Mass spectrum of type IIB ux compactications comments on AdS vacua and

2025-05-02 0 0 418.4KB 24 页 10玖币
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Mass spectrum of type IIB flux compactifications
comments on AdS vacua and
conformal dimensions
Erik Plauschinn
Institute for Theoretical Physics, Utrecht University
Princetonplein 5, 3584CC Utrecht
The Netherlands
Abstract
In this note we study the mass spectrum of type IIB flux compactifications.
We first give a general discussion of the mass matrix for F-term vacua in
four-dimensional N= 1 supergravity theories and then specialize to type
IIB Calabi-Yau orientifold compactifications in the presence of geometric
and non-geometric fluxes. F-term vacua in this setting are in general AdS4
vacua for which we compute the conformal dimensions of operators dual to
the scalar fields. For the mirror-dual of the DGKT construction we find
that one-loop corrections to the complex-structure moduli space lead to
real-valued conformal dimensions — only when ignoring these corrections
we recover the integer values previously reported in the literature. For an
example of a flux configurations more general than the DGKT mirror we
also obtain non-integer conformal dimensions. Furthermore, we argue that
stabilizing moduli in asymptotic regions of moduli space implies that at least
one of the mass eigenvalue diverges.
1
arXiv:2210.04528v1 [hep-th] 10 Oct 2022
Contents
1 Introduction 2
2 Mass matrix and conformal dimensions 4
3 Type IIB flux compactifications 6
4 Conformal dimensions 9
5 Asymptotic regions 15
6 Summary and conclusions 18
A Computational details 20
1 Introduction
String theory is a theory of quantum gravity including gauge interactions. Its
supersymmetric version is consistent in ten space-time dimensions and can be
connected to four-dimensional physics through compactification. Well-understood
compactification spaces are Calabi-Yau three-folds whose resulting lower-dimen-
sional theories have a Minkowski vacuum. Deformations that preserve the Calabi-
Yau condition correspond to massless scalar fields (moduli) in four dimensions,
however, it is possible to deform the compact space away from being Calabi-Yau
by turning on fluxes. Such fluxes generate mass terms for the moduli and typically
lead to AdS4vacua. For gravity theories in AdS spaces one can then apply the
AdS/CFT dictionary to relate, for instance, the masses of scalar fields in AdS4to
conformal dimensions of corresponding operators in a putative three-dimensional
CFT. For a certain class of type II flux compactifications, more concretely for
the construction by DeWolfe, Giryavets, Kachru, and Taylor (DGKT) in type IIA
string theory [1], it was observed in [2–5] that the conformal dimensions of all
scalar fields in the closed-string sector are integer-valued. In [2, 3] the analysis
was done for toroidal compactifications, while in [4,5] the authors performed their
computation for a general Calabi-Yau three-fold.
Obtaining integer conformal dimensions irrespective of the compactification
space is a rather surprising observation which one would like to understand. In
particular, one would like to know which features of the compactification are rel-
evant for this result. This question was addressed in [5], where it was found that
some non-supersymmetric type IIA vacua do not lead to integer-valued conformal
dimensions. However, one can argue that such configurations are unstable [6] and
2
therefore are not suitable for the applying the AdS/CFT correspondence [5]. In
this note we approach the question of integer conformal dimensions from the type
IIB side. We study orientifold compactifications of type IIB string theory with
geometric and non-geometric fluxes that lead to supersymmetric AdS4vacua. In
regard to the DGKT construction in type IIA string theory [1] we note the follow-
ing differences:
1. On the type IIA side one typically considers the large-volume limit without
corrections. In type IIB string theory this limit corresponds to the large-
complex-structure limit, for which corrections are well-understood. We can
therefore compute conformal dimensions in a setting that includes corrections
to the moduli-space geometry.
2. For DGKT flux compactifications in type IIA string theory the superpo-
tential splits into the sum of two independent terms [7]. From a type IIB
perspective this is a rather special case that corresponds to turning on only a
specific component of geometric and non-geometric Neveu-Schwarz–Neveu-
Schwarz fluxes. For a more general flux-choice the superpotential will not
split in this way.
In this work we investigate these two aspects. First, we consider the mirror-
dual of the DGKT setting — including perturbative corrections to the complex-
structure moduli space — and determine masses and conformal dimensions ana-
lytically. Second, we construct a flux configuration for which the superpotential
does not split into two separate terms and determine the masses and conformal
dimensions numerically. More concretely,
in section 2 we give a general discussion of the mass matrix for F-term vacua
of four-dimensional N= 1 supergravity theories. In section 3 we then spe-
cialize to Calabi-Yau orientifold compactifications of type IIB string theory
with O3- and O7-planes in the presence of geometric Ramond-Ramond (R-R)
and geometric and non-geometric Neveu-Schwarz–Neveu-Schwarz (NS-NS)
fluxes.
In section 4 we determine masses and conformal dimensions for AdS4flux-
vacua. For the mirror-dual of DGKT we find analytically that perturbative
corrections to the prepotential lead to non-integer conformal dimensions.
We also study an example with a flux choice more general than DGKT for
which the superpotential does not split into two separate terms. Here we
find numerically that the conformal dimensions are not integer.
Section 5 is independent of our discussion of AdS vacua and conformal di-
mensions, but uses many results from sections 2 and 3. Here we study flux
3
compactifications relevant for the KKLT and large-volume scenarios [8, 9],
where only the F-terms of the complex-structure moduli and the axio-dilaton
are considered. We compute the trace of the canonically-normalized mass
matrix and argue that if moduli are stabilized in an asymptotic regime of
moduli space, then at least one of the mass eigenvalues diverges.
In section 6 we summarize our findings and in appendix A we give some
technical details of the computations in the main text.
2 Mass matrix and conformal dimensions
Let us start with a discussion of masses of chiral multiplets in four-dimensio-
nal N= 1 supergravity theories. We consider minima of the scalar potential
corresponding to vanishing F-terms and determine the general form of the mass
matrix of the scalar fields. In the case of AdS4vacua we furthermore compute the
conformal dimension of operators dual to the scalar fields.
F-term minima
Let us consider a four-dimensional N= 1 supergravity theory with ncomplex
scalar fields φMwhere M= 1, . . . , n. The F-term scalar potential can be written
as
V=eKhFMGMN FN3|W|2i,(2.1)
where Kdenotes the real K¨ahler potential, Wdenotes the holomorphic superpo-
tential, and GMN =MNKdenotes the K¨ahler metric. The F-terms are given by
FM=MW+KMWwith KM=MK. In this work we are interested in F-term
minima of this potential given by
FM= 0 .(2.2)
Mass matrix
The mass matrix for the complex scalar fields of this theory corresponds to the
second derivatives of the potential (2.1). It can be arranged into the form
m2="m2
MN m2
MN
m2
MN m2
MN #,(2.3)
4
where the blocks in the first line are related to the ones appearing in the second
line by complex conjugation. For the former we find the following expressions at
the minimum (2.2)
m2
MN =eKhMFPGP Q NFQ2GM N |W|2i,
m2
MN =eK2MFNW.
(2.4)
In order to obtain the canonically-normalized mass matrix we note that the ahler
metric GMN is hermitian and positive definite. We can therefore write Gas the
square of a positive-definite matrix Γ and we define a matrix Qas
G= ΓΓ, Q = Γ1(F )ΓT.(2.5)
Here and in the following we suppress identity matrices δMN ,δMN , and δMN.
The canonically-normalized mass matrix is obtained by multiplying (2.3) with
appropriate factors of Γ from the left and the right and we find
m2
can =eKQQ2|W|2QW
QW QQ2|W|2.(2.6)
Mass eigenvalues
In order to determine the eigenvalues of (2.6) we first perform a singular-value
decomposition of Qas
Q=UΣV,(2.7)
where Uand Vare unitary matrices and Σ is a diagonal matrix that contains only
real entries. We can then write the canonically-normalized mass matrix (2.6) as
m2
can =eKU0
0VΣ22|W|2ΣW
ΣWΣ22|W|2U0
0V,(2.8)
and the corresponding eigenvalue equation for the mass eigenvalues m2is given by
0 = dethm2
can m2i
= dethe2Kh22|W|2eKm2)2Σ2|W|2ii.
(2.9)
Denoting the entries of the diagonal matrix Σ2by σ2
α, we can solve (2.9) as
m2
α±=eKhσ2
α±σα|W| − 2|W|2i.(2.10)
We finally note that QQ=UΣ2Uand QQ=VΣ2V, and hence σ2
αare the real
and positive eigenvalues of the hermitian matrices QQand QQ.
5
摘要:

MassspectrumoftypeIIBuxcompacti cations|commentsonAdSvacuaandconformaldimensionsErikPlauschinnInstituteforTheoreticalPhysics,UtrechtUniversityPrincetonplein5,3584CCUtrechtTheNetherlandsAbstractInthisnotewestudythemassspectrumoftypeIIBuxcompacti cations.We rstgiveageneraldiscussionofthemassmatrixforF...

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