Abstract

We discuss how positions of critical points of the three-dimensional Bose-Hubbard model can be accurately obtained from variance of the on-site atom number operator, which can be experimentally measured. The idea that we explore is that the derivative of the variance, with respect to the parameter driving the transition, has a pronounced maximum close to critical points. We show that Quantum Monte Carlo studies of this maximum lead to precise determination of critical points for the superfluid-Mott insulator transition in systems with mean number of atoms per lattice site equal to one, two, and three. We also extract from such data the correlation-length critical exponent through the finite-size scaling analysis and discuss how the derivative of the variance can be reliably computed from numerical data for the variance. The same conclusions apply to the derivative of the nearest-neighbor correlation function, which can be obtained from routinely measured time-of-flight images.

Highlights

  • The field of quantum phase transitions is significant for both fundamental and practical reasons1–3

  • One of the key current problems in accurate testing of the RG theory at the lambda transition is that gravity broadens the transition

  • We have studied equilibrium properties of the 3D Bose-Hubbard model focusing our attention on the variance of the on-site atom number operator and its derivative with respect to the parameter driving the superfluid-Mott insulator transition

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Summary

Introduction

The field of quantum phase transitions is significant for both fundamental and practical reasons. Despite fascinating experimental efforts that have been reported so far, the current characterization of quantum phase transitions in best cold atom simulators is nowhere near the level of accuracy that is found in top condensed matter experiments. To justify this statement and to place the research discussed in this paper in a broader context, we compare measurements of the lambda transition in liquid 4He to measurements of the superfluid–Mott insulator transition in the two-dimensional (2D) cold atom cloud. One of the key current problems in accurate testing of the RG theory at the lambda transition is that gravity broadens the transition

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