  Context: Recent satellite measurements in the turbulent magnetosheath of
Earth have given evidence of an unusual reconnection mechanism that is driven
exclusively by electrons. This newly observed process was called electron-only
reconnection, and its inter-play with plasma turbulence is a matter of great
debate.
  Aims: By using 2D-3V hybrid Vlasov-Maxwell simulations of freely decaying
plasma turbulence, we study the role of electron-only reconnection in the
development of plasma turbulence. In particular, we search for possible
differences with respect to the turbulence associated with standard ion-coupled
reconnection.
  Methods: We analyzed the structure functions of the turbulent magnetic field
and ion fluid velocity fluctuations to characterize the structure and the
intermittency properties of the turbulent energy cascade.
  Results: We find that the statistical properties of turbulent fluctuations
associated with electron-only reconnection are consistent with those of
turbulent fluctuations associated with standard ion-coupled reconnection, and
no peculiar signature related to electron-only reconnection is found in the
turbulence statistics. This result suggests that the turbulent energy cascade
in a collisionless magnetized plasma does not depend on the specific mechanism
associated with magnetic reconnection. The properties of the dissipation range
are discussed as well, and we claim that only electrons contribute to the
dissipation of magnetic field energy at sub-ion scales.
