Solar energetic particles (SEPs) in the energy range 10s KeV/nucleon - 100s
MeV/nucleon originate from the Sun. Their high flux near Earth may damage the
space-borne electronics and generate secondary radiation that is harmful for
life on Earth. Thus, understanding their energization on the Sun is important
for space weather prediction. Impulsive (or $ $He-rich) SEP events are
associated with the acceleration of charge particles in solar flares by
magnetic reconnection and related processes. The preferential acceleration
of heavy ions and the extraordinary abundance enhancement of $ ^3$He in
the impulsive SEP events are not understood yet. In this paper we study the acceleration of heavy ions and its consequences for
their abundance enhancements by magnetic reconnection, an established
acceleration source for
impulsive SEP events in which heavy-ion enhancement is observed We employed a two-dimensional hybrid-kinetic plasma model (kinetic ions and inertial
electron fluid) to simulate magnetic reconnection. All the ion species are
treated self-consistently in our
simulations. We find that heavy ions are preferentially accelerated to energies many
times higher than their initial thermal energies by a variety of
acceleration mechanisms operating in reconnection. The most efficient
acceleration takes place in the flux pileup regions of magnetic
reconnection. Heavy ions with sufficiently low values of charge-to-mass
ratio ($Q/M$) can be accelerated by pickup mechanism in outflow regions
even before any magnetic flux is piled up. The energy spectra of heavy ions
develop a shoulder-like region, a nonthermal feature, as a result of the
acceleration. The spectral index of the power-law fit to the shoulder region
of the spectra varies approximately as $(Q/M)^ $. The abundance
enhancement factor, defined as the number of particles above a threshold energy
normalized to the total number of particles, scales as $(Q/M)^ alpha $, where
alpha increases with the energy threshold. We discuss our simulation
results in the light of the SEP observations.