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Physical Review

Multiple Scattering and Many-Body Theory: Free Energy of Electrons in Helium

Michael H. Coopersmith

Published Aug 30, 1965• 19 citations
Publisher

Abstract

An electron in helium vapor at 4\ifmmode^\circ\else\textdegree\fi{}K is characterized by its $s$-wave scattering length off helium atoms. This scattering length is small compared with the average interparticle spacing in the helium vapor. Consequently, we have taken as a model a particle interacting via hard-core repulsion with an ideal gas. This establishes a connection with the hard-sphere Bose problem of more general interest. The model described above is simpler (a) because it has only Boltzmann statistics and (b) because the electron is very light compared with the helium atoms. For this model, we have calculated the interaction free energy of the electron assuming that it is in statistical equilibrium with the helium gas. In the $s$-wave approximation, it is shown that this interaction free energy is rigorously $2\ensuremath{\pi}\ensuremath{\rho}a(\frac{{\ensuremath{\hbar}}^{2}}{m})$ due to single scattering, all higher order multiple-scattering effects being zero. Here, $\ensuremath{\rho}$ is the average density of helium atoms, $d$ is the scattering length, and $m$, is the electron mass. Since the $p$-wave approximation contributes a term of order $\ensuremath{\rho}{a}^{3}$, it is evident that the term $2\ensuremath{\pi}\ensuremath{\rho}a(\frac{{\ensuremath{\hbar}}^{2}}{m})$ is good to higher densities than might previously have been supposed. This provides partial justification for the "bubble" model of the electron mobility since the term $2\ensuremath{\pi}\ensuremath{\rho}a(\frac{{\ensuremath{\hbar}}^{2}}{m})$ is certainly good up to densities at which the free energy of the "bubble" configuration becomes smaller.

DOI
10.1103/physrev.139.a1359

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An electron in helium vapor at 4\ifmmode^\circ\else\textdegree\fi{}K is characterized by its sss-wave scattering length off helium atoms. This scattering length is small compared with the average interparticle spacing in the helium vapor. Consequently, we have taken as a model a particle interacting via hard-core repulsion with an ideal gas. This establishes a connection with the hard-sphere Bose problem of more general interest. The model described above is simpler (a) because it has only Boltzmann statistics and (b) because the electron is very light compared with the helium atoms. For this model, we have calculated the interaction free energy of the electron assuming that it is in statistical equilibrium with the helium gas. In the sss-wave approximation, it is shown that this interaction free energy is rigorously 2\ensuremathπ\ensuremathρa(\ensuremathℏ2m)2\ensuremath{\pi}\ensuremath{\rho}a(\frac{{\ensuremath{\hbar}}^{2}}{m})2\ensuremathπ\ensuremathρa(m\ensuremathℏ2​) due to single scattering, all higher order multiple-scattering effects being zero. Here, \ensuremathρ\ensuremath{\rho}\ensuremathρ is the average density of helium atoms, ddd is the scattering length, and mmm, is the electron mass. Since the ppp-wave approximation contributes a term of order \ensuremathρa3\ensuremath{\rho}{a}^{3}\ensuremathρa3, it is evident that the term 2\ensuremathπ\ensuremathρa(\ensuremathℏ2m)2\ensuremath{\pi}\ensuremath{\rho}a(\frac{{\ensuremath{\hbar}}^{2}}{m})2\ensuremathπ\ensuremathρa(m\ensuremathℏ2​) is good to higher densities than might previously have been supposed. This provides partial justification for the "bubble" model of the electron mobility since the term 2\ensuremathπ\ensuremathρa(\ensuremathℏ2m)2\ensuremath{\pi}\ensuremath{\rho}a(\frac{{\ensuremath{\hbar}}^{2}}{m})2\ensuremathπ\ensuremathρa(m\ensuremathℏ2​) is certainly good up to densities at which the free energy of the "bubble" configuration becomes smaller.
A local effective potential, H ex has been used to account for electron exchange, together with a model hamiltonian for the helium atom in Kohn's variational approximation to the electron helium scattering length, a. H ex was chosen to give agreement with the Born-exchange and static-exchange approximations. Correlation was introduced in the 84 term that trial function by using interelectronic coordinates. The method provides an upper bound to the 'model' scattering length and the value of 1.16a 0 was obtained in good agreement with more elaborate calculations and with experiment.
A simplified version of a Bose gas with negative scattering length is studied with a model Hamiltonian similar to that used in the case of repulsive interactions. A new transformation is used which takes into account the attractive interactions in the system, and the ground-state energy is calculated from experimental values of the sound velocity in the system. Real values for the phonon energy spectrum are obtained, and the ratio of the effective mass to ordinary mass is deduced using experimental values of interparticle separation and core radius. A justification for using this modified Hamiltonian is attempted in the Appendix.
The thermodynamics of a free Bose gas with effective temperature scale T~\tilde{T}T~ and hard-sphere Bose gas with the T~\tilde{T}T~ scale are studied. T~\tilde{T}T~ arises as the temperature experienced by a single particle in a quantum gas with 2-body harmonic oscillator interaction VoscV_\textrm{osc}Vosc​, which at low temperatures is expected to simulate, almost correctly, the attractive part of the interatomic potential VHeV_\textrm{He}VHe​ between 4He^{4}\textrm{He}4He atoms. The repulsive part of VHeV_\textrm{He}VHe​ is simulated by a hard-sphere (HS) potential. The thermodynamics of this system of HS bosons, with the T~\tilde{T}T~ temperature scale (HSET), is investigated, first, by the Bogoliubov-Huang method and next by a modified version of this method, which takes approximate account of those terms of the 2-body repulsion which are linear in the zero-momentum Bose operators a0,  a0∗a_0,\,\,a^*_0a0​,a0∗​ (originally rejected by Bogoliubov). Theoretical heat capacity CV(T)C_V(T)CV​(T) exhibits good agreement, below 2.1 K, with the experimental heat capacity graph observed in 4He^{4}\textrm{He}4He at saturated vapour pressure. The phase transition to the low-temperature phase, with a Bose-Einstein condensate, occurs in the HSET at $T_λ=$2.17 K, and is accompanied, in the modified HSET version, by a singularity of CV(T)C_V(T)CV​(T). Other thermal properties of HSET, such as the momentum distribution function, the fraction of atoms in the momentum condensate and normal fluid density, agree qualitatively with those of 4He^{4}\textrm{He}4He, but improve those of the free Bose gas.
The thermodynamics of a free Bose gas with effective temperature scale [Formula: see text] and hard-sphere Bose gas with the [Formula: see text] scale are studied. [Formula: see text] arises as the temperature experienced by a single particle in a quantum gas with 2-body harmonic oscillator interaction V osc , which at low temperatures is expected to simulate, almost correctly, the attractive part of the interatomic potential V He between 4 He atoms. The repulsive part of V He is simulated by a hard-sphere (HS) potential. The thermodynamics of this system of HS bosons, with the [Formula: see text] temperature scale (HSET), and particle mass and density equal to those of 4 He , is investigated, first, by the Bogoliubov–Huang method and next by an improved version of this method, which describes He II in terms of dressed bosons and takes approximate account of those terms of the 2-body repulsion which are linear in the zero-momentum Bose operators a0, [Formula: see text] (originally rejected by Bogoliubov). Theoretical heat capacity CV(T) exhibits good agreement, below 1.9 K, with the experimental heat capacity graph observed in 4 He at saturated vapour pressure. The phase transition to the He II phase, occurs in the HSET at Tλ = 2.17 K, and is accompanied, in the modified HSET version, by a singularity of CV(T). The fraction of atoms in the momentum condensate at 0 K equals 8.86% and agrees with other theoretical estimates for He II. The fraction of normal fluid falls to 8.37% at 0 K which exceeds the value 0% found in He II.
In this work we investigate the structure and dynamics of small clusters of Helium atoms. We consider bound states of clusters having A = 2, 3, 4, 5, 6 atoms and continuum states in the three-atom system. Motivated by the fact that the He-He system has a very large scattering length a compared to the range r 0 of the He-He potential (r 0/a < 1/10), we propose the use of a soft-core interparticle potential. We use an attractive gaussian potential that reproduces the values of the dimer binding energy and the atomatom scattering length obtained with one of the widely used He-He interactions, the LM2M2 potential. In addition, we include a repulsive three-body force to reproduce the trimer binding energy. With this model, consisting in the sum of a two- and a three-body potential, we show the spectrum of the four, five, and sixparticle systems and phase-shifts and inelasticities in the three-atom system. Comparisons to calculations using realistic He-He potentials are given. In addition some universal relations are explored.
It is shown that the effective interaction strength of three bosons at small collision energies can be extracted from their wave function at zero energy. Asymptotic expansions of this wave function at large interparticle distances are derived, from which is defined a quantity DDD named three-body scattering hypervolume, which is an analog of the two-body scattering length. Given any finite-range interactions, one can thus predict the effective three-body force from a numerical solution of the Schr\"odinger equation. In this way, the constant DDD for hard-sphere bosons is computed, leading to the first complete result for the ground-state energy per particle of a dilute Bose-Einstein condensate (BEC) of hard spheres to order ${\ensuremath{\rho}}^{2}$, where $\ensuremath{\rho}$ is the number density. Effects of DDD are also demonstrated in the three-body energy in a finite box of size LLL, which is expanded to the order ${L}^{\ensuremath{-}7}$, and in the three-body scattering amplitude in vacuum. The three-body scattering amplitude calculated in this paper disagrees with an earlier calculation in the literature, because of the omission of the two-body effective range in that earlier work. Another key prediction is the condensate fractions of dilute BECs, which also disagree with an earlier work in the literature based on the effective field theory (EFT), as a result of short-range physics. An EFT prediction of the BEC ground-state energy, however, is corroborated.