Exact determination of asymptotic CMB temperature-redshift relation
arXiv:1712.08561 · doi:10.1142/S0217732318500293
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 as suggested by the topological nature of and the fact that both theories share a universality class. We do, however, line out a somewhat speculative map from the physical Ising temperature to a fictitious SU(2) Yang-Mills temperature , the latter continuing the asymptotic behavior of the scale factor on for down to , and an exponential map from to to reproduce critical Ising behavior.
v2: 4 pp, 1 fig, discussion added
References in corpus (2)
Cited by in corpus (5)
- SU(2) and the cosmological model: angular power spectra
- An SU(2) gauge principle for the Cosmic Microwave Background: Perspectives on the Dark Sector of the Cosmological Model
- Frequency-redshift relation of the Cosmic Microwave Background
- Cosmological parameters from Planck data in SU(2), their local CDM values, and the modified photon Boltzmann equation
- SU(2) Quantum Yang-Mills Thermodynamics: Some Theory and Some Applications