  This paper employs an MHD-PIC method to perform numerical simulations of
magnetic reconnection-driven turbulence and turbulent reconnection acceleration
of particles. Focusing on the dynamics of the magnetic reconnection, the
properties of self-driven turbulence, and the behavior of particle
acceleration, we find that: (1) when reaching a statistically steady state of
the self-driven turbulence, the magnetic energy is almost released by 50\%,
while the kinetic energy of the fluid increases by no more than 15\%. (2) the
properties of reconnection-driven turbulence are more complex than the
traditional turbulence driven by an external force. (3) the strong magnetic
field tends to enhance the turbulent reconnection efficiency to accelerate
particles more efficiently, resulting in a hard spectral energy distribution.
Our study provides a particular perspective on understanding turbulence
properties and turbulent reconnection-accelerated particles.
