
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-ℓsymmetric traceless representations, i.e.,
spin-ℓrepresentations. So all (primary and descendant)
operators have two quantum numbers (∆, ℓ). A primary
operator Owith quantum number ℓ= 0 is called a scalar
operator, and any of its descendants can be written as
∂ν1···∂νj□nO, 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-ℓprimary operator Oµ1···µℓare a bit more compli-
cated as there are two different types. The first type can
be written as,
∂ν1···∂νj∂µ1···∂µi□nOµ1···µℓ,(2)
with quantum number (∆ + 2n+j+i, ℓ +j−i) for
ℓ≥i≥0, 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 ∂ρ∂ν1···∂νj∂µ1···∂µi□nOµ1···µℓ,(3)
with quantum number (∆ + 2n+j+i+ 1, ℓ +j−i) for
ℓ−1≥i≥0, n, j ≥0. We note that the εtensor alters
spacetime parity symmetry of Oµ1···µℓ.
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 d−1 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 d−1-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 Sd−1×R,
as shown in the left hand side of Fig. 1. In the radial
quantization, the SO(d) Lorentz rotation acts on the
Sd−1sphere, while the dilatation acts as the scaling of
sphere radius. Therefore, the states defined on the folia-
tion Sd−1have 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 Md−1×Rmanifold:
Ris the time direction, while Md−1is a d−1-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 Sd−1×Rusing a Weyl transformation [7,14],
as shown in Fig. 1. Under the Weyl transformation the
dilatation r→eλrof Rdbecomes the translation along
the time direction τ→τ+λof Sd−1×R. If the theory
has conformal symmetry, we can simply relate correlators
and states on Rdto those on Sd−1×R. Moreover, we still
have the state-operator correspondence on the cylinder
Sd−1×R. In particular, the state-operator correspon-
dence on the cylinder has a nice physical interpretation,
namely the eigenstates |ψn⟩of the CFT quantum Hamil-
tonian on Sd−1are 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=En−E0=v
R∆n,(4)
where Ris the radius of sphere Sd−1and 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.