
4
UL, we identify a first-order AFM– SF phase transition,
signaled by a discontinuous jump of ψand θS[Fig. 2(e)].
This is in contrast to the second-order MI– SF transition
in the absence of the long-range interactions (UL= 0).
For larger Uv/U the AFM phase extends towards higher
tunneling strengths. AFM– SF transitions in the context
of entanglement properties have recently been studied
in three-component BH models with long-range interac-
tions [38]. For larger UL, we observe second-order phase
transitions from AFM to AF-SS and from CDW to SS
phases, along lines of constant UL/U [Fig. 2(f,g)]. The
second-order phase transitions from AFM to AF-SS and
CDW to SS are supported by perturbative estimations,
cf. black lines in Fig. 2(a,c) [47,56].
0.2
0.6
1.0
1.4
1.8
UL/U
(a) (b)
0.0 0.2 0.4 0.6 0.8 1.0
zt/U
0.1
0.4
0.7
1.0
1.3
UL/U
(c)
0.0 0.2 0.4 0.6 0.8 1.0
zt/U
(d)
0.0 0.2 0.4 0.6
zt/U
0.0
0.5
1.0
θD/2, θS/2, ψ
AFM SF
(e)
0.0 0.2 0.4 0.6 0.8
zt/U
CDW SS SF
(f)
0.2 0.4 0.6 0.8
zt/U
AFM
AF-SS
SF
(g)
0 0.4 0.8
ψ
012
θS
0 0.4 0.8
ψ
012
θS
012
θD
Figure 2. Mean field phase diagrams for a balanced-spin mix-
ture at unity filling, ρ= 2.The calculations are performed
for Us/Uv≈4.64 (a,b) and at Us/Uv≈0.33 (c,d). (a,c) De-
pendence of superfluid order parameter ψ. The solid lines are
perturbative estimations for the transition. (b,d) Dependence
of density and antiferromagnetic order parameters θDand
θS.(e,f,g) Cuts along the phase diagrams for Us/Uv≈4.64
at constant UL/U = 0.63 and UL/U = 1.41 (e,f) and for
Us/Uv≈0.33 at UL/U = 1.3 (g), indicated by thin hori-
zontal lines in (a,c). The basis truncation nmax =mmax = 3
leads to a saturation of the superfluid order parameter at large
tunneling.
C. Phase Diagrams for different U12/U
We now discuss the phase diagrams for different ratios
of inter- and intra-spin interactions U12/U and scalar and
vectorial long-range interactions Us/Uv. Besides the ho-
mogeneous phases, we also calculate the regions of phase
separation between the two spin states (PS), which nat-
urally occur in two-component BH models with repulsive
inter-spin interactions [37,41–45,57,58]. Additional re-
gions of phase instability arise from the concurring long-
range interactions [17,46]. To calculate the energy of a
phase separated state, the system is divided into halves
(A, B): one with higher spin-up density (ρA
↑> ρA
↓) and
the other with higher spin-down density (ρB
↓> ρB
↑), while
imposing a density conservation constraint in each of the
halves, i.e., ρ≡ρA,B
↑+ρA,B
↓= 2 to ensure unity filling.
We further assume either hˆ
ΘDi= 0 or hˆ
ΘSi= 0. Phase
instability, on the other hand, is signaled by a negative
compressibility, ∂ρµ < 0 [46], where µ(ρ) = ∂ρE(ρ) is
the chemical potential as a function of the density ρ. We
calculate the derivative numerically by using the energy
densities E(ρ) extracted from the variational ansatz in
Eq. (S22) [47].
We first discuss the results for Us/Uv>1, see Fig. 3(a-
c). For dominating intra-spin interactions [Fig. 3(a)],
U12 < U, the phases are identical as those obtained for
U12 =Uassuming a uniform mixture as discussed in
the context of Fig. 2. We additionally find a region of
instability in the SS phase for U12 ≤U. Our observa-
tions of phase instability are qualitatively different from
the results for spinless systems [17,46], which predict sta-
ble supersolid phases at integer filling in two-dimensional
systems. For U12 =U[Fig. 3(b)], the mixed CDW state
|φe, φoi=|↑↓,0i, the entangled state |φe, φoi=|↑↑,0i+
|↓↓,0iand the fully phase-separated (PS) configuration
with ρA
↑=ρB
↓= 2 are degenerate. Increasing U12/U
from 0.9 to 1 shrinks the CDW region: CDW→AFM
transition boundary is shifted towards higher UL/U and
CDW→AF-SS transition boundary is shifted towards
lower zt/U. For U12 > U [Fig. 3(c)], the obtained CDW,
SS and SF are fully phase separated.
In the case of dominating vectorial long-rage interac-
tions Us/Uv<1 [Fig. 3(d-f)], the phase diagrams for
U12 < U and U12 =Uare qualitatively similar: Besides
AFM, AF-SS and SF phases, we find extended regions
of instability in the AF-SS phase, which is similar to the
SS case. For U12 > U [Fig. 3(f)], the SF is replaced by
a fully PS SF, which is compatible with the results for
Us/Uv>1. We also find that both the AF-SS and the
instability region shrink when U12/U is increased above
1. In contrast, boundaries between insulating regions
(PS CDW, AFM) and the phase separated non-insulating
state (PS SS, PS SF) do not change with U12/U, as the
energy of the PS phases and the AFM phase do not de-
pend on U12.
We note here two limitations of our simulations.
First, the identification of different phases in the phase
diagrams relies on numerical minimization [47] in a
high-dimensional landscape. This can lead to spuri-
ous solutions, such as the scattered instability points
in Fig. 3(a,b) and the irregular phase boundaries in
Fig. 2and 3. Second, there is a small region of fully PS
SS for U12 =Uand Us/Uv>1, cf. Fig. 3(b). This is due
to the relatively small Hilbert space (nmax =mmax = 3)
used for the simulations. We expect that a larger Hilbert