Speaker
Mr
Peter Graf
(Max-Planck-Institut fuer Physik)
Description
We calculate the rate for thermal production of axions and saxions via scattering of quarks, gluons, squarks, and gluinos in the primordial supersymmetric plasma. Systematic field theoretical methods such as hard thermal loop resummation are applied to obtain a finite result in a gauge-invariant way that is consistent to leading order in the strong gauge coupling. We calculate the thermally produced yield and the decoupling temperature for both axions and saxions. For the generic case in which saxion decays into axions are possible, the emitted axions can constitute extra radiation already prior to big bang nucleosynthesis and well thereafter.We update associated limits imposed by recent studies of the primordial helium-4 abundance
and by precision cosmology of the cosmic microwave background and large scale structure. We show that the trend towards extra radiation seen in those studies can be explained by late decays of thermal saxions into axions and that upcoming Planck results will probe supersymmetric axion models with unprecedented sensitivity.
Primary authors
Dr
Frank Steffen
(Max-Planck-Institut fuer Physik)
Mr
Peter Graf
(Max-Planck-Institut fuer Physik)
