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Physical review. B, Condensed matter

Magnetic ordering in a normal Fermi liquid at absolute zero

Robert Alan Guyer, Michael David Miller

Published Oct 1, 1978• 4 citations
Publisher

Abstract

We investigate the magnetic-ordering phase transition in a model of a strongly interacting (normal) Fermi liquid at zero temperature. Our system consists of spin-\textonehalf{} fermions which interact with a Lennard-Jones potential. The ground-state thermodynamic properties are obtained by a variational calculation which is carried through in the quantum theorem of corresponding states picture. We show that magnetic ordering represents the balance between the kinetic energy and the repulsive part of the potential energy and that the attractive part of the potential energy tends to inhibit spin ordering.

DOI
10.1103/physrevb.18.3521

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A system of a finite number of harmonically trapped fermions in one dimension, in the presence of a static magnetic field, is studied within the framework of the static fluctuation approximation, for different repulsive and attractive potential strengths. Specifically, the thermodynamic properties of the system (the chemical potential, total energy, heat capacity, and entropy), as well as its magnetic properties (the magnetization and susceptibility), are calculated. It is observed that the system remains in an ordered phase for a small number of particles N, even at high temperatures T. Disorder sets in for large N, even at low T. The effect of the potential strength on the heat capacity is particularly tangible in the region bordering the quantum and classical regimes. The effect of the temperature (representing disorder) is directly opposite to that of the magnetic field (representing order), as expected on basic physical grounds. These features are consistent with experimental results.
The possible superfluidity of a system of strongly interacting fermions is investigated on the assumption that an adequate description of the system in its "normal" state is given by independent fermions in a momentum-dependent potential. On the basis of this assumption we have investigated whether a correlated wave function of the form used by Bardeen, Cooper, and Schrieffer minimizes the ground-state energy. The nonzero terms in the expectation value of the Hamiltonian contain the modified kinetic energy and the full two-body potential between the fermion pairs. An integral equation is obtained in configuration space for the correlation function between pairs. This integral equation is meaningful even for potentials with hard cores, and a nonzero solution implies the existence of a superfluid state. A variational method is devised which provides a criterion for superfluidity and a lower bound for the transition temperature into the superfluid state. We find that a repulsive hard core does not in principle forbid the existence of a superfluid state, but whereas in the absence of a hard core an attractive two-body potential always leads to a superfluid state at sufficiently low temperatures, in the presence of a repulsive core there appears to be a critical strength of attraction needed to form a superfluid state. When the variational principle is applied to liquid He3{\mathrm{He}}^{3}He3 or to nuclear matter, it is found for a wide class of trial functions that the system does not become a superfluid.
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