# Phenomenology of a universal super weak $SU(N)_{w}$ color hypothesis

**Authors:** Lobsang Dhargyal

arXiv: 1901.10940 · 2024-10-22

## TL;DR

This paper proposes a universal super weak $SU(N)_w$ color interaction that could explain galaxy rotation anomalies, dark matter, dark energy, and aspects of particle physics without introducing new particles.

## Contribution

It introduces a novel $SU(N)_w$ color interaction with a confining radius comparable to galaxies, offering explanations for dark matter, dark energy, and cosmological phenomena.

## Key findings

- Could explain galaxy rotation velocity anomalies without dark matter particles.
- May account for most of the galaxy mass through color interaction dynamics.
- Potentially explains Big Bang, Hubble's law, dark energy, and neutrino oscillations.

## Abstract

In this work we will propose a new universal super weak $SU(N)_{w}$ (or self interacting vector bosons) color to which all the SM fermions are assumed to be coupled universally whose confining radius is in the range of the size of galaxies. We will argue that the model has some very interesting consequences such as it could be able to explain the observed rotation velocity anomalies in large galaxies without requirement of specific DM particle. We will also show that it could constitute most of the observed mass of a galaxy, similar like the proton mass which is mostly made up of color interaction dynamics as shown recently, which could explain the observed DM in the rotation velocities of galaxies in galaxy clusters. Also when the N is very small, we will show that it could explain the Big Bang and Hubble's law, Dark Energy, and tentatively also flavor and neutrino oscillation.

## Full text

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## Figures

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## References

6 references — full list in the complete paper: https://tomesphere.com/paper/1901.10940/full.md

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Source: https://tomesphere.com/paper/1901.10940