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Physical Review A

Correlation of two weakly attractive particles on a sphere

Robert J. Hinde, R. Stephen Berry

Published Aug 1, 1990• 14 citations
Publisher

Abstract

We simulate the behavior of two weakly attractive atoms, either spin-polarized hydrogen atoms or $^{3}\mathrm{He}$ atoms, on a $^{4}\mathrm{He}$ cluster by examining the angular correlation of the atoms as they move on the surface of a sphere. We have calculated converged energy levels, wave functions, and reduced densities ${\mathrm{\ensuremath{\rho}}}^{(\mathit{J})}$(${\mathrm{\ensuremath{\theta}}}_{12}$) for the low-lying states of these two systems. We also give the oscillator strengths for several transitions between low-lying states for the case of spin-polarized hydrogen. The energy levels can be arranged in patterns reminiscent of the rovibrational levels of a linear triatomic molecule, but the reduced densities differ significantly from those predicted by the molecular model. The lowest state for two $^{3}\mathrm{He}$ atoms on a sphere of radius 13.0 bohr is bound, with E=-0.031 90 ${\mathrm{cm}}^{\mathrm{\ensuremath{-}}1}$.

DOI
10.1103/physreva.42.2259

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We simulate the behavior of two weakly attractive atoms, either spin-polarized hydrogen atoms or 3He^{3}\mathrm{He}3He atoms, on a 4He^{4}\mathrm{He}4He cluster by examining the angular correlation of the atoms as they move on the surface of a sphere. We have calculated converged energy levels, wave functions, and reduced densities \ensuremathρ(J){\mathrm{\ensuremath{\rho}}}^{(\mathit{J})}\ensuremathρ(J)(\ensuremathθ12{\mathrm{\ensuremath{\theta}}}_{12}\ensuremathθ12​) for the low-lying states of these two systems. We also give the oscillator strengths for several transitions between low-lying states for the case of spin-polarized hydrogen. The energy levels can be arranged in patterns reminiscent of the rovibrational levels of a linear triatomic molecule, but the reduced densities differ significantly from those predicted by the molecular model. The lowest state for two 3He^{3}\mathrm{He}3He atoms on a sphere of radius 13.0 bohr is bound, with E=-0.031 90 cm\ensuremath−1{\mathrm{cm}}^{\mathrm{\ensuremath{-}}1}cm\ensuremath−1.
Ground and excited-rovibrational states of weakly bound triatomic molecules containing two helium and one silver atoms are investigated. We consider three systems, $^{4}\mathrm{He}\text{\ensuremath{-}}^{4}\mathrm{He}\text{\ensuremath{-}}\mathrm{Ag}$, $^{3}\mathrm{He}\text{\ensuremath{-}}^{4}\mathrm{He}\text{\ensuremath{-}}\mathrm{Ag}$, and $^{3}\mathrm{He}\text{\ensuremath{-}}^{3}\mathrm{He}\text{\ensuremath{-}}\mathrm{Ag}$. The three-atom Schr\"odinger equation is solved in hyperspherical coordinates using the potential-energy surface represented as the addition of He-He and He-Ag pair interaction potentials. We compute the energy levels and analyze the structural properties by considering averaged pair distances and bond angles, one-dimensional pair and angle distribution functions, and two-dimensional pair-pair and angle-angle distribution functions. All the He-He-Ag bound states are found to possess similar characteristics, displaying obtuse isosceles (4He2Ag^{4}\mathrm{He}_{2}\mathrm{Ag}4He2​Ag and 3He2Ag^{3}\mathrm{He}_{2}\mathrm{Ag}3He2​Ag) or scalene (3He4HeAg^{3}\mathrm{He}^{4}\mathrm{He}\mathrm{Ag}3He4HeAg) triangle configurations where the He-Ag distances are nearly fixed and the Ag bond angle is variable.
We study a system of two electrons interacting with a Coulomb potential in a sphere of radius R, bounded by an infinite wall using exact diagonalization. We have also investigated the influence of an additional parabolic potential (of strength k)k)k) arising from a uniform background smeared throughout the sphere. The convergence of the ground state energy of the singlet spin state of the system is investigated as a function of sphere size (essentially rs,{r}_{s},rs​, the Wigner--Seitz density parameter) for cases where there is no background potential (k=0)(k=0)(k=0) and for when $k\ensuremath{\ne}0.$ With k=0k=0k=0 and small rs,{r}_{s},rs​, we observe a maximum in the ground state density at the origin of the sphere. At ${r}_{s}\ensuremath{\approx}8\mathrm{a}.\mathrm{u}.,$ the ground state density acquires a minimum at the origin. For this and larger systems we identify the formation of a ``Wigner'' molecule state. We further investigate the ground state density as a function of k and also the correlation hole density as a function of rs{r}_{s}rs​ and k. We invert the Kohn--Sham equation for a two electron system and calculate the local effective potential and correlation potential (to within an additive constant) as functions of the radial coordinate for a number of values of rs{r}_{s}rs​ and k.
The ground-state of the helium and spin-polarized hydrogen quantum clusters is investigated in this work using Quantum Monte Carlo methods, as well as the spin-polarized tritium (T↓) liquid. For small mixed helium clusters consisting of up to eight helium atoms the ground-state energy and structure have been obtained. Stability of the 3He4 4He3 cluster, which was previously considered unstable, is predicted. It is confirmed that tritium trimer (T↓)3 is an example of Borromean state. For pure large spin-polarized tritium clusters consisting of up to 320 atoms the ground-state energy is obtained. Stability limits have been investigated for small mixed (T↓)n(D↓)m clusters, for m ≥ 2 i n + m ≤ 10. Especially, it has been shown that all clusters (T↓)ND↓ are stable for N ≥ 3. It is also shown that even 60 T↓ atoms are not enough to form stable cluster (T↓)60H↓. Equation of state, spinodal density, energy per particle at the equilibrium density, unit radius and surface tension of the T↓ liquid have been determined using results obtained in the simulations of liquid phase.
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We study low-lying excited states of 4He{}^{4}\mathrm{He}4He clusters up to a cluster size of 40 atoms in a variational framework. The ansatz wave function combines two- and three-body correlations, coming from a translationally invariant configuration interaction description, and Jastrow-type short-range correlation. We have previously used this scheme to determine the ground-state energies of 4He{}^{4}\mathrm{He}4He and 3He{}^{3}\mathrm{He}3He clusters. Here we present an extension of this ansatz wave function having a good quantum angular momentum L. The variational procedure is applied independently to the cases with L=0,2,4,L=0,2,4,L=0,2,4, and upper bounds for the corresponding energies are thus obtained. Moreover, centroid energies for L excitations are calculated through the use of sum rules. A comparison with previous calculations is also made.
The model of two particles on a sphere is extended to two particles on concentric spheres (POCS). The quantum states are found for two electrons, one on a sphere of radius 10 a.u. (simulating the shell n=3n=3n=3 in He) and the other, on spheres of 10, 15, 25, 50, and 100 a.u. The eigenvalues and densities $\ensuremath{\rho}({\ensuremath{\theta}}_{12})$ exhibit a transition from collective, moleculelike behavior to independent-particle-like behavior with Russell-Saunders coupling. The parallel problem of two particles with electron masses interacting via a repulsive Gaussian potential is also treated and a similar transition from collective to independent-particle behavior found. The principal difference between the two cases is only the region of radius of the larger sphere where the transition occurs.