The flux of an evolving wavepacket is the definite time integral of it
s probability current density. A new method for calculating the flux,
based on a Chebychev polynomial expansion of the quantum evolution ope
rator is presented. The central point of the development is that the t
ime integration of the current density is performed analytically, resu
lting in a scheme which eliminates additional numerical errors. Using
this method, one benefits from both the time-dependent and time-indepe
ndent frameworks of the dynamics. Furthermore, the method requires onl
y a small modification to the existing Chebychev polynomial evolution
code. Examples of performance and accuracy and an application to the c
alculation of recombinative desorption probabilities of N-2 on Re are
shown and discussed.