Axial Anomaly in Galaxies and the Dark Universe
Janning Meinert, Ralf Hofmann

TL;DR
This paper proposes a model where ultralight axion dark matter, arising from SU(2) Yang-Mills theories, explains galactic structures and links dark matter, dark energy, and leptons through the axial anomaly.
Contribution
It introduces a novel SU(2)$_{ m CMB}$-based framework for dark matter and dark energy, connecting particle physics with cosmological observations.
Findings
Lightest axion mass estimated at 0.675×10⁻²³ eV from galaxy rotation curves.
Virial mass of dark matter lumps predicts properties of galactic centers and globular clusters.
SU(2)$_{ m CMB}$ remains thermalized, linking axion condensate to dark energy.
Abstract
Motivated by the SU(2) modification of the cosmological model CDM, we consider isolated fuzzy-dark-matter lumps, made of ultralight axion particles whose masses arise due to distinct SU(2) Yang-Mills scales and the Planck mass . In contrast to SU(2), these Yang-Mills theories are in confining phases (zero temperature) throughout most of the Universe's history and associate with the three lepton flavours of the Standard Model of particle physics. As the Universe expands, axionic fuzzy dark matter comprises a three-component fluid which undergoes certain depercolation transitions when dark energy (a global axion condensate) is converted into dark matter. We extract the lightest axion mass eV from well motivated model fits to observed rotation curves in low-surface-brightness galaxies (SPARC catalogue). Since the virial…
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