Statistical Physics of Dark and Normal Matter Distribution in Galaxy Formation : Dark Matter Lumps and Black Holes in Core and Halo of Galaxy

TL;DR

This paper explores the statistical physics and phase separation of dark and normal matter in galaxy formation, proposing mechanisms for dark matter collapse into black holes and their observational signatures.

Contribution

It introduces a unified field theory framework to describe dark matter lumps, condensate phases, and black hole formation within galaxies, linking particle physics with astrophysical phenomena.

Findings

Dark matter lumps can collapse into black holes at high densities.

Neutralino condensates may form and lead to black hole creation.

Dark matter black holes can evaporate, producing gamma rays and normal particles.

Abstract

In unified field theory the cosmological model of the universe has supersymmetric fields. Supersymmetric particles as dark and normal matter in galaxy clusters have a phase separation. Dark matter in halos have a statistical physics equation of state. Neutralino particle gas with gravitation can have a collapse of dark matter lumps. A condensate phase due to boson creation by annhillation and exchange can occur at high densities. The collapse of the boson condensate, including neutralinos, into the Schwarzschild radius creates dark matter black holes. Microscopic dark matter black holes can evaporate with Hawking effect giving gamma ray bursts and create a spectrum of normal particles. The phase separation of normal and dark matter in galaxy clusters and inside galaxies is given by statistical physics.