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Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields

Energy trajectories for the N -boson problem by the method of potential envelopes

Richard L. Hall

Published Oct 15, 1980• 49 citations
Publisher

Abstract

This paper concerns the ground-state energy ${E}_{N}$ of a system of $N$ identical bosons interacting via the attractive central pair potential $V({r}_{\mathrm{ij}})=\ensuremath{-}{V}_{0}f(\frac{{r}_{\mathrm{ij}}}{a})$ and obeying nonrelativistic quantum mechanics. It is assumed that the potential shape $f$ is decreasing and can be represented as the envelope of each of two complementary families of power-law potentials $\ensuremath{\alpha}+\ensuremath{\beta}{r}^{p}$ (one family is above $f$ and the other below) for suitable fixed $p={p}_{1}$ and $p={p}_{2}$. If $\ensuremath{\epsilon}=\ensuremath{-}\frac{m{a}^{2}{E}_{N}}{(N\ensuremath{-}1){\ensuremath{\hbar}}^{2}}$ and $v=\frac{\mathrm{Nm}{V}_{0}{a}^{2}}{2{\ensuremath{\hbar}}^{2}}$, then it is proved that the entire collection of nonintersecting energy trajectories $\ensuremath{\epsilon}={F}_{N}(v)$, $N=2, 3, 4, \dots{}$, is bounded between the fixed curves $(v, \ensuremath{\epsilon})=(\ensuremath{-}\ensuremath{\gamma}(p){[{s}^{3}{f}^{\ensuremath{'}}(s)]}^{\ensuremath{-}1}, (\frac{v}{2})[2f(s)+s{f}^{\ensuremath{'}}(s)])$, where the curve parameter $s>0$, and $p={p}_{1}, {p}_{2}$. Potentials, for example, with shapes $f(r)=\frac{{\ensuremath{\alpha}}_{1}}{r}+\frac{{\ensuremath{\alpha}}_{2}}{(r+{\ensuremath{\alpha}}_{3})}\ensuremath{-}{\ensuremath{\alpha}}_{4}\mathrm{ln}r\ensuremath{-}{\ensuremath{\alpha}}_{5}\mathrm{sgn}(q){r}^{q}$, where ${\ensuremath{\alpha}}_{i}\ensuremath{\ge}0$ and $|q|\ensuremath{\le}1$, have the $\ensuremath{\gamma}$ numbers $\ensuremath{\gamma}(\ensuremath{-}1)=2$ and $\ensuremath{\gamma}(1)=\frac{12}{\ensuremath{\pi}}$. The appropriate $\ensuremath{\gamma}$ numbers are provided for other classes of potential shape including perturbed harmonic oscillators, and also for problems in one spatial dimension. The method yields in effect a recipe for the way ${E}_{N}$ depends on $N$ and all the parameters of the pair potential.

DOI
10.1103/physrevd.22.2062

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This paper concerns the ground-state energy EN{E}_{N}EN​ of a system of NNN identical bosons interacting via the attractive central pair potential V(rij)=\ensuremath−V0f(rija)V({r}_{\mathrm{ij}})=\ensuremath{-}{V}_{0}f(\frac{{r}_{\mathrm{ij}}}{a})V(rij​)=\ensuremath−V0​f(arij​​) and obeying nonrelativistic quantum mechanics. It is assumed that the potential shape fff is decreasing and can be represented as the envelope of each of two complementary families of power-law potentials \ensuremathα+\ensuremathβrp\ensuremath{\alpha}+\ensuremath{\beta}{r}^{p}\ensuremathα+\ensuremathβrp (one family is above fff and the other below) for suitable fixed p=p1p={p}_{1}p=p1​ and p=p2p={p}_{2}p=p2​. If \ensuremathϵ=\ensuremath−ma2EN(N\ensuremath−1)\ensuremathℏ2\ensuremath{\epsilon}=\ensuremath{-}\frac{m{a}^{2}{E}_{N}}{(N\ensuremath{-}1){\ensuremath{\hbar}}^{2}}\ensuremathϵ=\ensuremath−(N\ensuremath−1)\ensuremathℏ2ma2EN​​ and v=NmV0a22\ensuremathℏ2v=\frac{\mathrm{Nm}{V}_{0}{a}^{2}}{2{\ensuremath{\hbar}}^{2}}v=2\ensuremathℏ2NmV0​a2​, then it is proved that the entire collection of nonintersecting energy trajectories \ensuremathϵ=FN(v)\ensuremath{\epsilon}={F}_{N}(v)\ensuremathϵ=FN​(v), N=2,3,4,…N=2, 3, 4, \dots{}N=2,3,4,…, is bounded between the fixed curves (v,\ensuremathϵ)=(\ensuremath−\ensuremathγ(p)[s3f\ensuremath′(s)]\ensuremath−1,(v2)[2f(s)+sf\ensuremath′(s)])(v, \ensuremath{\epsilon})=(\ensuremath{-}\ensuremath{\gamma}(p){[{s}^{3}{f}^{\ensuremath{'}}(s)]}^{\ensuremath{-}1}, (\frac{v}{2})[2f(s)+s{f}^{\ensuremath{'}}(s)])(v,\ensuremathϵ)=(\ensuremath−\ensuremathγ(p)[s3f\ensuremath′(s)]\ensuremath−1,(2v​)[2f(s)+sf\ensuremath′(s)]), where the curve parameter s>0s>0s>0, and p=p1,p2p={p}_{1}, {p}_{2}p=p1​,p2​. Potentials, for example, with shapes f(r)=\ensuremathα1r+\ensuremathα2(r+\ensuremathα3)\ensuremath−\ensuremathα4lnr\ensuremath−\ensuremathα5sgn(q)rqf(r)=\frac{{\ensuremath{\alpha}}_{1}}{r}+\frac{{\ensuremath{\alpha}}_{2}}{(r+{\ensuremath{\alpha}}_{3})}\ensuremath{-}{\ensuremath{\alpha}}_{4}\mathrm{ln}r\ensuremath{-}{\ensuremath{\alpha}}_{5}\mathrm{sgn}(q){r}^{q}f(r)=r\ensuremathα1​​+(r+\ensuremathα3​)\ensuremathα2​​\ensuremath−\ensuremathα4​lnr\ensuremath−\ensuremathα5​sgn(q)rq, where \ensuremathαi\ensuremath≥0{\ensuremath{\alpha}}_{i}\ensuremath{\ge}0\ensuremathαi​\ensuremath≥0 and ∣q∣\ensuremath≤1|q|\ensuremath{\le}1∣q∣\ensuremath≤1, have the \ensuremathγ\ensuremath{\gamma}\ensuremathγ numbers \ensuremathγ(\ensuremath−1)=2\ensuremath{\gamma}(\ensuremath{-}1)=2\ensuremathγ(\ensuremath−1)=2 and \ensuremathγ(1)=12\ensuremathπ\ensuremath{\gamma}(1)=\frac{12}{\ensuremath{\pi}}\ensuremathγ(1)=\ensuremathπ12​. The appropriate \ensuremathγ\ensuremath{\gamma}\ensuremathγ numbers are provided for other classes of potential shape including perturbed harmonic oscillators, and also for problems in one spatial dimension. The method yields in effect a recipe for the way EN{E}_{N}EN​ depends on NNN and all the parameters of the pair potential.
Suppose EN{E}_{N}EN​ is the lowest energy of a translation-invariant system of NNN identical bosons which interact by attractive central pair potentials and obey nonrelativistic quantum mechanics. Sufficient conditions are prescribed on the potential to prove that EN{E}_{N}EN​ is bounded above by $({N}{2}){({K}{2})}^{\ensuremath{-}1}{E}_{K}$, where $N\ensuremath{\ge}\ensuremath{\mu}K$. The $\ensuremath{\mu}$ numbers are specified for various classes of potential shape. In cases where $\ensuremath{\mu}\ensuremath{\le}\frac{3}{2}$, it follows that ${E}_{N}\ensuremath{\le}\frac{1}{2}N(N\ensuremath{-}1){E}_{2}$ for $N\ensuremath{\ge}3$.
We study the ground-state energy of a system of N identical bosons, each having mass m, which interact in one dimension via the pair potential V(x)=\ensuremath{\gamma}\ensuremath{\Vert}x\ensuremath{\Vert} and obey nonrelativistic quantum mechanics. It is shown that the energy is given by the formula \ensuremath{\varepsilon}=C(N)(N-1)(${\ensuremath{\Elzxh}}^{2}$/ m)1/3{)}^{1/3})1/3(\ensuremath{\gamma}N/2)2/3{/2)}^{2/3}/2)2/3, where 1.01879(N)1.02333 for all N\ensuremath{\ge}2. The lower bound is provided by the ``equivalent two-body method'' whereas the upper bound is derived by the use of collective field theory. The general relation between these complementary theories is investigated.
We consider a system of N identical bosons which interact in one dimension via attractive pair potentials and obey nonrelativistic quantum mechanics. This system is studied from two complementary viewpoints. The equivalent two-body method approximates the system as a collection of (N-1) independent two-particle systems with coupling constants enhanced by the factor N/2, and this yields energy lower bounds. The collective-field method approaches the problem from the standpoint of the limit as N\ensuremath{\rightarrow}\ensuremath{\infty} and leads to energy upper bounds. We find that Gaussian trial functions for the N-particle Hamiltonian and Gaussian trial densities in the collective-field theory lead to precisely the same energy upper bounds. The upper bounds provided by field theory allow for systematic improvement via a variational principle. Details are worked out for two exactly soluble problems, namely, the harmonic oscillator and the attractive \ensuremath{\delta} potential.
Studies the ground-state energy of a system of N identical bosons, each having mass m, which interact in one dimension via the pair potential V(x)= gamma f(x/a) and obey non-relativistic quantum mechanics. A recent energy lower bound based on the known exact solution for the delta potential is compared to an earlier bound provided by the equivalent two-body method. The delta bound is good whenever the potential is very narrow and deep. For any bounded potential, the earlier energy bound is always better for large N. Detailed results and graphs are given for the sech-squared potential and the square-well potential.
A simple upper bound to the ground-state energy of a quantal system composed of NNN equal particles obeying Boltzmann or Bose statistics and interacting through the interparticle potential V(r)V(r)V(r) is established. This bound applies in the limit of large NNN; different expressions obtain depending on whether the potential is or is not singularly attractive at the origin. In the former case, the bound reads - $C{N}^{\frac{(4\ensuremath{-}q)}{(2\ensuremath{-}q)}}$, - qqq being the (negative) exponent characterizing the behavior of the pair potential at the origin through ${\mathrm{lim}}_{r\ensuremath{\rightarrow}0}[{r}^{q}V(r)]={V}_{0}$, $\ensuremath{-}\ensuremath{\infty}<{V}_{0}<0$ (of course, q<2q<2q<2 to prevent two-body collapse); in the latter case, it reads $\ensuremath{-}B{N}^{2}$. Explicit expressions for the constants CCC and BBB in terms of the pair potential V(r)V(r)V(r) are obtained; it is expected (and, in some cases, demonstrated) that the associated upper bound to the ground-state energy of the system approximates closely the actual value. It is also noted that, if for some non-negative value of ppp the quantity $\ensuremath{\int}{0}^{\ensuremath{\infty}}\mathrm{dr}{r}^{2} \mathrm{exp}(\ensuremath{-}{p}^{2}{r}^{2})V(r)$ is negative, the NNN-body system is unstable in the sense that, at large NNN, its total energy is negative and increases in modulus at least as N2{N}^{2}N2 (so that the binding energy per particle increases in modulus at least as NNN). Examples illustrating the nontrivial nature of this conclusion are displayed.
We study a bound system of N identical bosons interacting by model pair potentials of the form $V(r)=\ensuremath{\lambda}\mathrm{sgn}{(p)r}^{p}+\ensuremath{\mu}{/r}^{2},$ $\ensuremath{\lambda}>0,$ $\ensuremath{\mu}>~0.$ By using a variational trial function and the ``equivalent two-body method,'' we find explicit upper and lower bound formulas for the N-particle ground-state energy in arbitrary spatial dimensions d> 3d>~3d> 3 for the two cases p=2p=2p=2 and $p=\ensuremath{-}1.$ It is demonstrated that the upper bound can be systematically improved with the aid of a special large-N limit in collective field theory.