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Main Author: Carreon, Gabriel, Rene
Format: Recurso digital
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Published: Zenodo 2026
Online Access:https://doi.org/10.5281/zenodo.18528443
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author Carreon, Gabriel, Rene
author_facet Carreon, Gabriel, Rene
contents <p><strong><em><span>The following document outlines the theoretical framework of the Dark Matter Aftermath (DMAfter). Please be advised that while the cosmological theory is public, the High-Resolution Calibration Tables and Scaling Coefficients required for hardware-level integration (CERN/LHC, GNSS, Satellite Nav) are held as Proprietary Trade Secrets. Commercial or institutional use of these precision datasets requires a formal license. Contact Gabriel Carreon for MNDA and Licensing terms. © Gabriel Carreon 2026</span></em></strong></p> <p> </p> <p>How the stellar physics of a Supernova changes under the DMafter Model </p> <p> </p> <p>Gabriel Carreon 2-7-26</p> <p>Dark matter Aftermath Theory</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_18528443
institution Zenodo
language
publishDate 2026
publisher Zenodo
record_format zenodo
spellingShingle The Supernova Luminosity-Gravity Coupling
Carreon, Gabriel, Rene
<p><strong><em><span>The following document outlines the theoretical framework of the Dark Matter Aftermath (DMAfter). Please be advised that while the cosmological theory is public, the High-Resolution Calibration Tables and Scaling Coefficients required for hardware-level integration (CERN/LHC, GNSS, Satellite Nav) are held as Proprietary Trade Secrets. Commercial or institutional use of these precision datasets requires a formal license. Contact Gabriel Carreon for MNDA and Licensing terms. © Gabriel Carreon 2026</span></em></strong></p> <p> </p> <p>How the stellar physics of a Supernova changes under the DMafter Model </p> <p> </p> <p>Gabriel Carreon 2-7-26</p> <p>Dark matter Aftermath Theory</p>
title The Supernova Luminosity-Gravity Coupling
url https://doi.org/10.5281/zenodo.18528443