A. N. Cox recently showed that a 20% opacity decrease in the 20,000-30
.000 K region as indicated by the new Livermore OPAL opacities reconci
les the discrepancy between pulsation and evolution masses of double-m
ode RR Lyrae variables. Nonlinear hydrodynamic calculations were perfo
rmed for RR Lyrae models of mass 0.75 M., 51 L.. and Z = 0.0001 (Oster
hoff II type) including this opacity decrease. The Stellingwerf period
ic relation method was used to converge the models to a limit cycle, a
nd the Floquet matrix eigenvalues calculated to search for a tendency
of the fundamental mode to grow from the full-amplitude overtone solut
ion, and the overtone mode to grow from the full-amplitude fundamental
solution, thereby predicting double-mode behavior. Models of T(eff) <
7000 K with the opacity decrease have positive fundamental-mode growt
h rates in the overtone solution, in contrast to earlier results by Ho
dson and Cox (1982), and models with T(eff) > 7000 have positive 1st o
vertone growth rates in the fundamental-mode solution, but double-mode
behavior was not found.