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Journal of Experimental and Theoretical Physics

One-parametric dependences of the spectra, scattering lengths, and recombination coefficients for a system of three bosons

Ф. М. Пеньков

Published Sep 1, 2003• 11 citations
Publisher

Abstract

A model of a two-pole pair t -matrix for the description of three-boson systems with r 0 / a 0 ≪ 1 is studied. The position of the second pole on the nonphysical sheet is treated as a parameter of the Faddeev integral equation. Close agreement with the calculations performed for realistic potentials was obtained, and interaction parameters for three bosons that were not calculated earlier were predicted.

DOI
10.1134/1.1618335

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A model of a two-pole pair t -matrix for the description of three-boson systems with r 0 / a 0 ≪ 1 is studied. The position of the second pole on the nonphysical sheet is treated as a parameter of the Faddeev integral equation. Close agreement with the calculations performed for realistic potentials was obtained, and interaction parameters for three bosons that were not calculated earlier were predicted.
We consider the three-boson problem with $\ensuremath{\delta}$-function interactions in one spatial dimension. Three different approaches are used to calculate the phase shifts, which we interpret in the context of the effective range expansion, for the scattering of one free particle off a bound pair. We first follow a procedure outlined by McGuire in order to obtain an analytic expression for the desired SSS-matrix element. This result is then compared to a variational calculation in the adiabatic hyperspherical representation, and to a numerical solution to the momentum-space Faddeev equations. We find excellent agreement with the exact phase shifts, and comment on some of the important features in the scattering and bound-state sectors. In particular, we find that the 1+21+21+2 scattering length is divergent, marking the presence of a zero-energy resonance which appears as a feature when the pairwise interactions are short range. Finally, we consider the introduction of a three-body interaction, and comment on the cutoff dependence of the coupling.
A model for the system of three identical bosons with interactions containing a Feshbach resonance is developed. The model assumes short-range interactions, but includes the energy dependence of the interaction due to the finite width of the resonance. The model is applied to the system of three bosons trapped in a harmonic potential. In particular we study the energy in the limit of infinite scattering length. In this limit the energy does not depend on the scattering length, but it does depend on the other parameters of the resonance.
We investigate finite-range effects in systems with three identical bosons. We calculate recombination rates and bound state spectra using two different finite-range models that have been used recently to describe the physics of cold atomic gases near Feshbach resonances where the scattering length is large. The models are built on contact potentials which take into account finite-range effects; one is a two-channel model and the other is an effective range expansion model implemented through the boundary condition on the three-body wavefunction when two of the particles are at the same point in space. We compare the results with the results of the ubiquitous single-parameter zero-range model where only the scattering length is taken into account. Both finite-range models predict variations of the well-known geometric scaling factor 22.7 that arises in Efimov physics. The threshold value at negative scattering length for creation of a bound trimer moves to higher or lower values depending on the sign of the effective range compared to the location of the threshold for the single-parameter zero-range model. Large effective ranges, corresponding to narrow resonances, are needed for the reduction to have any noticeable effect.
The threshold recombination coefficient for three bosons whose two-body scattering length aaa is positive and large compared with the nominal range of the potentials is shown to proceed via a crossing of hyperspherical adiabatic potential curves at $R\ensuremath{\approx}2.6a$. The hidden crossing theory gives a simple expression for the rate in terms of the scattering length and a phase $\ensuremath{\Delta}$. The phase depends upon the details of the interaction, and varies from species to species, however an upper limit to the rate which depends only upon the scattering length emerges from the hidden crossing theory.