2
three-hole systems with the full configuration interaction
quantum Monte Carlo (FCIQMC) method.
FCIQMC is based on stochastic simulations of the
dynamic evolution of the wave function in imaginary
time. Different to the diffusion quantum Monte Carlo
(DMC) [23] with the fixed node approximation and the
auxiliary-field quantum Monte Carlo (AFQMC) [24] with
the phaseless approximation, no systematic approxima-
tion is made in FCIQMC [25–27], and it thus serves as
a highly accurate method to approach the ground state
wave functions. The annihilation procedure of the algo-
rithm enables it to overcome the fermionic sign problem
exactly, as long as enough walkers are used. In practice,
for Hubbard systems at large U, this means, with the cur-
rently available hardware, systems up to 26 sites can be
studied [21]. (A 26-site lattice represents a useful increase
in size compared to exact-diagonalisation, for which 20-
sites is the largest lattice size so far reported [4]). In the
present paper, we extend this to the study of a system
with a few holes, as well as report on spin-spin correlation
functions for the obtained exact ground-states.
The software NECI, a state-of-the-art implementation
of the FCIQMC algorithm, utilizes a very powerful par-
allelization and scales efficiently to more than 24000 cen-
tral processing unit cores [27]. The FCIQMC method
in a Slater determinant (SD) basis has been extended to
calculate ground and excited state energies, spectral and
Green’s functions for ab initio and model systems, as well
as properties via the one-, two-, three- and four-body re-
duced density matrices(RDMs). To study magnetism, we
need to use the replica-sampled 2-RDMs [28–30] to ob-
tain the spatial spin distribution. The replica-sampling
technique removes the systematic error in the RDM, at
the expense of requiring a second walker distribution.
The premise is to ensure that these two walker distribu-
tions are entirely independent and propagated in parallel,
sampling the same (in this instance ground-state) distri-
bution. This ensures an unbiased sampling of the desired
RDM, by ensuring that each RDM contribution is derived
from the product of an uncorrelated amplitude from each
replica walker distribution. By using replica-sampled 2-
RDMs the spin-spin correlation function, hˆ
Si·ˆ
Sji, can
be calculated, where iand jare lattice site indices. This
spin-spin correlation function can then be used to iden-
tify the specific type of magnetism of the ground states.
FCIQMC in a spin-adapted basis is also used to study
the partial polarization in three-hole systems. Spin-
adapted FCIQMC uses SU(2) symmetry (arising from
the vanishing commutator [ ˆ
H, ˆ
S2] = 0) conservation.
SU (2) symmetry is imposed via the graphical unitary
group approach (GUGA) [31–33] which dynamically con-
strains the total spin Sof a multi-configuration and
highly open-shell wave function in an efficacious man-
ner. The spin-adapted version of the FCIQMC algorithm
based on GUGA has been developed in our group [34, 35],
with – among others – applications to ab initio sys-
tem [36, 37] and Nagaoka ferromagnetism in one-hole
system [21]. With the spin-adapted method, the mag-
netisation of the ground state can be determined in a
reliable way, especially for systems with small spin gaps.
The results of spin-adapted FCIQMC show the partial
spin-polarization only appears in small, three-hole sys-
tem (less than 18 sites) [22], which is the second impor-
tant result of this work.
The rest of this paper is organized as follows: In Sec.
II, we briefly describe the methods, where we mainly
provide some more details on the measurements of the
spin-spin correlation function, hˆ
Si·ˆ
Sjifrom the replica-
sampled 2-RDMs in FCIQMC. In Sec. III, results about
the spatial spin distribution and partial spin-polarization
are discussed. Finally, we conclude in Sec. IV.
II. METHODS
The Hamiltonian of the Hubbard model in real space
takes the form
ˆ
H=−tX
hijiσ
a†
i,σaj,σ +UX
i
ni↑ni↓(1)
where a†
iσ (aiσ) creates (annihilates) an electron with spin
σon site i, and niσ =a†
iσaiσ is the particle number oper-
ator. Urefers to the Coulomb interaction strength. We
consider only nearest neighbour hopping terms, where t
is positive and is used as the unit of the energy. When U
is infinitely large, there will be no double occupancy and
the system can be treated with an effective Hamiltonian
with constrained hopping terms [22]
Heff =−tX
hijiσ
˜a†
i,σ ˜aj,σ,(2)
with ˜a†
i,σ =ai,σ(1 −ni,σ). In our current work, we want
to study the magnetic properties for finite Uand thus will
stay with the original Hamiltonian (1). Tough, we find
that our results for the three-hole systems in the large U
limit (see Sec. III(B)), coincide with the result of Riera
et al. [22] for the effective Hamiltonian, Eq. (2). In our
investigation we apply two different FCIQMC methods,
which are based on full CI expansions in terms of SDs
and in terms of spin eigenfunctions (spin-adapted basis
states) respectively.
FCIQMC is a projector QMC method for obtaining
the ground state wave function |Ψ0i. By Monte Carlo
simulation of the imaginary-time evolution of the wave
function
|Ψ(τ)i=e−τ(ˆ
H−E0)|Ψ(0)i,(3)
the ground state wave function is approached in the long
time limit |Ψ(τ→ ∞)i∝|Ψ0i.
In a previous work [21], we have investigated the mag-
netism for one hole and two holes systems by using the
spin-adapted (SU (2) conserving) FCIQMC method. We
extend these investigations to three-hole systems in this
work. With the spin-adapted method, the magnetisation