Reheating in holographic cosmology and connecting to $\Lambda$-MSSM
  constructions for particle physics
  In this paper we model the transition from the non-geometric holographic
cosmology regime, to the usual radiation dominated (RD) cosmology, known as
reheating in the case of (perturbative) inflation. We find that we can easily
transition into any MSSM construction of intersecting D6-branes, via $\alpha'$
corrections in the 3 dimensional field theory as well as in cosmology, followed
by cosmological reheating via S-NS5-branes. Moreover, we can naturally obtain
the (true) cosmological constant $\Lambda$ of the observed order of magnitude.
The resulting supersymmetry breaking is just outside the currently observed
energies. The model is consistent with large (TeV scale) extra dimensions, but
it prefers smaller ones, and the string scale is generically low.
