Dark Matter, Cosmic Positrons in Alpha Magnetic Spectrometer Experiment and Particle-Cosmology with Yang-Mills Gravity
Jong-Ping Hsu, Leonardo Hsu

TL;DR
This paper proposes a high-energy anti-electron-neutrino dark matter model based on Lee-Yang's leptonic force, explaining cosmic positron excesses and suggesting new experimental tests for leptonic interactions.
Contribution
It introduces a novel neutrino-based dark matter model with leptonic force, linking particle physics, cosmology, and cosmic-ray observations, and predicts measurable effects in experiments.
Findings
Anti-electron-neutrinos could account for flat galaxy rotation curves.
The model explains AMS positron excess via neutrino-proton interactions.
Leptonic charge estimated at approximately 7 x 10^{-21}.
Abstract
We discuss a model of dark matter consisting of high energy anti-electron-neutrinos with leptonic force, which is produced by the conserved leptonic charge associated with Lee-Yang's gauge symmetry. Based on particle-cosmology for early universe, the high energy neutrino (HEN) model of dark matter assumes that the neutron decay processes, , dominate the epoch after the creation, collision and confinement processes of quarks and antiquarks in the beginning. The HEN model implies the following results: There are almost equal numbers of electrons, protons and anti-electron-neutrinos dominated the matter cosmos. There are unobservable and ubiquitous anti-electron-neutrinos with leptonic charge in the universe. Although the total mass of anti-electron-neutrino dark matter is negligible in the universe, its enhanced…
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