  Affleck-Dine leptogenesis after thermal inflation along the $LH_u$ direction
requires $m_L^2+m_{H_u}^2 < 0$ up to the AD scale ($|L|\simeq |H_u|\sim 10^9$
GeV). We renormalised this condition from the AD scale to the soft
supersymmetry breaking scale by solving the renormalisation group equations
perturbatively in the Yukawa couplings to obtain a semi-analytic constraint on
the soft supersymmetry breaking parameters. We also used a fully numerical
method to renormalise the baryogenesis condition and constrained the Minimal
Supersymmetric Cosmological Model using the resulting baryogenesis condition
and other constraints, specifically, electroweak symmetry breaking, the
observed Higgs mass, and the axino dark matter abundance.
