2006/07/24 by R. D. Peccei · 1 voice · 12 citations
#hep-ph
paper · pdf · doi:10.1007/978-3-540-73518-2_1
I describe how the QCD vacuum structure, necessary to resolve the U(1)A problem, predicts the presence of a P, T and CP violating term proportional to the vacuum angle θ. To agree with experimental bounds, however, this parameter must be very small (θ ≤ 10-9). After briefly discussing some possible other solutions to this, so-called, strong CP problem, I concentrate on the chiral solution proposed by Peccei and Quinn which has associated with it a light pseudoscalar particle, the axion. I discuss in detail the properties and dynamics of axions, focusing particularly on invisible axion models where axions are very light, very weakly coupled and very long-lived. Astrophysical and cosmological bounds on invisible axions are also briefly touched upon.