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首页二维超对称理论中的A-扭曲关联函数与霍里对偶
扭曲的相关器和Hori对偶是基于N=(2,2)超对称性的一系列关键概念,它们在二维量子场论中占据重要地位。这些对偶关系与四维Seiberg对偶相类似,展示了在不同理论之间存在的深刻联系。具体来说,研究集中在U(Nc)、USp(2Nc)、SO(N)和O(N)等规范群的理论上,这些对偶关系通过分析Riemann曲面Σg上的库仑分支算子的关联函数得以验证。 在Hori-Tong对偶的研究中,引入了A-扭曲,这是一种拓扑性质,它改变了量子场论的边界条件。这种扭曲对于理解理论在非平凡空间中的行为至关重要。通过A-扭曲,理论的对称性以及物理量的计算方式会发生改变,从而揭示了理论在红外区域的不同表现形式。 O(N)理论,这里被分为O+(N)和O_(N)两种形式,可以看作是SO(N)理论的ℤ2(二元群)倍性扩展。在具有非零曲率的Riemann曲面Σg(即g>0)上,这些理论的关联因子不是通过传统的自由场理论计算得出,而是通过对带有A-扭曲的边界条件进行计算,并通过双投影确定的权重求和得到的。 Cyril Closset、Noppadol Mekareeya和Daniel S. Park三位作者在2017年的JHEP08期刊上发表了他们的研究成果,这篇论文不仅深化了对二维超对称理论的理解,也为理论物理学家提供了一个新的工具来探索更深层次的对称性和物理现象。他们的工作不仅有助于理论的发展,也为未来的研究提供了新的视角,特别是在量子场论的对称性变换和空间拓扑效应的研究领域。
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JHEP08(2017)101
2.3 Handle-gluing operator and flux operator
The A-twisted theory is a topological field theory [29], whose local observables are fully
determined by the topological action:
S
TFT
=
Z
Σ
g
d
2
x
√
g
−2f
1
¯
1
a
∂W
∂σ
a
+
e
Λ
a
¯
1
Λ
b
1
∂
2
W
∂σ
a
∂σ
b
− 2F
1
¯
1
(F )
∂W
∂m
F
+
i
2
ΩR
, (2.24)
which is given in terms of W and Ω. Here f
a
= da
a
and F
(F )
= dA
(F )
. We refer to [34]
for a more thorough discussion.
As in any topological field theory, there exists a local operator H, the handle-gluing
operator, whose insertion corresponds to “adding a handle” to the Riemann surface:
hOHi
g
= hOi
g+1
. (2.25)
For A-twisted N = (2, 2) gauge theories, H was first computed explicitly in [31] — see
also [17, 32, 33]. It is given by:
H(σ) = exp (2πiΩ(σ)) H(σ) , (2.26)
where Ω is the effective dilaton (2.22) and H is the Hessian determinant (2.13). This latter
contribution comes from the gaugino zero-modes in the twisted theory, which couple to W
as indicated in the second term in (2.24). It is clear from (2.24) that H corresponds to a
local operator insertion one obtains by concentrating the curvature of a single handle at a
point, with a δ-function singularity.
Similarly, there exists local operators whose insertion changes the background fluxes
for the flavor symmetries. These so-called “flux operators” [34] are simply given by:
Π
F
= exp
2πi
∂W
∂m
F
, (2.27)
in term of the effective twisted superpotential W = W(σ, m
F
).
We should also note that the coupling of the GLSM to curved space introduces a
“gravitational” anomaly for the axial R-symmetry U(1)
ax
[14, 15], with coefficient:
ˆc
grav
= −dim(g) −
X
i
(r
i
− 1)dim(R
i
) . (2.28)
This corresponds to the U(1)
ax
−U(1)
R
‘t Hooft anomaly:
b
R
0
= −ˆc
grav
. (2.29)
This anomaly is reproduced by the handle-gluing operator, since
H → e
−2iαb
R
0
H (2.30)
under a U(1)
ax
rotation, corresponding to an anomalous shift of θ
R
. When b
I
0
= 0 and if
the theory flows to a conformal fixed point, c = 3 ˆc
grav
is the central charge of the infrared
SCFT [1].
– 8 –
JHEP08(2017)101
2.4 Correlation functions as sums over Bethe vacua
Let O = O(σ) be a gauge-invariant polynomial in σ. On the Coulomb branch, this corre-
sponds to a Weyl-invariant polynomial,
O(σ) ∈ C[σ
a
]
W
G
. (2.31)
The correlation functions of these Coulomb branch operators on Σ
g
(with background flux
n
F
) are given explicitly by the formula [17, 31–33]:
hO(σ)i
g; n
F
=
X
ˆσ∈S
BE
O(ˆσ) H(ˆσ)
g−1
Y
F
Π
F
(ˆσ)
n
F
. (2.32)
The sum is over all the distinct solutions (σ
a
) = (ˆσ
a
) to the Bethe equations (2.12). Let
us note a few simple properties of (2.32):
• It makes the quantum ring relations manifest. The twisted chiral ring relations are
the relations f (ˆσ) = 0 satisfied by any solution to the Bethe equations, and therefore
the insertion of any such relation in the correlation function gives a vanishing result:
hf(σ)O(σ)i
g; n
F
= 0 . (2.33)
• We easily check that the mixing (2.16) of the U(1)
R
symmetry with a flavor symmetry
corresponds to (2.17), as expected. This amounts to a shift of the dilaton effective
action by:
Ω → Ω + t
∂W
∂m
F
. (2.34)
• Similarly, the mixing of the R-symmetry with a gauge symmetry U(1)
I
does not
change the answer, as expected from gauge invariance. A mixing with the gauge
symmetry corresponds to:
Ω → Ω + t
∂W
∂σ
I
, (2.35)
but this does not affect H(ˆσ), the handle-gluing operator evaluated on any Bethe vac-
cum.
2.5 Correlation functions as sums over instantons
It is often interesting to write down the correlation functions in terms of an infinite sum
over instanton contributions [15] — two-dimensional vortices — in the GLSM:
hO(σ)i
g; n
F
=
1
|W
G
|
X
m∈Γ
G
∨
q
m
Z
g,n
F
,m
(O) . (2.36)
Here the weight factor q
m
are the FI parameters (2.5), the sum is over all GNO-quantized
fluxes for G, and |W
G
| is the order of the Weyl group. If the free center of G (2.3) is non-
trivial, the sum (2.36) typically converges for some values of q
I
, and can be defined more
generally by analytic continuation. However, even if G does not contain any U(1) factor,
– 9 –
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