Cosmological parameters from Planck data in SU(2)${}_{\mathrm{CMB}}$, their local $\Lambda$CDM values, and the modified photon Boltzmann equation

Abstract

A review of the spatially flat cosmological model SU(2)${}_{\mathrm{CMB}}$, minimally induced by the postulate that the Cosmic Microwave Background (CMB) is subject to an SU(2) rather than a U(1) gauge principle, is given. Cosmological parameter values, which are determined from the Planck CMB power spectra at small angular scales, are compared to their values in spatially flat $\Lambda$CDM from both local and global extractions. As a global model SU(2)${}_{\mathrm{CMB}}$ leans towards local $\Lambda$CDM cosmology and is in tension with some global $\Lambda$CDM parameter values. We present spectral antiscreening / screening effects in SU(2)${}_{\mathrm{CMB}}$ radiance within the Rayleigh-Jeans regime in dependence on temperature and frequency. Such radiance anomalies can cause CMB large-angle anomalies. Therefore, it is pointed out how SU(2)${}_{\mathrm{CMB}}$ modifies the Boltzmann equation for the perturbations of the photon phase space distribution at low redshift and why this requires to the solve the $\ell$-hierarchy on a comoving momentum grid ($q$-grid) for all $z$.

arXiv comment9 pages, 7 figures

References in corpus (65)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• Planck 2015 results. XIII. Cosmological parameters
• Efficient Computation of CMB anisotropies in closed FRW models
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• A Line of Sight Approach to Cosmic Microwave Background Anisotropies
• Cosmological Perturbation Theory in the Synchronous vs. Conformal Newtonian Gauge
• Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
• Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
• Evidence for Reionization at z ~ 6: Detection of a Gunn-Peterson Trough in a z=6.28 Quasar
• KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
• Asymmetries in the CMB anisotropy field
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• A high resolution foreground cleaned CMB map from WMAP
• The significance of the largest scale CMB fluctuations in WMAP
• The Baryon Census in a Multiphase Intergalactic Medium: 30% of the Baryons May Still Be Missing
• Detection of non-Gaussianity in the WMAP 1-year data using spherical wavelets
• Planck 2018 results. VII. Isotropy and Statistics of the CMB
• Late time Cosmological Phase Transition and Galactic Halo as Bose-liquid
• The cosmological baryon density from the deuterium to hydrogen ratio towards QSO absorption systems: D/H towards Q1243+3047
• The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics
• CMB Anomalies after Planck
• ARCADE 2 Measurement of the Extra-Galactic Sky Temperature at 3-90 GHz
• On the large-angle anomalies of the microwave sky
• The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3
• Spontaneous Isotropy Breaking: A Mechanism for CMB Multipole Alignments
• Scalar Fields as Dark Matter in Spiral Galaxies
• Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions
• The evolution of the Cosmic Microwave Background Temperature: Measurements of TCMB at high redshift from carbon monoxide excitation
• 2-Point Correlations in the COBE DMR 4-Year Anisotropy Maps
• Late-time Phase transition and the Galactic halo as a Bose Liquid: (II) the Effect of Visible Matter
• Small-scale structure of fuzzy and axion-like dark matter
• The microwave background temperature at the redshift of 2.33771
• A precise and accurate determination of the cosmic microwave background temperature at z=0.89
• Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipoles
• Lack of large-angle TT correlations persists in WMAP and Planck
• Large-scale alignments from WMAP and Planck
• A New Measurements of the Cosmic Microwave Background Radiation Temperature at z = 1.97
• Discovery of a Perseus-like cloud in the early Universe: HI-to-H2 transition, carbon monoxide and small dust grains at zabs=2.53 towards the quasar J0000+0048
• Measurement of the $T_{\mathrm{CMB}}$ evolution from the Sunyaev-Zel'dovich effect
• The cosmic microwave background radiation temperature at z = 3.025 toward QSO 0347--3819
• Microwave Background Temperature at a Redshift of 6.34 from H2O Absorption
• Explaining Cosmological Anisotropy: Evidence for Causal Horizons from CMB data
• A comprehensive overview of the Cold Spot
• Parity Asymmetry in the CMBR Temperature Power Spectrum
• Directional Variations of Cosmological Parameters from the Planck CMB Data
• The Physical Origins of the Identified and Still Missing Components of the Warm-Hot Intergalactic Medium: Insights from Deep Surveys in the Field of Blazar 1ES1553+113
• On the proper kinetic quadrupole CMB removal and the quadrupole anomalies
• Radiative corrections to the pressure and the one-loop polarization tensor of massless modes in SU(2) Yang-Mills thermodynamics
• Bias in low-multipole CMB reconstructions
• A model for the very early Universe
• A model for CMB anisotropies on large angular scales
• Axial Anomaly in Galaxies and the Dark Universe
• Relic photon temperature versus redshift and the cosmic neutrino background
• SU(2) Yang-Mills Theory: Waves, Particles, and Quantum Thermodynamics
• Gap in the black-body spectrum at low temperature
• SU(2)${}_{\mathrm{CMB}}$ and the cosmological model: angular power spectra
• Exact determination of asymptotic CMB temperature-redshift relation
• SU(2)$_{\tiny\mbox{CMB}}$ at high redshifts and the value of $H_0$
• Modification of black-body radiance at low temperatures and frequencies
• The isolated, uniformly moving electron: Selfintersecting SU(2) Yang-Mills center vortex loop and Louis de Broglie's hidden thermodynamics

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