This paper presents a thorough study of the properties of inhomogeneous, harmonically-confined quasi-one dimensional Bose gases as a function of the 3D scattering length . The behavior of confined Bose gases strongly depends on the ratio of the harmonic oscillator length in the tight transverse direction, , to the interaction range and to the average interparticle distance , where denotes the 3D central density.
Quasi-1D bosonic gases have been realized experimentally in highly-elongated harmonic traps. The strength of atom-atom interactions can be varied over a wide range by tuning the value of the 3D -wave scattering length through application of an external magnetic field in the proximity of a Feshbach resonance. For , the scattering length determines to a good approximation the effective 1D scattering length and the effective 1D coupling constant , which can be, just as the 3D coupling constant, tuned to essentially any value including zero and . By exploiting Feshbach resonance techniques, one should be able to achieve strongly-correlated quasi-one dimensional systems. The strong coupling regime is achieved for , it includes the TG gas, where a system of interacting bosons behaves as if it consisted of non-interacting spinless fermions, and the so-called unitary regime, where the properties of the gas become independent of the actual value of . In the unitary regime, the gas is dilute, that is, , and at the same time strongly-correlated, that is, .
The present analysis is carried out within various theoretical frameworks. We obtain the 3D energetics of the lowest-lying gas-like state of the system using a microscopic FN-MC approach, which accounts for all degrees of freedom explicitly. The resulting energetics are then used to benchmark our 1D calculations. Full microscopic 1D calculations for contact interactions with renormalized coupling constant result in energies that are in excellent agreement with the full 3D energies. This agreement implies that a properly chosen many-body 1D Hamiltonian describes quasi-one dimensional Bose gases well.
We also consider the LL and the hard-rod equation of state of a 1D system treated within the LDA. These approaches provide a good description of the energy of the lowest-lying gas-like state for as few as five or ten particles. Finite size effects are to a good approximation negligible. Our detailed microscopic studies suggest that these LDA treatments provide a good description of quasi-one dimensional Bose gases. In particular, we suggest a simple treatment of 1D systems with negative using the hard-rod equation of state.
Finally, we address the question of whether the lowest-lying gas-like state of inhomogeneous quasi-one dimensional Bose gases is actually stable. We find, utilizing a variational 1D many-body framework, that the lowest-lying gas-like state is stable for negative coupling constants, up to a minimum critical value of . Our numerical results suggest that the stability condition can be expressed as . Since our conclusions are derived from variational 1D calculations, more thorough microscopic calculations are needed to confirm our findings. We believe, however, that our findings will hold even in a 3D framework or when three-body recombination effects are included explicitly.
While our study was performed for inhomogeneous quasi-one dimensional Bose gases, many findings also apply to homogeneous quasi-one dimensional Bose gases. Furthermore, the Fermi-Bose mapping [Gir60,GB04,CS99,GO03], which allows one to map an interacting 1D gas of spin-polarized fermions to an interacting 1D gas of spin-polarized bosons, suggests that many of the results presented here for quasi-one dimensional Bose gases may directly apply to quasi-one dimensional Fermi gases.