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We investigate the dependence of the chiral condensate $<\bar qq>$ on thetemperature and quark density using the soft-wall holographic model of QCD,adopting geometries with black holes at finite temperature and quark chemicalpotential $\mu$. We find that, for $\mu$ below a critical value, increasing thetemperature the condensate decreases and vanishes at a temperature $\tildeT\simeq 210$ MeV (at $\mu=0$). An analogous behaviour is observed increasingthe chemical potential at fixed temperature. These results agree with thefindings obtained by other methods. We also comment on the robustness of theresults if geometries not involving black holes are adopted at low temperature,and an Hawking-Page transition is implemented.

Temperature and quark density effects on the chiral condensate: an AdS/QCD study