  In this work we study the inversion temperature associated with the
Joule-Thomson expansion from the thermodynamics of AdS-Reissner-N\"ordstrom
black holes. We include quantum corrections in a cosmological fluid that can
describe phantom dark matter or quintessence, both in a Kiselev scenario. The
description of such physical systems involves numerical solutions and the
results are presented as temperature-pressure plots for various values of the
parameters of our model. We find non-zero minimum inversion temperatures as
well as non-zero minimum pressures depending on the values of those parameters.
Completing our study, we also find isenthalpic curves associated with black
hole fixed mass processes.
