Kirkwood Phase Transition for Boson and Fermion Hard-Sphere Systems

dc.creatorSolis, M. A.
dc.creatorde Llano, M.
dc.creatorClark, J. W.
dc.date2003-06-12
dc.date.accessioned2026-07-07T02:51:48Z
dc.date.available2026-07-07T02:51:48Z
dc.descriptionThe London ground-state energy formula as a function of number density $ρ$ for a system of boson hard spheres of diameter $c$ at zero temperature (corrected for the reduced mass of a pair of particles in a ``sphere-of-influence'' picture) generalized to describe fermion hard-sphere systems with four and two intrinsic degrees of freedom such as helium-three or neutron matter and symmetric nuclear matter, respectively, is proposed as the crystalline energy branch for hard-sphere systems. For the fluid branch we use the well-known, exact, low-density equation-of-state expansions for many-boson and many-fermion systems, appropriately extrapolated to physical densities. Here, via a double-tangent construction the crystallization and melting densities for boson and fermion hard spheres are determined. They agree well with variational Monte Carlo, density-functional, and Green Function Monte Carlo calculations.
dc.description13 pages including 4 figures
dc.identifierhttps://arxiv.org/abs/cond-mat/0306338
dc.identifierhttp://arxiv.org/abs/cond-mat/0306338
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/21605
dc.subjectStatistical Mechanics
dc.subjectSoft Condensed Matter
dc.titleKirkwood Phase Transition for Boson and Fermion Hard-Sphere Systems
dc.typetext

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