QCD -vacuum energy and axion properties
arXiv:2003.01625 · doi:10.1007/JHEP05(2020)001
Abstract
At low energies, the strong interaction is governed by the Goldstone bosons associated with the spontaneous chiral symmetry breaking, which can be systematically described by chiral perturbation theory. In this paper, we apply this theory to study the -vacuum energy density and hence the QCD axion potential up to next-to-leading order with non-degenerate quark masses. By setting , we then derive the axion mass, self-coupling, topological susceptibility and the normalized fourth cumulant both analytically and numerically, taking the strong isospin breaking effects into account. In addition, the model-independent part of the axion-photon coupling, which is important for axion search experiments, is also extracted from the chiral Lagrangian supplemented with the anomalous terms up to .
22 pages, 1 figure, 2 tables; Version to appear in JHEP
References in corpus (12)
- Discovering the QCD Axion with Black Holes and Gravitational Waves
- Improved limit on the permanent electric dipole moment of 199Hg
- Bose-Einstein Condensation of Dark Matter Axions
- First results from a microwave cavity axion search at 24 micro-eV
- Dilute and dense axion stars
- Mesonic low-energy constants
- Relativistic axions from collapsing Bose stars
- Limits on Axion Couplings from the first 80-day data of PandaX-II Experiment
- Axion cold dark matter in view of BICEP2 results
- Portal Connecting Dark Photons and Axions
- Axions from cooling compact stars: pair-breaking processes
- Hydrogen Axion Star: Metallic Hydrogen Bound to a QCD Axion BEC