부산대학교 도서관

We derive a robust bound on the QCD axion by confronting momentum-dependent Boltzmann equations against up-to-date measurements of the Cosmic Microwave Background, including ground-based telescopes, and abundances from Big Bang Nucleosynthesis. We compare the axion phase-space distribution obtained from unitarized next-to-leading order chiral perturbation theory with the phenomenological one based on pion-scattering data. Our bound is $\sim$30\% stronger than what previously found: $m_{a} \leq \, 0.16 $ eV at 95\% probability. We present forecasts using dedicated likelihoods for future cosmological surveys and the sphaleron rate from unquenched lattice QCD.
Comment: 12 pages with appendix and references, 3+1 figures