XXZ spin-12 representation of a finite-U Bose-Hubbard chain at half-integer filling

Domenico Giuliano, Davide Rossini, Pasquale Sodano, and Andrea Trombettoni
Phys. Rev. B 87, 035104 – Published 3 January 2013

Abstract

Using a similarity Hamiltonian renormalization procedure, we determine an effective spin-12 representation of the Bose-Hubbard model at half-integer filling and at a finite onsite interaction energy U. By means of bosonization, we are able to recast the effective Hamiltonian as that of a spin-12 XXZ magnetic chain with pertinently renormalized coupling and anisotropy parameters. We use this mapping to provide analytical estimates of the correlation functions of the Bose-Hubbard model. We then compare such results with those based on density matrix renormalization group numerical simulations of the Bose-Hubbard model for various values of U and for a number L of lattice sites as low as L30. We find an excellent agreement up to 10% between the output of analytical and numerical computations, even for relatively small values of U. Our analysis implies that, also at finite U, the one-dimensional Bose-Hubbard model with suitably chosen parameters may be seen as a quantum simulator of the XXZ chain.

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  • Received 9 October 2012

DOI:https://doi.org/10.1103/PhysRevB.87.035104

©2013 American Physical Society

Authors & Affiliations

Domenico Giuliano1, Davide Rossini2, Pasquale Sodano3, and Andrea Trombettoni4

  • 1Dipartimento di Fisica, Università della Calabria, Arcavacata di Rende I-87036, Cosenza, Italy and INFN, Gruppo collegato di Cosenza, Arcavacata di Rende I-87036, Cosenza, Italy
  • 2NEST, Scuola Normale Superiore & Istituto Nanoscienze-CNR, I-56126 Pisa, Italy
  • 3International Institute of Physics, Universidade Federal do Rio Grande do Norte, 59012-970, Natal, Brazil and INFN, Sezione di Perugia, Via A. Pascoli, I-06123, Perugia, Italy
  • 4CNR-IOM DEMOCRITOS Simulation Center and SISSA, Via Bonomea 265 I-34136 Trieste, Italy and INFN, Sezione di Trieste, I-34127 Trieste, Italy

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Vol. 87, Iss. 3 — 15 January 2013

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