We study the optical response of a Mott Hubbard system in the framework of
the half--filled Extended Hubbard Model using the Density Matrix
Renormalization Group (DMRG) method. We discuss the appearance of excitonic
features inside the spectral gap as the system goes from the Spin Density Wave
(SDW) to the Charge Density Wave (CDW) phase.Comment: 4 pages, 4 figure