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April 6, 20260 citationsOpen Access

Subluminal eV-Scale Neutrino Tails from Core-Collapse Supernovae as Triggers for VEI 6–7 Volcanic Eruptions: A 6/6 Correlation and Beyond-Standard-Model Mechanism

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DSDon Stenberg

Key Points

  • This research examines the correlation between core-collapse supernovae and volcanic activity, exploring potential mechanisms for energy transfer.
  • Analyzed data from six core-collapse supernovae within 12,000 light-years
  • Used Gaussian Monte Carlo simulation to assess significance of correlations
  • Examined potential beyond-standard-model physics for energy transmission
  • Identified significant correlation with volcanic eruptions occurring 30-100 years after supernovae
  • Simulation yielded results indicating increasing significance of correlation based on threshold
  • Proposed mechanisms involving low-energy neutrino interactions could trigger volcanic events

Abstract

The complete sample of six well-documented core-collapse supernovae (CCSNe) with reliable age and distance estimates within 12, 000 light-years over the last 4, 200 years shows a temporal correlation with VEI 6. 5–7 volcanic eruptions, with delays of 30–100 years. This delay matches subluminal velocities (98–99. 9%c) for eV-scale particles, not relativistic propagation. A Gaussian Monte Carlo simulation—propagating all age uncertainties and requiring eruptions after supernovae—yields p (6+) = 5. 58 × 10^−3 (2. 5σ) for nine CCSNe in the sample. For higher match thresholds, significance increases: p (7+) = 3. 80 × 10^−4 (3. 4σ), p (8+) = 3. 00 × 10^−5 (4. 2σ), and p (9+) 4. 5σ). If this correlation reflects causation, what physical processes could transmit energy from a CCSN to Earth on decadal timescales? We explore whether beyond-Standard-Model physics could, in principle, account for the observed delays and localized heating. A low-energy (eV-scale) neutrino tail from the CCSN—generated via sterile neutrino oscillations, plasmon decay enhanced by a light Z′, or Bremsstrahlung enhanced by an energy-dependent magnetic moment—could meet the required criteria. Coherent neutrino-nucleus scattering would perturb 40K nuclei, temporarily enhancing electron capture (40K + e− →40Ar + νe), amplifying eV triggers into MeV energy release. Random walk transport through the mantle (λ ∼ 10–100 m) would yield ∼ 10^9–10^11 scatters per neutrino and ∼ 10^4–10^6 triggered decays per neutrino. Deposited energy (∼ 10^13–10^17 J) would raise local magma chamber temperatures by ∼ 10–100 K —potentially sufficient to destabilize pressurized chambers and trigger eruptions. If causal, the model would make a falsifiable prediction: a VEI 6. 5–7+ eruption and low-energy neutrino signals within 8 months to 13 years of a Betelgeuse supernova (∼ 650 ly). The required BSM parameter space lies near or beyond current experimental bounds and should be regarded as speculative. The statistical correlation stands independently; failure of any specific mechanism would not invalidate the correlation, but would instead imply either non-causality or a different physical process.

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Cite This Study

Don Stenberg (2026) studied this question.

synapsesocial.com/papers/69d34e579c07852e0af97f2ehttps://doi.org/10.5281/zenodo.19413204
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