没有合适的资源?快使用搜索试试~ 我知道了~
在这项工作中,我们介绍了五维膨胀引力理论的最小超对称扩展,它捕获了小弦理论全息对偶的主要特性。 它通过沿着SU(2)R对称的U(1)子组的N = 2超重力和与字符串dilaton相关的一个矢量多重性的特定度量来描述。 运动方程第五个坐标解中的线性膨胀(使用平弦框架度量)在四个维度上将超对称的一半分解为N = 1。 在钟表机构的背景下,人们对线性膨胀模型的兴趣最近得到了恢复,钟表机构最近被提出作为场论中指数尺度分离的新来源。
资源推荐
资源详情
资源评论
Eur. Phys. J. C (2018) 78:146
https://doi.org/10.1140/epjc/s10052-018-5632-4
Regular Article - Theoretical Physics
The effective supergravity of little string theory
Ignatios Antoniadis
1,2,a
, Antonio Delgado
3,b
, Chrysoula Markou
1,c
, Stefan Pokorski
4,d
1
Sorbonne Université, CNRS, Laboratoire de Physique Théorique et Hautes Energies, LPTHE, 75005 Paris, France
2
Albert Einstein Center for Fundamental Physics, Institute for Theoretical Physics, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
3
Department of Physics, University of Notre Dame, 225 Nieuwland Hall, Notre Dame, IN 46556, USA
4
Faculty of Physics, Institute of Theoretical Physics, University of Warsaw, ul. Pasteura 5, 02-093 Warsaw, Poland
Received: 17 November 2017 / Accepted: 10 February 2018
© The Author(s) 2018. This article is an open access publication
Abstract In this work we present the minimal supersym-
metric extension of the five-dimensional dilaton-gravity the-
ory that captures the main properties of the holographic dual
of little string theory. It is described by a particular gauging
of N = 2 supergravity coupled with one vector multiplet
associated with the string dilaton, along the U (1) subgroup
of SU(2) R-symmetry. The linear dilaton in the fifth coor-
dinate solution of the equations of motion (with flat string
frame metric) breaks half of the supersymmetries to N = 1
in four dimensions. Interest in the linear dilaton model has
lately been revived in the context of the clockwork mecha-
nism, which has recently been proposed as a new source of
exponential scale separation in field theory.
1 Introduction
Besides its own theoretical interest, little string theory pro-
vides a framework with interesting phenomenological con-
sequences. It offers a way to address the hierarchy when the
string scale is at the TeV scale [1–3], without postulating large
extra dimensions (in string units) but instead an ultra-weak
string coupling [4,5]. Recently, interest in the holographic
dual to LST (the linear dilaton model) has been revived in
the context of the so-called clockwork models [6–8] which
address the exponential scale separation in field theory in a
new way [9,10].
Little string theory (LST) corresponds to a non-trivial
weak coupling limit of string theory in six dimensions with
gravity decoupled and is generated by stacks of (Neveu–
Schwarz) NS5-branes [11]. Its holographic dual corresponds
to a seven-dimensional gravitational background with flat
a
e-mail: antoniad@lpthe.jussieu.fr
b
e-mail: antonio.delgado@nd.edu
c
e-mail: chrysoula@lpthe.jussieu.fr
d
e-mail: Stefan.Pokorski@fuw.edu.pl
string-frame metric and the dilaton linear in the extra dimen-
sion [12]. Its properties can be studied in a simpler toy model
by reducing the theory in five dimensions. Introducing back
gravity weakly coupled, one has to compactify the extra
dimension on an interval and place the Standard Model on
one of the boundaries, in analogy with the Randall–Sundrum
model [13] on a slice of a five-dimensional (5d) anti-de Sitter
bulk [1].
Since we know that the bulk LST geometry preserves
space-time supersymmetry, in this work we study the corre-
sponding effective supergravity which in the minimal case
is N = 2. In principle, there should be a generalisation
with more supersymmetries, or equivalently in higher dimen-
sions. The N = 2 gravity multiplet contains the graviton,
a graviphoton and the gravitino (8 bosonic and 8 fermionic
degrees of freedom), while the heterotic (or type I) string dila-
ton is in a vector multiplet containing a vector, a real scalar
and a fermion. The corresponding supergravity action [15]
admits a gauging of the U(1) subgroup of the SU(2) R-
symmetry, that generates a potential for the single scalar
field [15,16]. This potential depends on two parameters
allowing a multiple of possibilities with critical or non critical
points, or even flat potential with supersymmetry breaking.
Here, we observe that the vanishing of one of the parameters
generates the runaway dilaton potential of the non-critical
string. This potential has no critical point with 5d maximal
symmetry but it leads to the linear dilaton solution in the fifth
coordinate that preserves 4d Poincaré symmetry. We show
that this solution breaks one of the two supersymmetries,
leading to N = 1 in four dimensions.
The outline of the paper is the following. In Sect. 2,we
review the gauged N = 2 supergravity in five dimensions,
based on the references [14–17], and specialize in the case of
one vector multiplet using the results of the string effective
action of Ref. [18]. In Sect. 3, we present the 5d graviton-
dilaton toy model that describes the holographic dual of
123
146 Page 2 of 9 Eur. Phys. J. C (2018) 78:146
LST and identify it with a particular choice of the gaug-
ing of the N = 2 supergravity. We also show that the linear
dilaton solution preserves half of the supersymmetries, i.e.
N = 1 in four dimensions. In Sect. 4, we write the com-
plete Lagrangian, including the fermion terms, depending
on three constant parameters. In Sect. 5, we derive the spec-
trum classified using the 4d Poincaré symmetry and we con-
clude with some phenomenological remarks. Finally, there
are three appendices containing our conventions, the equa-
tions of motion with the linear dilaton solution, and some
explicit calculations that we use in the study of supersym-
metry transformations.
2 Gauged N = 2, D = 5 supergravity
The references used in the following are [14–17], while our
conventions may be found in the Appendix A. In D = 5
spacetime dimensions, the pure N = 2 supergravity multi-
plet contains the graviton e
m
M
, the gravitino SU(2)-doublet
ψ
i
M
, where i is the SU(2) index, and the graviphoton, while
the N = 2 Maxwell multiplet contains a real scalar φ,an
SU(2) fermion doublet λ
i
and a gauge field. Upon coupling
n Maxwell multiplets to pure N = 2, D = 5 supergravity,
the total field content of the coupled theory can be written as
e
m
M
,ψ
i
M
, A
I
M
,λ
ia
,φ
x
, (1)
where I = 0, 1,...,n , a = 1,...,n and x = 1,...,n.
The real scalars φ
x
can be seen as coordinates of an n-
dimensional space M that has metric g
xy
that is symmetric
for our purposes, while the spinor fields λ
ia
transform in the
n-dimensional representation of SO(n), which is the tangent
space group of M, so that
g
xy
= f
a
x
f
b
y
δ
ab
, (2)
where f
a
x
is the corresponding vielbein. The bosonic part of
the Lagrangian is
e
−1
L
bos
=−
1
2
R(ω) −
1
2
g
xy
(∂
M
φ
x
)(∂
M
φ
y
)
−
1
4
G
IJ
F
I
MN
F
MNJ
+
e
−1
6
√
6
C
IJK
MNP
F
I
MN
F
J
P
A
K
,
(3)
where e = det(e
m
M
), ω is the spacetime spin-connection,
G
IJ
is the symmetric gauge kinetic metric, C
IJK
are totally
symmetric constants and the gravitational coupling κ has
been set equal to 1. The supersymmetry transformations of
the fermions of the theory are
δψ
Mi
= D
M
(ω)
i
+···
δλ
a
i
=−
1
2
if
a
x
(
/
∂φ
x
)
i
+···,
(4)
where
i
is the supersymmetry spinor parameter and the dots
stand for terms that vanish in the vacuum.
In fact, the n-dimensional M can be seen as a hypersurface
of an (n + 1)-dimensional space E with coordinates
ξ
I
= ξ
I
(φ
x
, F ), (5)
where F is the additional coordinate of E compared to M.It
can be shown that F is a homogeneous polynomial of degree
three and, more precisely, that
F = β
3
C
IJK
ξ
I
ξ
J
ξ
K
, (6)
where β =
√
2/3. It can also be shown that, on M,the
scalars φ
x
satisfy the constraint
F = 1. (7)
Moreover,
G
IJ
=−
1
2
∂
I
∂
J
ln F|
F =1
, g
xy
= G
IJ
∂
x
ξ
I
∂
y
ξ
J
|
F =1
,
(8)
where ∂
I
=
∂
∂ξ
I
and ∂
x
=
∂
∂φ
x
. Finally, we note that the
symmetric third-rank tensor T
xyz
on M is covariantly con-
stant for the symmetric M that we will be concerned with
and thus satisfies the algebraic constraint
T
w
(xy
T
zu)w
=
1
2
g
(xy
g
zu)
. (9)
The gauging of the U (1) subgroup of SU(2) generates a
scalar potential P, with
P =−P
2
0
+ P
a
P
a
, (10)
where P
0
and P
a
are functions of the scalars φ
x
that satisfy
the following constraints due to supersymmetry
P
0,x
=−
√
2β P
x
P
0,x;y
+ β T
z
xy
P
0,z
− β
2
g
xy
P
0
= 0,
(11)
where the symbols “,” and “;” denote differentiation and
covariant differentiation respectively and P
x
= f
a
x
P
a
.The
functions P
0
and P
a
also appear in the fermion transforma-
tions that get deformed due to the gauging, namely
123
剩余8页未读,继续阅读
资源评论
weixin_38607552
- 粉丝: 7
- 资源: 944
上传资源 快速赚钱
- 我的内容管理 展开
- 我的资源 快来上传第一个资源
- 我的收益 登录查看自己的收益
- 我的积分 登录查看自己的积分
- 我的C币 登录后查看C币余额
- 我的收藏
- 我的下载
- 下载帮助
最新资源
资源上传下载、课程学习等过程中有任何疑问或建议,欢迎提出宝贵意见哦~我们会及时处理!
点击此处反馈
安全验证
文档复制为VIP权益,开通VIP直接复制
信息提交成功