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

Lobsang Dhargyal

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arXiv · 1901.10940

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

Lobsang Dhargyal

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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.

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Lobsang Dhargyal. 2024-10-19. Phenomenology of a universal super weak $SU(N)_{w}$ color hypothesis. https://arxiv.org/abs/1901.10940

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