New Bounds on Heavy QCD Axions from Big Bang Nucleosynthesis

TL;DR

This paper derives new constraints on heavy QCD axions using Big Bang Nucleosynthesis data, showing that certain axion lifetimes are excluded based on their impact on primordial element abundances, surpassing future CMB bounds.

Contribution

It provides the first comprehensive BBN-based bounds on heavy QCD axions, including detailed modeling of hadronic decay effects and improved treatment of hadronic scattering processes.

Findings

Axion lifetimes below 0.017 seconds are excluded for masses above 300 MeV.

BBN constraints are more stringent than future CMB $N_{eff}$ bounds.

Bounds are robust against uncertainties in hadronic processes and initial axion abundance.

Abstract

We study Big Bang Nucleosynthesis (BBN) constraints on heavy QCD axions. BBN offers a powerful probe of new physics that modifies the neutron-to-proton ratio during the process, thanks to the precisely measured primordial Helium-4 abundance. A heavy QCD axion provides an attractive target for this probe, because not only is it a well-motivated hypothetical particle by the strong CP problem, but also it dominantly decays to hadrons if kinematically allowed. A range of its lifetime is thus excluded where the hadronic decays would significantly alter the neutron-to-proton ratio. We compute axion-induced modification of the neutron-to-proton ratio, and obtain robust upper bounds on the axion lifetimes, as low as 0.017 s for the axion mass higher than 300 MeV. Remarkably, this is stronger than projected future CMB bounds via $N_{\rm eff}$. Our bounds are largely insensitive to uncertainties in hadronic cross sections and the axion's branching fractions into various hadrons, as well as to the precise value of the initial axion abundance. We also incorporate, for the first time, several key improvements, such as scattering processes by energetic $K_L$ and secondary hadrons, that can also be important for studying general hadronic injections during BBN, not limited to those from axion decays.