Correlation of energy density in deconfining SU(2) Yang-Mills thermodynamics
Jochen Keller, Ralf Hofmann, and Francesco Giacosa
TL;DR
This paper calculates the energy density correlation in deconfining SU(2) Yang-Mills thermodynamics, suggesting potential applications to cold atomic hydrogen clouds in the Milky Way.
Contribution
It presents a novel computation of energy density correlations in a specific gauge theory relevant to astrophysical phenomena.
Findings
Correlation of energy density computed for massless modes
Potential implications for understanding atomic hydrogen clouds
Provides a theoretical basis for astrophysical applications
Abstract
We compute the two-point correlation of the energy density for the massless mode in deconfining SU(2) Yang-Mills thermodynamics and point towards a possible application for the physics of cold, dilute, and stable clouds of atomic hydrogen within the Milky Way.
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