  Deep X-ray surveys by Chandra and XMM-Newton have resolved about 80% of the
2-10 keV cosmic extragalactic X-ray background (CXRB) into point sources, the
majority of which are obscured AGN. The obscuration might be connected to
processes within the host galaxy, possibly the star-formation rate. Here, we
use the results of CXRB synthesis calculations as input to detailed Cloudy
simulations in order to predict the evolution of AGN properties at several
mid-IR wavelengths. Computations were performed for three different evolutions
of the AGN type 2/type 1 ratio between z=0 and 1: where the ratio increased as
(1+z)^{0.9}, as (1+z)^{0.3} and one with no redshift evolution. Models were
calculated with the inner radius of the absorbing gas and dust at 1 pc or at 10
pc. Comparing the results of the calculations to combined X-ray and Spitzer
data of AGN shows that the predicted spectral energy distributions are a good
description of average AGNs found in the deep surveys. The existing data
indicates that the mid-IR emission from an average AGN is best described by
models where the attenuating material is ~10 pc from the central engine. We
present the expected Spitzer cumulative number count distributions and the
evolution of the total AGN (type 1 + type 2) luminosity function (LF) between
z=0 and 1 at rest-frame 8 microns and 30 microns for the three evolutionary
scenarios. The mid-IR AGN LF will be an excellent tool to measure the evolution
of the covering factor of the gas and dust from z~0 to 1.
