Renormalization of Supersymmetric Lifshitz Sigma Models Ziqi Yan Nordita KTH Royal Institute of Technology and Stockholm University

2025-04-29 0 0 646.55KB 36 页 10玖币
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Renormalization of Supersymmetric Lifshitz Sigma Models
Ziqi Yan
Nordita, KTH Royal Institute of Technology and Stockholm University
Hannes Alfv´ens v¨ag 12, SE-106 91 Stockholm, Sweden
E-mail: ziqi.yan@su.se
Abstract: We study the renormalization of an N= 1 supersymmetric Lifshitz sigma model
in three dimensions. The sigma model exhibits worldvolume anisotropy in space and time
around the high-energy z= 2 Lifshitz point, such that the worldvolume is endowed with
a foliation structure along a preferred time direction. In curved backgrounds, the target-
space geometry is equipped with two distinct metrics, and the interacting sigma model is
power-counting renormalizable. At low energies, the theory naturally flows toward the rel-
ativistic sigma model where Lorentz symmetry emerges. In the superspace formalism, we
develop a heat kernel method that is covariantized with respect to the bimetric target-space
geometry, using which we evaluate the one-loop beta-functions of the Lifshitz sigma model.
This study forms an essential step toward a thorough understanding of the quantum critical
supermembrane as a candidate high-energy completion of the relativistic supermembrane.
arXiv:2210.04950v2 [hep-th] 27 Feb 2023
Contents
1. Introduction 2
2. O(N)Nonlinear Sigma Models at a z= 2 Lifshitz point 4
2.1. Relativistic O(N) Nonlinear Sigma Model 5
2.2. Scalar Field Theories at a Lifshitz Point 5
2.3. O(N) Nonlinear Sigma Model at a z= 2 Lifshitz Point 7
2.4. Lifshitz Nonlinear Sigma Model with N= 1 Supersymmetry 9
3. General Sigma Models at a z= 2 Lifshitz Point 12
3.1. The Classical Theory 12
3.1.1. Supersymmetric sigma models and bimetricity 13
3.1.2. Covariant background field method 14
3.1.3. The classical propagator 16
3.1.4. Quaternions and bimetric symmetry 17
3.2. One-Loop Effective Action in Superspace 19
3.2.1. The heat kernel equation 20
3.2.2. Fourier transform in superspace 20
3.2.3. Seeley-Gilkey coefficients 21
3.2.4. Solving the recursion relations 23
3.2.5. Changing the reference metric 25
3.3. Renormalization Group Flows 26
4. Quantum Critical Membranes 27
5. Conclusions 29
– 1 –
1. Introduction
The quantization of supermembranes in eleven-dimensional spacetime is key to a better un-
derstanding of M-theory, which provides a unification of different superstring theories in a
nonperturbative manner. Supermembranes are described by a three-dimensional sigma model
[1], whose quantization is fundamentally distinct from quantizing strings. One of the major
difficulties is that three-dimensional relativistic sigma models are not renormalizable, which
invalidates any perturbative treatment. Nevertheless, it is possible to probe some features
of the supermembrane in the light-cone quantization, at least when a matrix regularization
is employed on the spatial manifold of the worldvolume [2,3]. This regularization restricts
the infinite-dimensional basis on the continuum manifold to a finite-dimensional Lie group,
and the supermembrane is described as a subtle limit of supersymmetric matrix quantum
mechanics [4], closely related to D0-branes in the infinite momentum frame and the Matrix
theory description of M-theory [5]. 1However, a complete understanding of the continuous
spectrum of Matrix theory is still lacking [12,13], which requires a multiparticle interpreta-
tion and thus a second quantization of the membrane [5]. This light-cone treatment is also
limited to special backgrounds, due to the absence of spacetime covariance. Finally, when the
sigma model is coupled to a dynamical worldvolume described by three-dimensional quantum
supergravity, there still exists neither clear quantization technique nor classical expansion for
the membrane [14]. See, e.g., [15,16] for excellent reviews.
According to the Matrix theory description, a supermembrane is unstable and tends to
be dissolved into dynamical bits [12]. 2This suggests that membranes might not be the funda-
mental objects. However, it is still highly valuable to probe M-theory from the worldvolume
perspectives, especially in regard of the lacking of any covariant formalism of supermem-
branes. Since the three-dimensional sigma model is nonrenormalizable, which suggests that
new physics may arise above a particular cutoff. It is therefore natural to ask whether there
exists a renormalizable QFT at our disposal, which can be regarded as an ultra-violet (UV)
completion of the nonrenormalizable membrane theory. If so, there might exist a stable
notion of membranes that only become strongly coupled at low energies, where the Matrix
theory description becomes valid and the physics is captured by emergent multiparticle states.
Unfortunately, no such renormalizable worldvolume theory seems to be available within the
relativistic framework.
It is pioneered in [17] that the relativistic membrane might admit a UV completion
that exhibits nonrelativistic behaviors on the worldvolume: a renormalizable sigma model
describing membranes propagating in spacetime can be constructed if an anisotropy between
the worldvolume space and time is introduced. Furthermore, this sigma model is required
1Another way of obtaining Matrix theory is by considering the discrete light cone quantization (DLCQ)
of M-theory, which is usually defined as a subtle limit of the compactification over a spatial circle [69]. An
alternative treatment of the DLCQ of string/M-theory as nonrelativistic string/M-theory is recently revived
in e.g. [10,11].
2This instability of the membrane was resolved in the Matrix theory description by realizing that the Hilbert
space of the matrix quantum mechanics naturally contains multi-particle states of the D0-bits [5].
– 2 –
to satisfy a Lifshitz scaling with the dynamical critical exponent z= 2 , which measures the
anisotropy between the worldvolume time tand space x,
tb t , xb1/z x.(1.1)
Consequently, the worldvolume degrees of freedom satisfy a quadratic dispersion relation,
ω2∼ |k|4,(1.2)
where ωdenotes the frequency and kthe two-dimensional spatial momentum. The mem-
brane described by such a Lifshitz-type sigma model is referred to as the membrane at
quantum criticality [17]. On a curved worldvolume, this Lifshitz sigma model is coupled to
three-dimensional Hoˇrava gravity, which geometrizes the foliation-preserving diffeomorphisms
compatible with the worldvolume anisotropy. Since the worldvolume is foliated by leaves of
constant time, it is possible to consistently restrict the sum over general three-manifolds in
the membrane theory to foliated manifolds, where the spatial leaves are Riemann surfaces.
This may facilitate a perturbative expansion in membranes, akin to the perturbative expan-
sion with respect to the genera of Riemann surfaces in string theory [17]. At low energies, a
relevant deformation is turned on and modifies the dispersion relation (1.2) to be
ω2∼ |k|4+c2|k|2,(1.3)
with a coupling cthat is dimensionful from the UV perspective around the z= 2 Lifshitz
point. Classically, this relevant deformation ostensibly generates a renormalization group
(RG) flow toward the relativistic, nonperturbative membrane theory in the deep infrared
(IR), where low-energy Lorentz symmetry emerges. Whether and how this RG flow toward
a Lorentzian fixed point could be realized quantum mechanically poses a challenging ques-
tion, which requires detailed analysis of the worldvolume dynamics. If achieved, it is then
tempting to conjecture that the ultimately fundamental objects in M-theory might be such
nonrelativistic membranes at quantum criticality.
In this paper, we study a renormalizable three-dimensional Lifshitz-type sigma model that
exhibits a z= 2 Lifshitz scaling symmetry at the critical point. This sigma model constitutes
an essential ingredient for the construction of the membrane at quantum criticality. We will
focus on the case where the worldvolume is flat. The full-fledged membrane theory, however,
requires us to couple the matter contents of the sigma model to dynamical worldvolume
Hoˇrava gravity. On the other hand, in the absence of worldvolume gravitational dynamics,
the quantization of Lifshitz-type sigma models already imposes intriguing challenges and
requires new techniques to tackle with.
In the bosonic case, the most general three-dimensional sigma model at a z= 2 Lifshitz
point is coupled to higher-rank tensorial background fields, which makes the quantization
rather difficult. In the simpler case where the target space is O(N) symmetric, the z= 2
nonlinear sigma model (NLSM) already exhibits intriguing RG properties [1820], for which
– 3 –
we will give a quick review as a preparation for the quantization of Lifshitz sigma models
in arbitrary geometric background fields. The study of Lifshitz O(N) NLSM bears potential
applications to the condensed matter systems of quantum spin liquids [2123] and quantum
spherical models [2426].
In connection to the studies of supermembranes, we are ultimately interested in super-
symmetric sigma models, which bring significant simplifications in comparison to the pure
bosonic case. The three-dimension N= 1 supersymmetric sigma model around a z= 2 Lif-
shitz point has been introduced in [27,28] (also see [29] for a review), which is power-counting
renormalizable. The relevant target-space geometry is Lorentzian and has two independent
metrics, but there is no extra higher-form tensorial structure as in the bosonic case. In
the deep IR, a relevant deformation controlled by the coupling constant associated with the
worldvolume speed of light dominates, which drives the theory toward the relativistic fixed
point satisfying a z= 1 Lifshitz scaling. We will generalize the heat kernel method in [29,30]
to supersymmetric field theories on a foliated spacetime manifold, and use it to study the
RG flows of the supersymmetric Lifshitz sigma model. This will form an essential step to-
ward determining whether such a worldvolume theory is qualified to be a quantum membrane
theory that UV completes the relativistic supermembranes, which also requires coupling the
Lifshitz sigma model to dynamical worldvolume supergravity. At the z= 2 Lifshitz point,
the worldvolume supergravity is also power-counting renormalizable in three dimensions and
possesses a preferred time direction, which makes it possible to study its quantization as a
conventional quantum field theory.
The paper is organized as follows. In Section 2, as a warm-up, we discuss the renormaliza-
tion of three-dimensional z= 2 Lifshitz O(N) NLSM. In Section 3, we study three-dimensional
N= 1 supersymmetric z= 2 Lifshitz sigma model, which is described by the action (3.4) and
is coupled to a bimetric target-space geometry. We derive the one-loop beta-functionals for
the bimetric fields in this Lifshitz sigma model in Eq. (3.84), which form the major results of
this paper. In Section 4, as a preliminary step toward the formulation of the supersymmetric
quantum critical membrane, we couple the bosonic part of the sigma model to dynamical
worldvolume Hoˇrava gravity. We conclude the paper in Section 5.
2. O(N)Nonlinear Sigma Models at a z= 2 Lifshitz point
In this section, we illustrate some of the basic ingredients in our later construction of general
three-dimensional Lifshitz sigma models by a simple example, where the target space of the
sigma model is O(N) symmetric. We parametrize the target space by a vector field na,
a= 1,··· , N , which satisfies the constraint
n·n= 1 .(2.1)
We will first review the relativistic O(N) NLSM in three dimensions, which is not renormaliz-
able. Then, we proceed to the construction of the three-dimensional O(N) NLSM at a z= 2
Lifshitz point, which flows toward the relativistic NLSM in the deep IR.
– 4 –
摘要:

RenormalizationofSupersymmetricLifshitzSigmaModelsZiqiYanNordita,KTHRoyalInstituteofTechnologyandStockholmUniversityHannesAlfvensvag12,SE-10691Stockholm,SwedenE-mail:ziqi.yan@su.seAbstract:WestudytherenormalizationofanN=1supersymmetricLifshitzsigmamodelinthreedimensions.Thesigmamodelexhibitsworldv...

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