The temperature dependence of the high-frequency optical conductivity of th
e half-filled Hubbard model is calculated in the strong coupling limit, usi
ng the non-crossing approximation. For large dimensionality, d, the electro
nic spectral density is of the order of the coulomb interaction U in the st
rong coupling limit, as expected from the arguments of Mott and Hubbard. Th
e Value of the gap is renormalized by spin fluctuations and is strongly aff
ected by the dimensionality, in accordance with the Mermin-Wagner theorem.
The spin fluctuation energies are governed by Anderson's kinetic exchange,
J = t(2)/U, as is the temperature dependence of the gap. The width of the i
ncoherent peaks is due to spin-wave shake off processes and is of the order
of U. The intensity of the coherent quasi-particle peaks in the spectral d
ensity is renormalized down to small values. The optical conductivity is ca
lculated for various dimensionalities and the results are compared with the
exact solutions found in the limits of d --> infinity and d = 1. (C) 2000
Elsevier Science B.V. All rights reserved.