Figure 4: Time-dependent autocorrelation function of the unit C–N vectors.
From: Ionic polarization-induced current–voltage hysteresis in CH3NH3PbX3 perovskite solar cells

The autocorrelation function has been computed averaging over the microcanonical ensemble sampled by constant number of particles, volume and energy (NVE) first-principles MD simulations performed at four different energies corresponding to average temperatures of 100, 200, 300 and 400 K. In the inset log τ1 vs is shown, together with the linear fitting from which the rotational reorientation activation energy is obtained.