Exact determination of asymptotic CMB temperature-redshift relation
Steffen Hahn, Ralf Hofmann

TL;DR
This paper derives the high-temperature-redshift relation coefficient for the CMB using a theoretical model based on a deconfining SU(2) gauge theory, revealing a topological invariant closely related to the 3D Ising model's critical exponent.
Contribution
It provides a novel theoretical calculation of the CMB temperature-redshift coefficient using nonperturbative gauge theory and topological invariants, linking cosmological observations to fundamental physics.
Findings
Calculated $ u_{CMB} = (1/4)^{1/3} \\approx 0.63
Found $ u_{CMB}$ closely matches the 3D Ising model's critical exponent
Established a topological invariant in the CMB temperature relation
Abstract
Based on energy conservation in a Friedmann-Lemaitre-Robertson-Walker (FLRW) Universe, on the Legendre transformation between energy density and pressure, and on nonperturbative asymptotic freedom at high temperatures we derive the coefficient in the high-temperature () -- redshift () relation, , of the Cosmic Microwave Background (CMB). Theoretically, our calculation relies on a deconfining SU(2) rather than a U(1) photon gas. We prove that , representing a topological invariant. Interestingly, the relative deviation of from the critical exponent associated with the correlation length of the 3D Ising model, , is less than . We are not yet in a position to establish a rigorous theoretical link between and…
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