Revision 2

Accepted · core change · record

Changes against revision 1:

Title: Does the QCD axion exist?
Plain: The axion would be a very light, very weakly interacting particle that removes the strong CP puzzle. Detectors search for it turning into a photon inside strong magnets.
Precise · changed · core: Revision 1: Determine whether a pseudoscalar a with $m_a \sim 5.7\ \mathrm{micro-eV}\ (1e12\ \mathrm{GeV}/f_a)$ and photon coupling g_agamma inside the QCD axion band (KSVZ to DFSZ and beyond) exists, for $f_a\ \text{between}\ \sim 1e8\ \text{and}\ \sim 1e17\ \mathrm{GeV}$. An answer is a detection with $m_a$ and g_agamma consistent with the QCD mass-decay constant relation, or exclusion of the band over the full range.; Revision 2: Determine whether a pseudoscalar a with $m_a \sim 5.7\ \mathrm{micro-eV}\ (10^{12}\ \mathrm{GeV}/f_a)$ and photon coupling $g_{agamma}$ inside the QCD axion band (KSVZ to DFSZ and beyond) exists, for $f_a\ \text{between}\ \sim 10^{8}\ \text{and}\ \sim 10^{17}\ \mathrm{GeV}$. An answer is a detection with $m_a$ and $g_{agamma}$ consistent with the QCD mass-decay constant relation, or exclusion of the band over the full range.
Settled by: Haloscope, helioscope (IAXO) and nuclear-coupling (CASPEr-type) searches covering the QCD axion band across micro-eV to meV masses.
Kind: well-posed
Answer type: yes-no
References: (empty)
Literature status: open
Status note: Haloscopes reach DFSZ sensitivity only in narrow windows of a few micro-eV as of 2025.
Posed since: 1978

Decisions