Uncovering conformal symmetry in the 3DIsing transition State-operator correspondence from a fuzzy sphere regularization Wei Zhu1Chao Han2Emilie Huffman3Johannes S. Hofmann4and Yin-Chen He3

2025-05-06 0 0 2.38MB 18 页 10玖币
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Uncovering conformal symmetry in the 3DIsing transition:
State-operator correspondence from a fuzzy sphere regularization
Wei Zhu,1, Chao Han,2Emilie Huffman,3Johannes S. Hofmann,4and Yin-Chen He3,
1School of Science, Westlake University, Hangzhou, 310030, China
2Westlake Institute of Advanced Study, Westlake University, Hangzhou, 310024, China
3Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada
4Department of Condensed Matter Physics, Weizmann Institute of Science, Rehovot, 76100, Israel
The 3DIsing transition, the most celebrated and unsolved critical phenomenon in nature, has
long been conjectured to have emergent conformal symmetry, similar to the case of the 2DIsing
transition. Yet, the emergence of conformal invariance in the 3DIsing transition has rarely been
explored directly, mainly due to unavoidable mathematical or conceptual obstructions. Here, we
design an innovative way to study the quantum version of the 3DIsing phase transition on spherical
geometry, using the “fuzzy (non-commutative) sphere” regularization. We accurately calculate
and analyze the energy spectra at the transition, and explicitly demonstrate the state-operator
correspondence (i.e. radial quantization), a fingerprint of conformal field theory. In particular, we
have identified 13 parity-even primary operators within a high accuracy and 2 parity-odd operators
that were not known before. Our result directly elucidates the emergent conformal symmetry of
the 3DIsing transition, a conjecture made by Polyakov half a century ago. More importantly,
our approach opens a new avenue for studying 3DCFTs by making use of the state-operator
correspondence and spherical geometry.
I. INTRODUCTION
Symmetry is one of the most important organizing
principles in physics. As is well known, symmetries
present microscopically (e.g. condensed matter systems,
ultraviolet (UV) Lagrangians) can be spontaneously bro-
ken at low energies, giving rise to various distinct phases
of matter such as crystals and magnets. Conversely and
rather unexpectedly, symmetries absent microscopically
can emerge at low energies, and such a phenomenon is
called emergent symmetry. One prominent example is
the order-disorder phase transition of 2DIsing model, for
which Polyakov discovered emergent conformal symme-
try in 1970 [1], 26 years after Onsager’s exact solution [2].
Polyakov’s remarkable discovery of emergent confor-
mal symmetry in the 2DIsing transition gave birth to
conformal field theory (CFT) [3], a class of quantum
field theories with profound applications in various fields
of physics including statistical mechanics, quantum con-
densed matter, string theory and quantum gravity. In
statistical physics, it is a common belief that many uni-
versality classes of (classical and quantum) phase transi-
tions are captured by CFTs, however this has not been
proven for 3Dtransitions. 1The emergence of conformal
symmetry at phase transitions is not only aesthetically
beautiful, but also useful in understanding the properties
of these transitions, such as computing experimentally
measurable critical exponents. In 2Dthe (local) confor-
mal symmetry has an infinite-dimensional algebra, and it
zhuwei@westlake.edu.cn
yhe@perimeterinstitute.ca
1For phase transitions in 2D[4] and 4D[5] the combination of
scale symmetry, Lorentz symmetry and unitarity was shown to
lead to conformal symmetry.
makes many 2DCFTs exactly solvable [3,6]. In d > 2 di-
mensions, there is only a finite-dimensional (global) con-
formal symmetry, i.e. SO(d+ 1,1), with which one is
not able to analytically solve CFTs as in 2D. There-
fore, CFTs beyond 2Dare rather poorly understood,
with their solutions remaining outstanding for decades
despite their broad appeal to physics and mathematics.
Historically, the study of lattice models for 2Dclassi-
cal phase transitions and their quantum cousins (1 + 1D
quantum phase transitions) played a key role in the dis-
covery and understanding of 2DCFTs [1,2,7]. Sim-
ilar progress in the study of conformal symmetry for
d3 dimensional theories, however, has stalled due to
the natural limitation of the lattice formulation. There
are a plenty of papers studying 3Dphase transitions on
the lattice, e.g. computing critical exponents. How-
ever, the perspective of conformal symmetry has rarely
been explored [813]. The conformal symmetry of a
ddimensional CFT is most transparent in geometries
such as Rd,Sdas well as Sd1×R. In particular, CFTs on
Sd1×Robey a property called state-operator correspon-
dence (i.e. radial quantization), which is a direct con-
sequence of conformal symmetry [7]. Specifically, for a
quantum Hamiltonian defined on sphere Sd1, its eigen-
states are in one-to-one correspondence with the scaling
operators (including primary and descendant operators)
of the infrared (IR) CFT. Moreover, the energy gaps of
these eigenstates are proportional to the scaling dimen-
sions of their corresponding scaling operators [14]. This
nice feature can be used to explore various properties of
CFTs, including scaling dimensions of operators, oper-
ator product expansion coefficients, and even operator
algebras [7]. For 2DCFTs, S1×Ris very natural as one
just needs to study a 1 + 1Dquantum lattice model de-
fined on a 1Dperiodic chain (i.e. S1) [1518]. However,
simulating lattice models of d3 dimensional CFTs on
arXiv:2210.13482v3 [cond-mat.stat-mech] 30 Oct 2023
2
Sd1×Rwill be problematic, because a regular lattice
cannot be put on a sphere Sd12due to its nontrivial
curvature. 2While efforts have nevertheless been made
to discretize the sphere, no signature of state-operator
correspondence has been found so far [19,20].
To overcome this geometric obstacle, in this paper we
are pursuing a different direction, namely we fuzzify a
sphere [21]. Specifically, we study a 2 + 1Dquantum
Ising transition defined on a fuzzy (non-commutative)
sphere in light of Landau level regularization [22]. As a
result of this innovative discretization, we have observed
almost perfect state-operator correspondence in surpris-
ingly small system sizes. We use exact diagonalization to
calculate properties of the 2+1DIsing transition for up to
16 effective spins, and we have found its low lying eigen-
states (up to 70 lowest states) split into representations of
the 3Dconformal symmetry (i.e. conformal multiplets),
hence directly demonstrating the emergence of confor-
mal symmetry. Among these low energy states, we have
found 15 conformal primary states, most of which have
not been discovered in any previous model studies of the
3D Ising transition. Specifically, we have found 13 parity-
even primaries, whose scaling dimensions agree well with
state-of-the-art conformal bootstrap results [23,24] with
discrepencies smaller than 1.6%. We have also identified
two parity-odd primaries which were unknown before.
Our observations directly verify conformal symmetry
for the 3DIsing transition, which was conjectured by
Polyakov 50 years ago [1]. Before our results, the most
compelling evidence for the 3DIsing transition being
conformal was from numerical conformal bootstrap [23
27], which assumes conformal symmetry and found crit-
ical exponents close to the values obtained by various
methods such as Monte Carlo simulation [28,29] and
measured by experiments [30]. In addition, there was
an effort [13] to justify the conformal invariance of the
3DIsing by showing that the virial current operator
does not exist. 3Our obtained operator spectrum from
the state-operator correspondence indeed convincingly
shows that the 3DIsing transition does not have the
virial current, which is a structural explanation of the
3DIsing being conformal [32]. A major surprise of our
results is that an incredibly small system size (8 16 to-
tal spins) is already enough to yield accurate conformal
data of the 3DIsing CFT. So we expect this approach
to open a new avenue for studying higher dimensional
phase transitions and CFTs. Firstly, there is a zoo of
universalities that can be studied using our approach,
which is amenable to various numerical techniques such
as exact diagnolization (ED), density-matrix renormal-
ization group (DMRG) and determinantal Monte Carlo.
2In mathematics the problem of tiling a sphere is called spherical
tiling or spherical polyhedron.
3We note that Ref. [31] claimed a proof of the conformal invariance
of 3DIsing transition, but it is unclear if the proof is correct (see
the comment in Appendix B in the first arXiv version of Ref.[13]).
This offers an opportunity to tackle many open questions
regarding phase transitions, critical phases and CFTs.
Secondly, a number of new universal quantities can be
computed once the 3DCFT is simulated on a sphere,
such as operator product expansion coefficients, F(of F-
theorem) [3336], and the spherical binder ratio [37], just
to name a few.
The paper is organized as follows. In Sec. II A we
will review background knowledge including the radial
quantization of CFTs and the state-operator correspon-
dence. The spherical Landau level quantization and re-
lated fuzzy sphere are discussed in Sec. II B. Readers
familiar with these topics can skip some of these subsec-
tions. In Sec. III, we formulate spherical Landau levels
to regularize the 3DIsing transition on a fuzzy sphere.
A global quantum phase diagram is presented. In Sec.
IV, we present the low-lying energy spectra at the phase
transition point, and analyze their one-to-one correspon-
dence with the scaling operators as predicted by the Ising
CFT. This is the main result of this paper. At last, we
present a discussion and outlook in Sec. V.
II. REVIEW OF BACKGROUND
A. Radial quantization of CFTs: state-operator
correspondence
In this subsection we review some basics of radial quan-
tization, and for an elaborated discussion we refer the
readers to CFT lecture notes such as those in [6,38].
The conformal group in ddimensions SO(d+ 1,1) is
generated by d-dimensional translations Pµ=i∂µ,d-
dimensional Lorentz rotations Mµν =i(xµνxνµ),
dilatations D=ixµµ, and special conformal transfor-
mations Kµ=i(2xµ(xνν)x2µ). From the operator
point of view, a CFT can be thought of as a theory whose
operators form an infinite-dimensional representation of
the conformal group. Specifically, one can write CFT
operators {ˆ
Oα}as eigen-operators (i.e. irreducible repre-
r
τ
Sd1
Sd1
Weyl transformation
τ= log r
FIG. 1. Through a Weyl transformation, Euclidean flat space-
time Rdis mapped to the manifold of cylinder Sd1×R. As
a result, a CFT on Rdquantized on equal radius slices can be
described equivalently in terms of a CFT on Sd1×Rquan-
tized on equal time slices. The states defined on the Sd1×R
have well-defined quantum numbers of SO(d) Lorentz rota-
tion and dilatation, and thus they are in one-to-one correspon-
dence with operators of the CFT, dubbed as state-operator
correspondence.
3
sentations) of the dilatation and Lorentz rotation SO(d).
In particular, the eigenvalue ∆ of dilatation is called scal-
ing dimension of the operator, and it corresponds to the
exponent in the power law correlation function of the
operator, e.g. O(x)O(0)⟩ ∼ 1/|x|2∆. One can further
categorize operators into primary operators and descen-
dant operators: 1) primary operators are operators that
are annihilated by the special conformal transformation
Kµ; 2) descendant operators are not annihilated by Kµ,
and all of them can be obtained by applying translations
Pµ(multiple times) to the primary operators. There-
fore, one can organize CFT operators as primary oper-
ators and their descendants, and each primary and its
descendants form a set of operators called a conformal
multiplet. 4A CFT has an infinite number of primary
operators, which makes it hard to tackle theoretically. A
major task of solving a CFT is thus to obtain its low
lying (if not full) spectrum of primary operators.
To facilitate later analysis of our numerical results, we
will elaborate a bit more about the operator contents of
a 3DCFT. In 3Dthe Lorentz rotation group is the fa-
miliar SO(3) group, all the irreducible representations of
which are rank-symmetric traceless representations, i.e.,
spin-representations. So all (primary and descendant)
operators have two quantum numbers (∆, ℓ). A primary
operator Owith quantum number = 0 is called a scalar
operator, and any of its descendants can be written as
ν1···νjnO, n, j 0,(1)
with quantum number (∆ + 2n+j, j). We note =2.
Here and hereafter all the free indices shall be sym-
metrized with the trace subtracted. The descendants of
a spin-primary operator Oµ1···µare a bit more compli-
cated as there are two different types. The first type can
be written as,
ν1···νjµ1···µinOµ1···µ,(2)
with quantum number (∆ + 2n+j+i, ℓ +ji) for
i0, n, j 0. Here and hereafter the repeated
indices shall be contracted. The other type will involve
the εtensor of SO(3), and can be written as,
εµlρτ ρν1···νjµ1···µinOµ1···µ,(3)
with quantum number (∆ + 2n+j+i+ 1, ℓ +ji) for
1i0, n, j 0. We note that the εtensor alters
spacetime parity symmetry of Oµ1···µ.
We also remark that conserved operators (i.e. global
symmetry current Jµand energy momentum tensor Tµν )
should be treated a bit differently, because they satisfy
the conservation equations µJµ= 0 and µTµν = 0.
4Here we are talking about primary operators under the global
conformal symmetry SO(d+ 1,1). For 2DCFTs one usually
talks about primary operators under Virasoro symmetries, and
the global conformal primaries are called quasi-primaries.
Therefore, their descendants in Eq. (2) and (3) should
have i= 0. 5
Now we turn to the state perspective of CFTs. To de-
fine states of a CFT, we first need to quantize it, or in
other words find a Hilbert space construction of it. A
quantum phase transition, namely a quantum Hamilto-
nian realization of a d-dimensional CFT in d1 space
dimensions, can be viewed as a way to quantize the CFT.
The states of the CFT are nothing but the quantum
Hamiltonian’s eigenstates. Formally, the quantization of
CFTs can be more general than quantum phase transi-
tions. Specifically, one can foliate d-dimensional space-
time into d1-dimensional surfaces, and each leaf of the
foliation is endowed with its own Hilbert space. One con-
venient quantization is radial quantization, which has the
d-dimensional Euclidean space Rdfoliated to Sd1×R,
as shown in the left hand side of Fig. 1. In the radial
quantization, the SO(d) Lorentz rotation acts on the
Sd1sphere, while the dilatation acts as the scaling of
sphere radius. Therefore, the states defined on the folia-
tion Sd1have well-defined quantum numbers of SO(d)
rotation and dilatation, and they are indeed in one-to-
one correspondence with operators of the CFT, dubbed
as state-operator correspondence.
For a quantum Hamiltonian realization, the radial
quantization described above is not natural, and instead
one may want a quantization scheme that has an iden-
tical Hilbert space on each leaf of foliation. A quantum
Hamiltonian is usually defined on the Md1×Rmanifold:
Ris the time direction, while Md1is a d1-dimensional
space manifold (e.g. sphere, torus, etc.), the leaf of folia-
tion, on which the Hilbert space (and the quantum state)
lives. In order to discuss state-operator correspondence
in such a quantization scheme, one needs to map Rdto
the cylinder Sd1×Rusing a Weyl transformation [7,14],
as shown in Fig. 1. Under the Weyl transformation the
dilatation reλrof Rdbecomes the translation along
the time direction ττ+λof Sd1×R. If the theory
has conformal symmetry, we can simply relate correlators
and states on Rdto those on Sd1×R. Moreover, we still
have the state-operator correspondence on the cylinder
Sd1×R. In particular, the state-operator correspon-
dence on the cylinder has a nice physical interpretation,
namely the eigenstates |ψnof the CFT quantum Hamil-
tonian on Sd1are in one-to-one correspondence with
the CFT operators, and the energy gaps δEnof these
states are proportional to the scaling dimensions ∆nof
CFT operators [7,14],
δEn=EnE0=v
Rn,(4)
where Ris the radius of sphere Sd1and vis the velocity
of light that is model dependent. Also the SO(d) rotation
5The conformal multiplet of a conserved operator is called a short
multiplet.
4
symmetry of Sd1is identified with the SO(d) Lorentz
rotation of the conformal group, so the SO(d) quantum
numbers of |ψnare identical to those of CFT operators.
We emphasize that in contrast to radial quantiza-
tion on Rd, conformal symmetry is indispensable for the
state-operator correspondence of radial quantization on
the cylinder Sd1×R. Therefore, observing the state-
operator correspondence on the cylinder Sd1×Rwill be
direct evidence for the conformal symmetry of the theory
or phase transition. For d= 2, the cylinder S1×Rcorre-
sponds to nothing but a quantum Hamiltonian defined on
a periodic chain, and there are very nice results studying
the resulting state-operator correspondence [1518]. In
higher dimensions, one needs to study a quantum Hamil-
tonian defined on Sd1, however, it is highly nontrivial
for a discrete lattice model as Sd12has a curvature.
B. Spherical Landau levels, fuzzy two-sphere and
lowest Landau level projection
As originally shown by Landau, electrons moving in
2Dspace under a magnetic field will form completely
flat bands called Landau levels, which is the key to the
quantum Hall effect. Landau level quantization can be
considered on any orientable manifold, and Haldane [39]
first introduced Landau levels on spherical geometry to
study the fractional quantum Hall physics.
For electrons moving on the surface of a radius-rsphere
with a 4πs monopole (2sZ) placed at the origin (Fig.
2), the Hamiltonian is
H0=1
2Mer2Λ2
µ,(5)
where Meis the electron’s mass and Λµ=µ+iAµis
the covariant angular momentum, Aµis the gauge field
of the monopole. As usual we take =e=c= 1. The
eigenstates will be quantized into spherical Landau levels,
whose energies are En= [n(n+ 1) + (2n+ 1)s]/(2Mer2),
with n= 0,1,2,··· the Landau level index. The (n+1)th
Landau level is (2s+ 2n+ 1)-fold degenerate, and the
single particle states in each Landau level are called Lan-
dau orbitals. Assuming all interactions are much smaller
than the energy gap between Landau levels, we can just
consider the lowest Landau level (LLL) n= 0, which is
2s+ 1-fold degenerate. The wave-functions for each Lan-
dau orbital on LLL are called monopole harmonics [40]
Φm(θ, φ) = Nmeimφ coss+mθ
2sinsmθ
2,(6)
with m=s, s+ 1,··· , s and Nm=q(2s+1)!
4π(s+m)!(sm)! .
Here (θ, φ) is the spherical coordinate.
These LLL Landau orbitals indeed form a SO(3) spin-
sirreducible representation. This can be understood by
constructing the SO(3) angular momentum operator [41],
Lµ= Λµ+sxµ
r,(7)
which satisfies the SO(3) algebra [Lµ, Lν] = µνρLρ.
Projecting the system into the LLL, the kinetic energy
of the covariant angular momentum will be quenched, so
effectively we have Lµs˜xµ/r. (˜xµdenotes the coordi-
nates in the projected LLL.) As a result, the coordinates
˜xµof electrons will not actually commute, instead we
have
[˜xµ,˜xν] = ir
sϵµνρ ˜xρ.(8)
This defines a fuzzy two-sphere [21]. Moreover, Landau
orbitals (6) are in one-to-one correspondence with states
on the fuzzy two-sphere. Formally, a system defined on
the LLL can be equivalently viewed as a system defined
on a fuzzy two-sphere. We will not delve into details
along that direction, and refer the reader to [42] for more
discussions.
As is usually done in the literature, we will consider
the limit where the interaction strength is much smaller
than the Landau level gap, so we can project the system
into the LLL. Technically, this can be done by rewriting
the annihilation operator ψ(θ, φ) on the LLL as
ˆ
ψ(θ, φ) = 1
2s+ 1
s
X
m=s
Φ
mˆcm.(9)
ˆcmstands for the annihilation operator of Landau orbital
m, and is independent of coordinates (θ, φ). The density
operator n(θ, φ) = ψψcan be written as,
n(θ, φ) = 1
2s+ 1 X
m1,m2
Φm1Φ
m2c
m1cm2.(10)
Any interaction can be straightforwardly (though per-
haps tediously) written in the second quantized form
using Landau orbital operators c
m, cm. For example,
the density-density interaction HI=Rd2rad2rbU(ra
rb)n(ra)n(rb) can be written as,
HI= (2s+ 1)2ZdadbU(θa, φa;θb, φb)n(θa, φa)n(θb, φb)
=X
m1,m2,m3,m4
Vm1,m2,m3,m4c
m1c
m2cm3cm4,(11)
where Vm1,m2,m3,m4can be further expanded using the
so-called Haldane pseudopotential Vl[39], corresponding
to the two-fermion scattering in the spin-2slchannel
(see Appendix Sec. A).
In summary, the model we are working with is a fer-
monic Hamiltonian enclosing 2s+1-Landau orbitals with
long-range SO(3) invariant interactions. Interestingly, all
the orbitals form an SO(3) spin-sirrep. Furthermore, the
length scale of the system is 2s+ 1 instead of 2s+ 1
since the spatial dimension is d= 2, and the thermody-
namic limit corresponds to taking sto infinity.
III. MODEL ON A FUZZY-TWO SPHERE
A. Hamiltonian
摘要:

Uncoveringconformalsymmetryinthe3DIsingtransition:State-operatorcorrespondencefromafuzzysphereregularizationWeiZhu,1,∗ChaoHan,2EmilieHuffman,3JohannesS.Hofmann,4andYin-ChenHe3,†1SchoolofScience,WestlakeUniversity,Hangzhou,310030,China2WestlakeInstituteofAdvancedStudy,WestlakeUniversity,Hangzhou,3100...

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