due to neutrino couplings and variation in neutrino density. The radiocarbon evidence for a nearby supernova is discussed and related to the possibility that such a supernova showered the earth at the time of Noah’s Flood. This would contribute to accelerated decay and provide evidence that radioisotope data can be consistent with a biblical timescale.
Item Type: | Article |
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Subjects: | Q Science (General) > QC Physics > QC770 Nuclear and Particle Physics. Atomic Energy. Radioactivity Q Science (General) > QB Astronomy > QB495 Descriptive astronomy > QH491.1 Solar System Q Science (General) > QE Geology > QE508 Geochronometry > QE508.1 Radiometric Dating. Carbon Dating |
Depositing User: | Admin |
Date Deposited: | 18 Mar 2025 21:46 |
Last Modified: | 18 Mar 2025 21:46 |
URI: | https://crsq.creationresearch.org/id/eprint/1204 |