  Spectroscopic observations of the 2006 outburst of RS Oph at both infrared
(IR) and X-ray wavelengths have shown that the blast wave has decelerated at a
higher rate than predicted by the standard test-particle adiabatic shock-wave
model. The observed blast-wave evolution can be explained, however, by the
diffusive shock acceleration of particles at the forward shock and the
subsequent escape of the highest energy ions from the acceleration region.
Nonlinear particle acceleration can also account for the difference of shock
velocities deduced from the IR and X-ray data. We discuss the evolution of the
nova remnant in the light of efficient particle acceleration at the blast wave.
