The QCD Axion: Some Like It Hot
arXiv:2310.08169 · doi:10.1103/PhysRevD.110.123527
Abstract
We compare the QCD axion phase-space distribution from unitarized next-to-leading order chiral perturbation theory with the one extracted from pion-scattering data. We derive a robust bound by confronting momentum-dependent Boltzmann equations against up-to-date observations of the Cosmic Microwave Background, of the Baryonic Acoustic Oscillations and of primordial abundances. These datasets imply eV for the 95% credible interval, i.e. 30% stronger bound than what previously found. We present forecasts using dedicated likelihoods for future cosmological surveys and the sphaleron rate from unquenched lattice QCD.
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References in corpus (30)
- The Chiral Magnetic Effect
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- An Improved Experimental Limit on the Electric Dipole Moment of the Neutron
- Massive neutrinos and cosmology
- The QCD transition temperature: results with physical masses in the continuum limit
- Measurement of the permanent electric dipole moment of the neutron
- Revisiting the bound on axion-photon coupling from Globular Clusters
- The pion-pion scattering amplitude. IV: Improved analysis with once subtracted Roy-like equations up to 1100 MeV
- The effects of He I 10830 on helium abundance determinations
- Big Bang Nucleosynthesis as a Probe of New Physics
- Cosmological parameters derived from the final (PR4) Planck data release
- Revisiting the axion bounds from the Galactic white dwarf luminosity function
- The Sphaleron Rate in SU(N) Gauge Theory
- Standard big bang nucleosynthesis and primordial CNO Abundances after Planck
- The primordial deuterium abundance of the most metal-poor damped Lyman-alpha system
- Probing Physics Beyond the Standard Model: Limits from BBN and the CMB Independently and Combined
- Thermal axion production in the primordial quark-gluon plasma
- Relic Neutrinos, thermal axions and cosmology in early 2014
- The PHLEK Survey: A New Determination of the Primordial Helium Abundance
- Constraints on Cosmological Parameters from the 500 deg SPTpol Lensing Power Spectrum
- Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest
- An improved cosmological bound on the thermal axion mass
- Thermal QCD Axions across Thresholds
- Cosmological constraints on neutrino plus axion hot dark matter
- A new determination of the primordial helium abundance using the analyses of HII region spectra from SDSS
- Production of Thermal Axions across the ElectroWeak Phase Transition
- The DFSZ axion in the CMB
- Future cosmological sensitivity for hot dark matter axions
- Resolving conclusions about the early Universe requires accurate nuclear measurements
- Revisiting signatures of thermal axions in nonstandard cosmologies
Cited by in corpus (11)
- Massive neutrinos and cosmic composition
- Neutrino masses from large-scale structures: future sensitivity and theory dependence
- Precise predictions for the QCD axion contribution to dark radiation with full phase-space evolution
- Free-Streaming Neutrinos and Their Phase Shift in Current and Future CMB Power Spectra
- Catalogues of Cosmologically Self-Consistent Hadronic QCD Axion Models
- Using to constrain preferred axion model dark matter
- Hunting axion dark matter with anti-ferromagnets: a case study with nickel oxide
- New Bounds on Heavy QCD Axions from Big Bang Nucleosynthesis
- Improved cosmological constraints on axion-lepton interactions
- Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments
- Beyond thermal approximations: Precise cosmological bounds on Axion-Like Particles