Supernova Neutrino Signal Timing Through a Bounce Frame
This paper computes a specific neutrino quantity in a cosmology whose collapse is regulated by a maximum density, the Aldred Limit evaluated on its neutron branch at 9.72e+54 grams per cubic centimetre. A galactic supernova will deliver roughly ten thousand neutrino events over about ten seconds, with energies between five and fifty megaelectronvolts. The arrival-time structure encodes the neutrino mass, the distance, and any additional propagation effect accumulated over the journey. The calculation gives the following headline values: distance_kpc = 10, mass_eV = 0.05, energy_MeV = 15, mass_delay_s = 5.718173613219375e-06, burst_duration_s = 10.0, delay_fraction = 5.718173613219375e-07. Each value is obtained from stated assumptions by the deposited script and is compared with published observational values where such values exist. Where the computed frame effect is far below observational reach, that negative result is stated plainly rather than softened. This study is simulated and computed from stated assumptions; it is not a measurement.
Authors
- William Alexander Aldred (ORCID: https://orcid.org/0009-0000-1215-577X)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-11-11
- DOI
- https://doi.org/10.5281/zenodo.24129941
- Primary Topic
- Neutrino Physics Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00