  A problematic feature of low energy scale inflationary models, such as
Starobinsky inflation, in a spatially closed universe is the occurrence of a
recollapse and a big crunch singularity before inflation can even set in. In a
recent work it was shown that this problem can be successfully resolved in loop
quantum cosmology for a large class of initial conditions due to a non-singular
cyclic evolution and a hysteresis-like phenomena. However, for certain highly
unfavorable initial conditions the onset of inflation was still difficult to
obtain. In this work, we explore the role of dissipative particle production,
which is typical in warm inflation scenario, in the above setting. We find that
entropy production sourced by such dissipative effects makes hysteresis-like
phenomena stronger. As a result, the onset of inflation is quick in general
including for highly unfavorable initial conditions where it fails or is
significantly delayed in the absence of dissipative effects. We
phenomenologically consider three warm inflation scenarios with distinct forms
of dissipation coefficient, and from dynamical solutions and phase space
portraits find that the phase space of favorable initial conditions turns out
to be much larger than in cold inflation.
