Direct numerical simulations (DNS) are conducted to study the turbulence-ch
emical reaction interactions in homogeneous decaying compressible fluid flo
ws. The reaction is of a single-step irreversible Arrhenius type. The resul
ts indicate that the heat of reaction has a noticeable influence on the sol
enoidal and the dilatational turbulent motions. The effect of reaction on t
he solenoidal velocity field is primarily due to variation of the molecular
diffusivity coefficients with temperature and appears at small scales. How
ever, the dilatational motions are affected more than the solenoidal motion
s and are intensified at all length scales. The decay rate of the turbulent
kinetic energy is dependent on the molecular dissipation and the pressure-
dilation correlation. In isothermal reacting cases, the net contribution of
the pressure-dilatation is small and the turbulent energy decays continuou
sly due to viscous dissipation. In the exothermic reacting cases, the press
ure-dilatation tends to increase the turbulent kinetic energy when the reac
tion is significant. Analysis of the flow structure indicates that the flow
is dominated by strain in the reaction zones. Also, consistent with previo
us studies, the scalar gradient tends to align with the most compressive st
rain eigenvector and the vorticity vector tends to align with the intermedi
ate strain eigenvector. The heat of reaction weakens this preferential alig
nment, primarily due to variation in molecular transport coefficients. The
spatial and the compositional structure of the flame are also affected by t
he modification of the turbulence and the molecular coefficients. (C) 2000
American Institute of Physics. [S1070-6631(00)00205-1].