Long-Range Free Fermions Lieb-Robinson Bound Clustering Properties and Topological Phases Zongping Gong1 2Tommaso Guaita1 2 3and J. Ignacio Cirac1 2 1Max-Planck-Institut f ur Quantenoptik Hans-Kopfermann-Straße 1 D-85748 Garching Germany

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Long-Range Free Fermions: Lieb-Robinson Bound, Clustering Properties, and Topological Phases
Zongping Gong,1, 2 Tommaso Guaita,1, 2, 3 and J. Ignacio Cirac1, 2
1Max-Planck-Institut f¨
ur Quantenoptik, Hans-Kopfermann-Straße 1, D-85748 Garching, Germany
2Munich Center for Quantum Science and Technology, Schellingstraße 4, 80799 M¨
unchen, Germany
3Dahlem Center for Complex Quantum Systems, Freie Universit¨
at Berlin, 14195 Berlin, Germany
(Dated: December 5, 2022)
We consider free fermions living on lattices in arbitrary dimensions, where hopping amplitudes follow a
power-law decay with respect to the distance. We focus on the regime where this power is larger than the
spatial dimension (i.e., where the single particle energies are guaranteed to be bounded) for which we provide
a comprehensive series of fundamental constraints on their equilibrium and nonequilibrium properties. First
we derive a Lieb-Robinson bound which is optimal in the spatial tail. This bound then implies a clustering
property with essentially the same power law for the Green’s function, whenever its variable lies outside the
energy spectrum. The widely believed (but yet unproven in this regime) clustering property for the ground-
state correlation function follows as a corollary among other implications. Finally, we discuss the impact of
these results on topological phases in long-range free-fermion systems: they justify the equivalence between
Hamiltonian and state-based definitions and the extension of the short-range phase classification to systems
with decay power larger than the spatial dimension. Additionally, we argue that all the short-range topological
phases are unified whenever this power is allowed to be smaller.
Introduction.—Locality is a central concept in quantum
many-body physics [1]. One of the most important implica-
tions of locality, which explicitly means the Hamiltonian is a
sum of local terms, is the Lieb-Robinson bound that claims
a “soft” light cone for correlation propagation [24]. Further
assuming an energy gap in the Hamiltonian, locality implies
that the ground-state correlation functions should decay ex-
ponentially [5,6]. This so-called clustering property gives
a partial justification for studying phases of quantum matter
[7] by focusing on short-range correlated many-body states,
which typically obey entanglement area laws [8,9] and admit
efficient representations based on tensor networks [10].
The past couple of years has witnessed a series of break-
throughs on generalizing the above locality-related results
to those “not-so-local” quantum many-body systems with
power-law decaying interactions [1121], commonly dubbed
long-range systems [22]. This topic is of both fundamen-
tal and pratical importance as long-range interactions appear
ubiquitously in nature and quantum simulators [2327]. In
particular, the problem of finding Lieb-Robinson bounds with
optimal light-cone behaviors has recently been solved for both
interacting [20] and noninteracting (free-fermion) [18] long-
range systems. In contrast, other results such as clustering
properties and phase classifications remain to be improved
or explored, even on the noninteracting level [28]. We note
that, despite their simplicity, free fermions can already ac-
commodate various topological phases [2931], whose long-
range generalizations have been considered in various specific
models [3237] and may be realized effectively in spin sys-
tems such as atomic arrays [38,39] and NV centers [40].
Also, long-range models appear naturally in the context of
fermionic Gaussian projected entangled pair states [4143].
In this work, we report some essential progress on long-
range free fermions, focusing on universal and rigorous results
both in and out of equilibrium. First, we derive a new Lieb-
Robinson bound as the noninteracting counterpart of that in
Ref. [12], which is optimal in the spatial tail but not in the
light cone. This bound implies an (almost) optimal cluster-
ing property for Green’s functions, leading to a widely be-
lieved ground-state clustering property among other appli-
cations. The latter result justifies the equivalence between
state and Hamiltonian formalisms for long-range free-fermion
topological phases. In addition, we argue that the topologi-
cal classification of short-range phases remains applicable to
long-range phases if the decay power is larger than the spatial
dimension, and collapses otherwise.
Setup.—For simplicity, we focus on free fermions living on
ad-dimensional hypercubic lattice ΛZdwith particle num-
ber conservation, where possible internal states (e.g., spin)
per site form a set I. The generalization to the cases with-
out number conservation and other lattices is straightforward
[44]. Denoting ˆc
rs/ˆcrsas the creation/annihilation operator of
a fermion with internal state sIat site rΛ, we know that
the Hamiltonian generally reads
ˆ
H=X
r,r0Λ
s,s0I
Hrs,r0s0ˆc
rsˆcr0s0,(1)
where His a |Λ||I|×|Λ||I|Hermitian matrix. We assume the
hopping amplitudes follow a power-law decay. This means
for any |I| × |I|block [Hrr0]ss0Hrs,r0s0, or equivalently
Hrr0PrHPr0with Prbeing the projector onto site r, there
exist two positive O(1) constants [45]Jand αsuch that its
operator norm satisfies
kHrr0k ≤ J
(|rr0|+ 1)α,(2)
where |rr0|is the distance between rand r0. We call such a
long-range system satisfying Eq. (2)α-decaying to highlight
the explicit exponent.
Two comments are in order. First, given a fixed α, one can
equivalently replace |rr0|+ 1 by |rr0|in Eq. (2) with
arXiv:2210.05389v2 [quant-ph] 2 Dec 2022
2
Rr
CR
R0
CR0
r0
(1)
1
FIG. 1. Coarse-graining of a square lattice Λ(grey circles) into ˜
Λ
(red circles) with a rescaling χ. Here CRdenotes all the sites in
Λ, including r, that are coarse-grained into R˜
Λ. The coarse-
grained projector is thus defined as PRPrCRPr. Note that no
periodicity of the Hamiltonian is assumed.
r6=r0specified. While both are commonly used conventions,
we prefer Eq. (2) as we need not exclude r=r0. Second,
one can check that α > d is necessary and sufficient for any
α-decaying Hamiltonian to have bounded single particle ener-
gies, i.e., kHk<, so that the total energy is extensive. Our
results are mostly obtained in this thermodynamically stable
regime [19].
Lieb-Robinson bound.—For free fermions it suffices to con-
sider individual single particles. Our first main result concerns
how fast an initially localized particle propagates under the
time evolution governed by ˆ
H:
Theorem 1 (Lieb-Robinson bound) For any α-decaying
Hamiltonian Hwith α > d, there exists an O(1) constant tc
depending only on αand dsuch that for any t>tc
kPreiHtPr0k ≤ K(t)
(|rr0|+ 1)α,(3)
where K(t)grows polynomially fast in time and K(t)
tα(α+1)/(αd)for large t.
Equation (3) essentially gives an upper bound on the wave-
function amplitude on site rat time tof a single-particle state
initially localized at r0. It thus constrains the spreading of
wave function in this “continuous-time quantum walk” setting
[46].
This bound (3) appears to be rather similar to the bound
in Ref. [12] for interacting long-range systems, but a cru-
cial difference here is that in our (free) case it holds for
the whole α > d regime while the interacting case requires
α > 2d, as we will explain for the derivation in the next
paragraph. As is also the case in Ref. [12], the time scal-
ing of K(t)in Eq. (3) is far from optimal. Indeed, the light
cone t∝ |rr0|(αd)/(α+1) is linear only in the short-
range limit α→ ∞, while optimally it would be linear al-
ready for α > d + 1 [18]. On the other hand, the spatial
tail of Eq. (3) is optimal. To see this, we only have to con-
sider ˆ
H=J/(|rr0|+ 1)α(ˆc
rˆcr0+ H.c.). Then we have
kPreiHtPr0k ≥ 2t/[π(|rr0|+ 1)α]at large distance, i.e.
π(|rr0|+ 1)α/(2J)> t. It is also worthwhile to compare
this bound (3) to the free-fermion bound in Ref. [18], which
is optimal in the light cone but not in the tail.
Let us outline the proof of Theorem 1. It is instructive
to first recall that a direct Taylor expansion of eiHt gives
a bound like Eq. (3) but with K(t)eλt [6]. To tighten
this exponential dependence, the basic idea is to separate the
Hamiltonian into the short-range and long-range parts, i.e.,
H=Hsr +Hlr, where the short-range part is determined
[Hsr]rs,r0s0=Hrs,r0s0for |rr0| ≤ χ(χ: cutoff parame-
ter) but otherwise [Hsr]rs,r0s0= 0. We can then work in the
interaction picture with respect to the former:
eiHt =eiHsrtTeiRt
0dt0H(I)
lr (t0),(4)
where Tdenotes the time ordering and H(I)
lr (t) =
eiHsrtHlreiHsr t. By Taylor expansion in the interaction pic-
ture, we can also obtain an exponential factor but with a mod-
ified coefficient λχ, which can be made sufficiently small by
properly choosing χ. While so far the procedure largely fol-
lows Ref. [12], a crucial difference here is that we further per-
form a coarse graining of the lattice Λinto ˜
Λat the same
scale χ(see Fig. 1). This helps us get rid of a factor χdin
λχcompared to the interacting case, making it proportional to
χ(αd)rather than χ(α2d). Therefore, α > d is enough
for suppressing λχtby choosing a sufficiently large χ.
To further illustrate how and why the coarse graining
works, we first write down the Taylor-expansion bound on the
left-hand side of Eq. (3) in the interaction picture (4) [47]:
kPreiHtPr0k ≤
X
n=0 Zt
0
dtnZtn
0
dtn1···Zt2
0
dt1
×
PreiHsr(ttn)
Yn
m=1HlreiHsr (tmtm1)Pr0
,
(5)
where t00. Instead of inserting 1=PrΛPr(1: identity)
as is essentially the strategy used in Ref. [12], we insert the
coarse-grained decomposition 1=PR˜
ΛPR(see Fig. 1) so
that each integrand in Eq. (5) can be upper bounded by
X
{Rj˜
Λ}2n
j=1
kPReiHsr(ttn)PR2nk
n
Y
m=1 kPR2mHlrPR2m1kkPR2m1eiHsr (tmtm1)PR2m2k,(6)
3
where R0R0and R,R0are determined such that
they include r,r0respectively. Obviously, except for the
two boundary factors, the bulk product is always smaller
than the refined decomposition (to each lattice site). In
fact it turns out to be smaller by a factor χnd which
leads to the qualitative improvement of λχdiscussed above.
This is because each kPR2mHlrPR2m1kis roughly smaller
than the corresponding sum of kPr2mHlrPr2m1kby a fac-
tor χd(rmΛis a site coarse-grained into Rm
˜
Λ), while kPR2m1eiHsr(tmtm1)PR2m2kdiffers from
kPr2m1eiHsr(tmtm1)Pr2m2kby mostly an O(1) factor
[44]. Note that in the interacting case this improvement is
canceled by a factor of χdfrom (the interacting counterpart
of) each kPR2m1eiHsr(tmtm1)PR2m2k, accounting for
the size of support of PR. It is the single-particle nature of
free systems that allows us not to “pay the price”.
Clustering properties.—We move on to introduce the sec-
ond main result — the clustering property of the Green’s func-
tion (or resolvent [48])
G(z)(zH)1.(7)
We assume zis outside the spectrum of Hand we define
∆(z)≡ kG(z)k1as the distance of zto such spectrum. Pre-
cisely speaking, we have:
Theorem 2 (Clustering property of the Green’s function)
For an α-decaying Hamiltonian Hwith α > d and zCthat
is not an eigenvalue of H, the Green’s function (7)satisfies
kGrr0(z)k ≤ poly(log(|rr0|+ 1))
(|rr0|+ 1)α,(8)
where Grr0(z) = PrG(z)Pr0and poly(·)means a polyno-
mially large function with |rr0|-independent coefficients,
which nevertheless depend on ∆(z)and diverge for ∆(z)
0.
Here the condition ∆(z)6= 0 is absolutely necessary since
otherwise even short-range hopping (α→ ∞) can generate
long-range correlations and interactions, manifesting as, for
instance, Friedel oscillations [49] and RKKY interactions [50]
in the presence of impurities. The short-range counterpart of
Theorem 2has been considered in Ref. [51].
A direct corollary of Theorem 2is the clustering prop-
erty of ground-state correlation functions. In the case of free
fermions, it is natural to consider the covariance matrix:
Crs,r0s0≡ hΨ0|ˆc
r0s0ˆcrs|Ψ0i,(9)
where |Ψ0iis the ground state of ˆ
H. Without loss of gener-
ality, we may assume the Fermi energy, which lies in a band
gap, to be zero, so that [52,53]
2C=1sgnH. (10)
Thanks to Wick’s theorem, any correlation functions can be
obtained from the covariance matrix (9), so it suffices to con-
sider the clustering properties for the latter, i.e., a bound on
kCrr0kwith Crr0PrCPr0. Note that
C=I`<
dz
2πi G(z),(11)
where `<is a closed loop that encompasses all the bands on
the negative real axis, i.e., below the Fermi energy. Since the
length of `<is bounded by a constant (due to the finiteness
of kHk) while kGrr0(z)ksatisfies Eq. (8)z`<, we know
that kCrr0kalso satisfies Eq. (8). Moreover, Theorem 2has
broader implications. For example, it implies that any bound
state outside the spectrum induced by an impurity supported
on O(1) sites has an algebraically decaying profile in real
space, with essentially the same exponent α. This can be seen
from ψb=G(Eb)Vψb, where ψbis the wave function of the
bound state with eigenenergy Eband Vis the impurity poten-
tial [54]. We will again exploit Theorem 2when discussing
topological phases in the next section.
Finally, let us sketch out the proof of Theorem 2[44]. Sim-
ilar to Refs. [5,6,18,55,56] concerning ground-state corre-
lations, the main idea is to construct an analytic filter function
fσ(t)such that it decays rapidly for large tand its Fourier
transform F[fσ](ω)R
−∞
dt
2πfσ(t)eiωt (also analytic) well
approximates (zω)1if ωis away from zby a few σs,
a control parameter to be determined later. Via Eq. (7) and
up to some error terms involving σ, such a filter enables us to
express Grr0(z)as
PrF[fσ](H)Pr0=Z
−∞
dt
2πfσ(t)PreiHtPr0,(12)
which can be bounded by the Lieb-Robinson bound (3) (and
the trivial bound kPreiHtPr0k ≤ 1for late times). The
desired bound (8) is obtained by choosing an appropriate
σ, which turns out to be proportional to ∆(z)and sub-
logarithmically suppressed by |rr0|.
Topological phases.—Free-fermion topological phases are
defined in terms of equivalence classes under continuous de-
formations of gapped quadratic Hamiltonians or alternatively
of free-fermion (Gaussian) states. In the short-range case
these two approaches can be readily seen to be equivalent [57].
In the long-range case, given an α-decaying free-fermion
state, it is easy to construct a parent Hamiltonian that is also
α-decaying by taking H=12C(cf. Eq. (10)). It follows
that a continuous deformation of a state implies that of the
parent Hamiltonian.
According to the clustering properties proven above, we
know that the converse is also true if α > d. Given
a continuous path of gapped α-decaying Hamiltonians Hλ
parametrized by λ[0,1], their ground states will also be
(almost) α-decaying due to the clustering property of ground-
state correlations. It can be further shown that they define a
continuous path in the space of states by using the clustering
property of the Green’s function. Indeed, we have
Cλ0Cλ=I`<
dz
2πi Gλ(z)(Hλ0Hλ)Gλ0(z),(13)
4
where `<encircles the lower bands of both Hλand Hλ0,
which is always possible given a minimal gap during the de-
formation. Due to Theorem 2, we have that kGλ(z)k ≤
maxrPr0kGλ, rr0(z)kis bounded along `<, implying that
Cλdepends continuously on Hλ.
This analysis justifies the equivalence of considering free-
fermion states and gapped quadratic Hamiltonians for α > d.
In this case we can also say something more about the struc-
ture of existing phases. One can show that every long-range
gapped Hamiltonian with α > d is continuously connected
to a short-range one, implying that there are no new phases
unique to long-range Hamiltonians. To see this, consider the
Hamiltonians defined by Hκ,rr0=eκ|rr0|Hrr0which
constitute a continuous path with respect to κand can be
shown to be gapped for sufficiently small but finite κ[44].
This path connects the long-range Hamiltonian at κ= 0 to a
short-range one (i.e., exponentially decaying) at finite κ.
Furthermore, there should be no unification of short-range
phases in the regime α > d, since for translation-invariant sys-
tems the Bloch Hamiltonians h(k)remain continuous in kand
all the short-range topological invariants remain well-defined
and robust under continuous deformations of the Hamiltonian.
For disordered systems, the index theorem of Ref. [58] shows
that topological invariants must remain equal to a fixed inte-
ger along any path Hλprovided that Cchanges continuously
with respect to H, which we have shown above to be true.
Remarkably, the threshold α=dabove which the short-
range paradigm persists is optimal, i.e., cannot be improved
to be smaller. This is because if we allow α < d then all
the short-range topological phases are expected to be unified
(up to a 0D topological invariant such as the fermion number
parity). Without loss of generality, we focus on translation-
invariant representatives described by Bloch Hamiltonians.
The argument is based on the well known result that all the
short-range topological phases can be obtained by perturbing
a Dirac Hamiltonian with a mass term [31]
h(k) =
d
X
µ=1
sin kµΓµ d
X
µ=1
cos kµm!Γ0,(14)
where {Γµ}µ=0,...,d are Hermitian Dirac matrices satisfying
{Γµ,Γν}= 2δµν . Decreasing mfrom m > d to m
(d2, d), there is a single band crossing at k=0, giving rise
to a transition from a trivial phase to a topological phase with
unit topological number [59]. Let us take, for instance, the
topological Bloch Hamiltonian hTopo(k)defined by choosing
m=d1. We can show that hTopo(k)is connected to the
trivial Hamiltonian h0(k) = Γ0through a continuous path of
long-range gapped Hamiltonians, provided that αis not con-
strained to be larger than d. To this end, we consider a linear
interpolation from h0(k)to hfD(k)and then from hfD(k)to
hTopo(k), where hfD(k)is the flattened Dirac Hamiltonian
hfD(k) =
d
X
µ=1
sin kµ
qPd
µ=1 sin2kµ
Γµ.(15)
FIG. 2. Decay rates of kCrr0kfor the ground states of the Hamil-
tonians hλdefined by hλ= (1 2λ)h0+ 2λhfD for λ[0,0.5]
and hλ= 2(1 λ)hfD + (2λ1)hTopo for λ[0.5,1] in di-
mensions d= 1,2,3. The red dashed lines are a fit of the long
distance behavior of the data with kCrr0k ∝ |rr0|d, implying
the ill-definedness of conventional topological numbers. The numer-
ical calculations are performed on finite hypercubic lattices of side
L= 500 with anti-periodic boundary conditions [60]. In all cases
the odd sites along the x-axis are plotted, as this is the subset of sites
in the lattice that shows the slowest decay.
One can see that h(k)2>0during the whole deformation,
meaning that the gap does not close. Furthermore hfD(k)
is (almost) d-decaying in real space [44], while h0(k)and
hTopo(k)are local, so the Hamiltonian is at most as nonlo-
cal as d-decaying during the deformation. Numerical analysis
suggests that also the ground state covariance matrix Cre-
mains always d-decaying along such path, as shown in Fig. 2.
Summary and outlook.—We have derived a tight (in the
sense of spatial tail) Lieb-Robinson bound for α-decaying
free-fermion systems with α > d. This bound allows
us to prove an (almost) optimal clustering property for the
Green’s function, which implies the clustering property for
the ground-state correlations in gapped systems. These results
justify the equivalence between state and Hamiltonian-based
definitions of topological phases in long-range free-fermion
systems. In addition, we argue that all the short-range topo-
logical phases are connected within the space of α-decaying
systems with α < d.
A relevant open problem is how to further improve the
Lieb-Robinson bound to be consistent with the optimal light
cone [18]. Also, one still has to examine the validity of bulk-
edge correspondence [61] and prove the clustering properties
for topological edge modes localized at sharp edges, where
our local-impurity argument does not apply. Improving the
摘要:

Long-RangeFreeFermions:Lieb-RobinsonBound,ClusteringProperties,andTopologicalPhasesZongpingGong,1,2TommasoGuaita,1,2,3andJ.IgnacioCirac1,21Max-Planck-Institutf¨urQuantenoptik,Hans-Kopfermann-Straße1,D-85748Garching,Germany2MunichCenterforQuantumScienceandTechnology,Schellingstraße4,80799M¨unchen,Ger...

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