Correlation of energy density in deconfining SU(2) Yang-Mills thermodynamics

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.

22 pages, 8 figures, v6: formulas (6), (7), (11), (12), (18), (20) altered, figures (2), (6), (7), (8) altered, figures (1), (4), (5) exchanged, no qualitative changes in the results and no change of our conclusions

References in corpus (5)

• The Transition from Atomic to Molecular Hydrogen in Interstellar Clouds: 21cm Signature of the Evolution of Cold Atomic Hydrogen in Dense Clouds
• A Cold Nearby Cloud Inside the Local Bubble
• Radiative corrections to the pressure and the one-loop polarization tensor of massless modes in SU(2) Yang-Mills thermodynamics
• Irreducible three-loop contributions to the pressure in Yang-Mills thermodynamics
• Black-Body Anomaly: Analysis of Temperature Offsets