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Phys. Rev. B 58, R14685–R14688 (1998)

Phase separation in the two-dimensional Hubbard model: A fixed-node quantum Monte Carlo study

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A. C. Cosentini
Dipartimento di Fisica, Università di Roma La Sapienza, Piazzale Aldo Moro 2, I-00185 Rome, Italy
Istituto Nazionale di Fisica della Materia (INFM), Italy

M. Capone and L. Guidoni
Dipartimento di Fisica, Università di Roma La Sapienza, Piazzale Aldo Moro 2, I-00185 Rome, Italy
Istituto Nazionale di Fisica della Materia (INFM), Italy
International School for Advanced Studies (SISSA-ISAS), I-34014 Trieste, Italy

G. B. Bachelet
Istituto Nazionale di Fisica della Materia (INFM), Italy
Dipartimento di Fisica, Universita di Roma La Sapienza, Piazzale Aldo Moro 2, I-00185 Rome, Italy

Received 20 August 1998; published in the issue dated 1 December 1998

Fixed-node Green’s-function Monte Carlo calculations have been performed for very large 16×16 two-dimensional Hubbard lattices, large interaction strengths U=10,20, and 40, and many (1520) densities between empty and half-filling. The nodes were fixed by a simple Slater-Gutzwiller trial wave function. For each value of U we obtained a sequence of ground-state energies which is consistent with the possibility of a phase separation close to half-filling, with a hole density in the hole-rich phase which is a decreasing function of U. The energies suffer, however, from a fixed-node bias: more accurate nodes are needed to confirm this picture. Our extensive numerical results and their test against size, shell, shape, and boundary-condition effects also suggest that phase separation is quite a delicate issue, on which simulations based on smaller lattices than considered here are unlikely to give reliable predictions.

© 1998 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.58.R14685
DOI:
10.1103/PhysRevB.58.R14685
PACS:
71.10.Fd, 64.70.-p, 71.45.Lr