In this work, the Thermodynamic Geometry (TG) of quantum fluids (QF) is
analyzed. We present results for two models. The first one is a quantum
hard-sphere fluid (QHS) whose Helmholtz free energy is obtained from Path
Integrals Monte Carlo simulations (PIMC). It is found that due to quantum
contributions in the thermodynamic potential, the anomaly found in TG for the
classical hard-sphere fluid related to the sign of the scalar curvature, is now
avoided in a considerable region of the thermodynamic space. The second model
is a semi-classical square-well fluid (QSW), described by a quantum hard-sphere
repulsive interaction coupled with a classical attractive square-well
contribution. Behavior of the semi-classical curvature scalar as a function of
the thermal de Broglie wavelength λB is analyzed for several
attractive-potential ranges, and description of the semi-classical R-Widom
lines defined by the maxima of the curvature scalar, are also obtained and
compared with classical results for different square-well ranges.Comment: 9 pages, 8 figure