The Cosmological Axino Problem
Abstract
We revisit the cosmology of the supersymmetric QCD axion, highlighting the existence of a serious cosmological axino problem that is fully analogous to the gravitino problem of overclosure via thermal production. A general analysis implies that the QCD axino has a mass greater than or equal to that of the gravitino in the absence of unnatural fine-tuning or sequestering. As a consequence, bounds from thermal gravitino and QCD axino production are complementary in parameter space, and together provide a quite stringent limit on the reheating temperature after inflation given by TR < 103 - 106 GeV for an axion decay constant of fa = 109 - 1012 GeV. Motivated by this result, we explore the cosmology of gravitino LSP and axino NLSP at low TR and present three realistic scenarios for dark matter.