Magnetism and Quantum Melting in Moir e-Material Wigner Crystals Nicol as Morales-Dur an1Pawel Potasz2and Allan H. MacDonald1 1Department of Physics The University of Texas at Austin Austin Texas 78712 USA

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Magnetism and Quantum Melting in Moir´e-Material Wigner Crystals
Nicol´as Morales-Dur´an,1Pawel Potasz,2and Allan H. MacDonald1
1Department of Physics, The University of Texas at Austin, Austin, Texas, 78712, USA
2Institute of Physics, Faculty of Physics, Astronomy and Informatics,
Nicolaus Copernicus University, Grudziadzka 5, 87-100 Toru´n, Poland
(Dated: July 21, 2023)
Recent experiments have established that semiconductor-based moir´e materials can host incom-
pressible states at a series of fractional moir´e-miniband fillings. These states have been identified as
generalized Wigner crystals in which electrons localize on a subset of the available triangular-lattice
moir´e superlattice sites. In this article, we use momentum-space exact diagonalization to investigate
the many-body ground state evolution at rational fillings from the weak-hopping classical lattice
gas limit, in which only spin degrees-of-freedom are active at low energies, to the strong-hopping
metallic regime where the Wigner crystals melt. We specifically address the nature of the magnetic
ground states of the generalized Wigner crystals at fillings ν= 1/3 and ν= 2/3.
I. INTRODUCTION
It is now several years since Wu et al. [1] pointed out
that the Hamiltonian of interacting holes in the moir´e
bands of transition metal dichalcogenide (TMD) heter-
obilayers can be mapped to the triangular lattice Hub-
bard model. Experiments quickly confirmed the validity
of this assertion by observing Mott insulating states at
band filling νN/M = 1 of the moir´e superlattice [2–
5], where Nis the number of holes and Mthe number of
moir´e unit cells in the system. Subsequent experiments
have established that TMD-based moir´e materials also
exhibit correlated insulating states at a discrete series
of fractional fillings of the lowest moir´e miniband [5–10].
These insulating states form because electrons localize on
a subset of moir´e sites in order to minimize strong long-
range Coulomb interactions. Because they break transla-
tional symmetry, they are reminiscent of the Wigner crys-
tals expected to appear in the two-dimensional electron
gas (2DEG) at very low densities [11]. There are how-
ever some qualitative differences between Wigner crystals
formed in an electron gas with continuous translational
symmetry, and the incompressible states at fractional fill-
ings in moir´e materials, which have only discrete trans-
lational symmetry. Most importantly, the moir´e super-
lattice potential narrows bands and reduces the relevant
single-particle energy scales, making interactions domi-
nant in much of the available phase space.
The incompressible states in moir´e superlattices are
commonly referred to as generalized Wigner crystals and
we adopt that terminology in this paper. The ubiquity of
robust crystalline states at fractional fillings in the moir´e
material platform opens up a new thread in the study
of strongly interacting electrons in low dimensions and
promises to reveal new physics. Given the abundance
of distinct moir´e semiconductor heterostructures, even
within the group VI transition metal dichalcogenide fam-
ily alone, and the ability to tune samples through large
ranges of filling factor by varying gate voltage, it seems
likely that it will be possible to realize a rich variety of
generalized Wigner crystal states with distinct structural
and magnetic properties in the coming years.
The emergence of incompressible states at non-integer
partial band filling can be explained only if inter-site
electron-electron interactions are included. Recent ex-
periments have therefore established moir´e TMDs as a
platform to simulate extended Hubbard models whose
Hamiltonians have tunable hoppings tn, on-site inter-
action U0, and long-range interaction strengths Un(n
stands for n-th neighbor). Assisted hopping and direct
exchange non-local interaction terms can also play a cru-
cial role [12] in determining the magnetic properties of
moir´e Hubbard systems. The mapping to a Hubbard
model is a one-band approximation, whose applicability
at ν1 has generally been confirmed by experiment. For
fillings above half-filling, there is a competition between
the upper Hubbard band and remote bands; hence the
simple one-band Hubbard model is often insufficient. For
that reason, in this work we focus on the regime ν < 1,
having addressed ν= 1 in a previous study [12, 13].
In moir´e superlattices, localization of electrons in an
insulating state is expected [1] in the long-moir´e-period
narrow-moir´e-band limit. In this regime, the dominant
energy scale is U0at ν= 1 and U1for 1/3ν < 1. When
the twist angle is increased and the moir´e period de-
creased, or a displacement field is applied to decrease the
moir´e potential strength, the effective hopping parame-
ters tbetween moir´e lattice sites increase and eventually
become comparable to inter-site interaction strengths U1,
complicating the electronic properties. The interplay be-
tween spin and charge degrees of freedom can give rise
to different magnetic orders at each filling factor. For
example, recent experiments have reported that some of
the crystal states are striped phases [8], and that antifer-
romagnetic interactions are frustrated for ν= 2/3 band
filling factor [14]. When hopping is strong enough to
overcome the near-neighbor interaction, the Wigner crys-
tal will melt into a liquid state – the Mott-Wigner tran-
sition. Interestingly a recent experiment performed on
MoSe2/WS2observed that the charge gap continuously
vanishes as the superlattice potential is weakened [10].
Further experiments have shown that the charge gaps
of the generalized Wigner crystal states are asymmetric
arXiv:2210.15168v2 [cond-mat.str-el] 20 Jul 2023
2
with respect to half-filling (ν= 1) of a single spinful
band, and also with respect to quarter-filling (ν= 1/2)
[6] and demonstrate the role of quantum fluctuations in-
volving remote bands, as we will show in this work, before
and across the Mott-Wigner transition.
The magnetic order of the generalized Wigner crys-
tal phases, as well as the nature of their bandwidth
and density-tuned quantum melting transitions are still
a matter of debate. Previous theoretical efforts to un-
derstand moir´e Wigner crystals and their evolution with
interaction strength have focused on the deep crystalline
regime [15–17], where classical Monte Carlo simulations
can be used to investigate the ground state charge order
at different fillings. Hartree-Fock [18–20] and classical
Monte Carlo studies [21] have addressed the competition
between different charge and spin orders in the crystal
phase, and its transition to metal when bandwidth or
density are tuned. An analysis that includes quantum
fluctuations and goes beyond mean-field is needed, how-
ever, since mean-field theory approximations are known
to favor ferromagnetic groundstates and to overestimate
the stability of insulating states in the proximity of metal-
insulator transitions.
In this work, we report on a finite-system exact di-
agonalization study of semiconductor moir´e materials at
fractional filling factors. Starting from the continuum
model description [1], we add relevant electron-electron
interactions projected to the topmost moir´e band and ob-
tain the many-body spectrum. We find, as already sug-
gested by experiment, that a rich set of fractional band
fillings νsupport correlated insulating states with tun-
able magnetic properties. We show that there is an over-
riding competition between antiferromagnetism and fer-
romagnetism particularly at ν= 2/3 band filling, which
we explain using a low-energy effective spin model de-
scription and relate to a recent experiment [14]. We also
address the Mott-Wigner transitions at fractional fillings,
finding that as in the ν= 1 case they are not strongly
first order.
II. MOIR´
E MATERIAL MODEL
A. Continuum model
Our starting point is the continuum model description
of TMD heterobilayers with type-I or type-II band align-
ment [1]. In this case the topmost moir´e band is concen-
trated in one of the layers, which we refer to as the active
layer, depicted in red in Fig. 1(a)-(b). The influence of
the second layer, shown in blue in Fig. 1(a)-(b), is re-
sponsible for a moir´e potential that affects charge carriers
in the active layer. The moir´e pattern can be induced by
a small twist angle θor a lattice mismatch δbetween
the two layers. The moir´e lattice constant is given by
aM=a0/(θ2+δ2)1/2, with a0the lattice constant of
the active TMD layer. To date most heterobilayer ex-
periments have focused on unrotated WSe2/WS2with a
moir´e lattice constant of aM8.2 nm, or MoSe2/WS2,
with a moir´e lattice constant of aM7.5 nm. Because
the moir´e lattice constant reaches a maximum, the sys-
tem is expected to be less sensitive to twist angle disorder
at zero twist angle.
Valley and spin are locked in TMD heterobilayers and
the valley (or spin) projected continuum Hamiltonian is
given by [1]
H0=2
2mk2+ ∆(r),(1)
∆(r) =2VmX
j=1,3,5
cos(bj·r+ψ).(2)
The first term in Eq. (1), which corresponds to the kinetic
energy of carriers in the top moir´e band, is diagonal in
momentum space and the second term, the moir´e poten-
tial, is diagonal in coordinate space. The moir´e potential
depends on only two parameters (Vm, ψ) because [1] of
the system’s C3symmetry. The phase ψfixes the ge-
ometry of the moir´e superlattice, which we take to be
triangular as it is in most of the TMD heterostructures,
and the strength of the moir´e potential Vmcan be re-
lated to the experimentally tunable displacement field.
For concreteness, throughout this work we take the ef-
fective mass m= 0.45 m0and ψ= 45, corresponding
to WSe2/WS2[22]. We take the modulation potential
strength Vmas an experimentally controllable parameter
since it has been demonstrated to be sensitive to the dis-
placement field D. The form we have used for the moir´e
modulation parameter assumes that it varies smoothly
with position on the moir´e scale; higher harmonics in the
plane-wave expansion are more important in longer pe-
riod moir´es in which relation relative to rigidly twisted
bilayers is stronger.
An example of the bandstructure obtained from di-
agonalizing Eq. (1) is shown in Fig. 1(c). We label
the band energies of Eq. (1) as ϵn
k, while the eigen-
states can be written in a plane wave expansion as
|n, ψk=PGzn
k,G|k+G, where nis a band index
and Gare reciprocal lattice vectors. In order to study
the emerging many-body phases we consider the interact-
ing Hamiltonian projected to the topmost moir´e valence
band (hence we omit band index)
H=X
k
ϵkc
kσckσ+X
i,j,k,l
σ,σ
Vσ,σ
i,j,k,l
2c
kiσc
kjσcklσckkσ,(3)
where the Coulomb matrix elements are given by
Vσ,σ
i,j,k,l =1
AX
Gi,Gj
Gk,Glz
ki,Giz
kj,Gjzkk,Gkzkl,Gl2πe2
ε q .(4)
The summation involving the term in brackets results
from the projection of interactions to a single band and
can be rewritten in terms of the form factors, as described
3
elsewhere [23]. In Eq. (4), q=|ki+GikkGk|is
the momentum transfer, Ais the area of the system,
εthe effective dielectric constant, and total momentum
conservation is implicit.
FIG. 1. (a) Schematics of a TMD heterobilayer with metallic
gates at distance dfrom the sample. By varying gate voltages
a displacement field is applied. (b) Schematics of the heter-
obilayer in momentum space. Charge carriers populate the
active WSe2band while the presence of a WS2layer generates
the moir´e potential, Eq. (2), whose strength is modified by
the displacement field D. (c) Example of WSe2/WS2moir´e
minibands obtained from Eq. (1), with Vm= 40 meV. (d)
Evolution of the energy scales of the problem as Vmis varied:
the interaction strength UM(green), the kinetic energy scale
WM(black), the bandwidth B(blue) and the gap to the first
remote ∆R(brown).
B. Exact diagonalization methodology
In this article we take the same approach as in pre-
vious work [12, 13], utilizing exact diagonalization (ED)
to solve the many-body Hamiltonian. We present our
results in phase diagrams that depend on dimensionless
parameters obtained by taking ratios of the relevant en-
ergy scales of the system. In particular, three energy
scales can be identified; the moir´e potential depth Vm,
the interaction strength UM=e2/(εaM), and the kinetic
energy scale WM=2/ma2
M. By varying the two ratios
of these three scales, we can simulate any heterobilayer as
long as the moir´e period is much larger than the micro-
scopic lattice constant. This ensures that our conclusions
apply for arbitrary heterobilayers as long as their low en-
ergy physics is captured by the continuum model, Eq.
(1) and that the shape of the moir´e potential is similar to
that of a triangular lattice model. The energy gap to the
remote moir´e bands ∆Rcan, in principle, be viewed as
another relevant energy scale. We take parameter values
such that this scale is always larger than all other scales
involved, as can be seen in Fig. 1(d), justifying the sin-
gle band projection of Eq. (3). As we have pointed out
above, however, interactions renormalize bands more at
higher electron densities. For this reason the single-band
approximation should be treated with caution for fillings
ν > 1, where remote band mixing is often relevant.
The model we study has orbital and spin degrees of
freedom, discrete triangular lattice translational symme-
try, SU(2) spin-rotational invariance, and no spin-orbit
coupling. The Hilbert space can be divided into smaller
subspaces with total momentum Kwith discrete values
determined by the number of moir´e unit cells M, to-
tal spin S, and azimuthal spin Sz. The basis is con-
structed in an occupation number representation, dis-
tributing particles among single-particle states labeled by
Szquantum number and quasi-particle (kx, ky) momen-
tum. The total number of possible configurations Nconf
for particles distributed on Msingle particle states with
Nspins up and Nspins down is determined by a prod-
uct of binomial coefficients, Nconf =M
N·M
N. The
many-body Hamiltonian projected to a given total mo-
mentum Kis diagonalized in Szsubspaces. We do not
rotate the Hamiltonian matrix to a Sbasis as this is
an additional computational cost, and instead determine
the ground state total total spin Sby identifying mul-
tiplets from the Sz-dependent energy eigenvalues. The
total spin Sassignments have been confirmed by calcu-
lating the spin structure factor S(q= 0). For a given
momentum, the S-multiplet structure implies that the
largest subspace corresponds to the lowest possible Sz
which contains states with all values of total spin S.
All of our exact diagonalization calculations are limited
only by the maximal matrix size of a given subspace, with
the largest subspace corresponding to the lowest possible
Sz. The results presented here correspond to systems
containing M= 9,12 and 16 moir´e unit cells. Despite the
limited system sizes that can be reached with the exact
diagonalization method, important information can still
be extracted concerning the behaviors of charge gaps and
the nature of the magnetic order of insulating states. Nu-
merical non-perturbative approaches, like the one taken
in this paper or DMRG, are particularly important in the
quantum melting regime, where Hartree-Fock is known
to overestimate the stability of the insulating phase.
III. FINITE-SIZE PHASE DIAGRAMS
A phase diagram for TMD heterobilayers as a function
of filling factor and the kinetic-energy-scale to moir´e-
depth ratio W/Vmis shown in Fig. 2(a) . The color
scale specifies the ratio of the charge gap to the Coulomb
interaction-energy scale ∆c/U. A finite value of the
charge gap indicates an incompressible state, while a van-
ishing charge gap indicates a metallic state. The charge
gap is extracted from the many-body spectrum via the
摘要:

MagnetismandQuantumMeltinginMoir´e-MaterialWignerCrystalsNicol´asMorales-Dur´an,1PawelPotasz,2andAllanH.MacDonald11DepartmentofPhysics,TheUniversityofTexasatAustin,Austin,Texas,78712,USA2InstituteofPhysics,FacultyofPhysics,AstronomyandInformatics,NicolausCopernicusUniversity,Grudziadzka5,87-100Toru´...

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Magnetism and Quantum Melting in Moir e-Material Wigner Crystals Nicol as Morales-Dur an1Pawel Potasz2and Allan H. MacDonald1 1Department of Physics The University of Texas at Austin Austin Texas 78712 USA.pdf

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