Chiral Gauge Theories Revisited
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On the Trace Anomaly of a Weyl Fermion in a Gauge Background
On the trace anomaly of a Weyl fermion in a gauge background Fiorenzo Bastianelli,a;b;c Matteo Broccoli,a;c aDipartimento di Fisica ed Astronomia, Universit`adi Bologna, via Irnerio 46, I-40126 Bologna, Italy bINFN, Sezione di Bologna, via Irnerio 46, I-40126 Bologna, Italy cMax-Planck-Institut f¨ur Gravitationsphysik (Albert-Einstein-Institut) Am M¨uhlenberg 1, D-14476 Golm, Germany E-mail: [email protected], [email protected] Abstract: We study the trace anomaly of a Weyl fermion in an abelian gauge background. Although the presence of the chiral anomaly implies a breakdown of gauge invariance, we find that the trace anomaly can be cast in a gauge invariant form. In particular, we find that it does not contain any odd-parity contribution proportional to the Chern-Pontryagin density, which would be allowed by the con- sistency conditions. We perform our calculations using Pauli-Villars regularization and heat kernel methods. The issue is analogous to the one recently discussed in the literature about the trace anomaly of a Weyl fermion in curved backgrounds. Keywords: Anomalies in Field and String Theories, Conformal Field Theory arXiv:1808.03489v2 [hep-th] 7 May 2019 Contents 1 Introduction1 2 Actions and symmetries3 2.1 The Weyl fermion3 2.1.1 Mass terms5 2.2 The Dirac fermion8 2.2.1 Mass terms9 3 Regulators and consistent anomalies 10 4 Anomalies 13 4.1 Chiral and trace anomalies of a Weyl fermion 13 4.1.1 PV regularization with Majorana mass 14 4.1.2 PV regularization with Dirac mass 15 4.2 Chiral and trace anomalies of a Dirac fermion 16 4.2.1 PV regularization with Dirac mass 16 4.2.2 PV regularization with Majorana mass 17 5 Conclusions 18 A Conventions 19 B The heat kernel 21 C Sample calculations 22 1 Introduction In this paper we study the trace anomaly of a chiral fermion coupled to an abelian gauge field in four dimensions. -
Regularization and Renormalization of Non-Perturbative Quantum Electrodynamics Via the Dyson-Schwinger Equations
University of Adelaide School of Chemistry and Physics Doctor of Philosophy Regularization and Renormalization of Non-Perturbative Quantum Electrodynamics via the Dyson-Schwinger Equations by Tom Sizer Supervisors: Professor A. G. Williams and Dr A. Kızılers¨u March 2014 Contents 1 Introduction 1 1.1 Introduction................................... 1 1.2 Dyson-SchwingerEquations . .. .. 2 1.3 Renormalization................................. 4 1.4 Dynamical Chiral Symmetry Breaking . 5 1.5 ChapterOutline................................. 5 1.6 Notation..................................... 7 2 Canonical QED 9 2.1 Canonically Quantized QED . 9 2.2 FeynmanRules ................................. 12 2.3 Analysis of Divergences & Weinberg’s Theorem . 14 2.4 ElectronPropagatorandSelf-Energy . 17 2.5 PhotonPropagatorandPolarizationTensor . 18 2.6 ProperVertex.................................. 20 2.7 Ward-TakahashiIdentity . 21 2.8 Skeleton Expansion and Dyson-Schwinger Equations . 22 2.9 Renormalization................................. 25 2.10 RenormalizedPerturbationTheory . 27 2.11 Outline Proof of Renormalizability of QED . 28 3 Functional QED 31 3.1 FullGreen’sFunctions ............................. 31 3.2 GeneratingFunctionals............................. 33 3.3 AbstractDyson-SchwingerEquations . 34 3.4 Connected and One-Particle Irreducible Green’s Functions . 35 3.5 Euclidean Field Theory . 39 3.6 QEDviaFunctionalIntegrals . 40 3.7 Regularization.................................. 42 3.7.1 Cutoff Regularization . 42 3.7.2 Pauli-Villars Regularization . 42 i 3.7.3 Lattice Regularization . 43 3.7.4 Dimensional Regularization . 44 3.8 RenormalizationoftheDSEs ......................... 45 3.9 RenormalizationGroup............................. 49 3.10BrokenScaleInvariance ............................ 53 4 The Choice of Vertex 55 4.1 Unrenormalized Quenched Formalism . 55 4.2 RainbowQED.................................. 57 4.2.1 Self-Energy Derivations . 58 4.2.2 Analytic Approximations . 60 4.2.3 Numerical Solutions . 62 4.3 Rainbow QED with a 4-Fermion Interaction . -
Nonperturbative Definition of the Standard Models
PHYSICAL REVIEW RESEARCH 2, 023356 (2020) Nonperturbative definition of the standard models Juven Wang 1,2,* and Xiao-Gang Wen3 1School of Natural Sciences, Institute for Advanced Study, Princeton, New Jersey 08540, USA 2Center of Mathematical Sciences and Applications, Harvard University, Cambridge, Massachusetts 02138, USA 3Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA (Received 14 June 2019; accepted 21 May 2020; published 17 June 2020) The standard models contain chiral fermions coupled to gauge theories. It has been a longstanding problem to give such gauged chiral fermion theories a quantum nonperturbative definition. By classification of quantum anomalies (including perturbative local anomalies and nonperturbative global anomalies) and symmetric interacting invertible topological orders via a mathematical cobordism theorem for differentiable and triangulable manifolds, and by the existence of a symmetric gapped boundary (designed for the mirror sector) on the trivial symmetric invertible topological orders, we propose that Spin(10) chiral fermion theories with Weyl fermions in 16-dimensional spinor representations can be defined on a 3 + 1D lattice without fermion doubling, and subsequently dynamically gauged to be a Spin(10) chiral gauge theory. As a result, the standard models from the 16n-chiral fermion SO(10) grand unification can be defined nonperturbatively via a 3 + 1D local lattice model of bosons or qubits. Furthermore, we propose that standard models from the 15n-chiral fermion -
U(1) Gauge Extensions of the Standard Model
U(1) Gauge Extensions of the Standard Model Ernest Ma Physics and Astronomy Department University of California Riverside, CA 92521, USA U(1) Gauge Extensions of the Standard Model (int08) back to start 1 Contents • Anomaly Freedom of the Standard Model • B − L • Le − Lµ and B − 3Lτ • U(1)Σ • Supersymmetric U(1)X • Some Remarks U(1) Gauge Extensions of the Standard Model (int08) back to start 2 Anomaly Freedom of the Standard Model Gauge Group: SU(3)C × SU((2)L × U(1)Y . Consider the fermion multiplets: (u, d)L ∼ (3, 2, n1), uR ∼ (3, 1, n2), dR ∼ (3, 1, n3), (ν, e)L ∼ (1, 2, n4), eR ∼ (1, 1, n5). Bouchiat/Iliopolous/Meyer(1972): The SM with n1 = 1/6, n2 = 2/3, n3 = −1/3, n4 = −1/2, n5 = −1, is free of axial-vector anomalies, i.e. 2 [SU(3)] U(1)Y : 2n1 − n2 − n3 = 0. 2 [SU(2)] U(1)Y : 3n1 + n4 = 0. 3 3 3 3 3 3 [U(1)Y ] : 6n1 − 3n2 − 3n3 + 2n4 − n5 = 0. U(1) Gauge Extensions of the Standard Model (int08) back to start 3 It is also free of the mixed gravitational-gauge anomaly, U(1)Y : 6n1 − 3n2 − 3n3 + 2n4 − n5 = 0. Geng/Marshak(1989), Minahan/Ramond/Warner(1990) : Above 4 equations ⇒ n1(4n1 − n2)(2n1 + n2) = 0. n2 = 4n1 ⇒ SM; n2 = −2n1 ⇒ SM (uR ↔ dR); n1 = 0 ⇒ n4 = n5 = n2 + n3 = 0. Here eR ∼ (1, 1, 0) may be dropped. (u, d)L, (ν, e)L have charges (1/2, −1/2) and (uR, dR) have charges (n2, −n2). -
Arxiv:0812.3578V2 [Hep-Ph] 20 Aug 2017 A
arXiv:0812.357 Regularization, Renormalization, and Dimensional Analysis: Dimensional Regularization Meets Freshman E&M ∗ Fredrick Olness & Randall Scalise Department of Physics, Southern Methodist University, Dallas, TX 75275-0175, U.S.A. (Dated: August 22, 2017) We illustrate the dimensional regularization (DR) technique using a simple problem from elementary electrostatics. This example illustrates the virtues of DR without the complications of a full quan- tum field theory calculation. We contrast the DR approach with the cutoff regularization approach, and demonstrate that DR preserves the translational symmetry. We then introduce a Minimal Sub- traction (MS) and a Modified Minimal Subtraction (MS) scheme to renormalize the result. Finally, we consider dimensional transmutation as encountered in the case of compact extra-dimensions. PACS numbers: 11.30.-j Symmetry and conservation laws 11.10.Kk Field theories in dimensions other than four 11.15.-q Gauge field theories 11.10.Gh Renormalization Keywords: Renormalization, Dimensional Regularization, Regularization, Gauge Symmetries Contents VI. Renormalization 6 A. Connection to QFT 6 I. Dimensional Regularization 2 VII. The Renormalization Group Equation 6 A. Introduction and Motivation 2 A. Physical Observables: 6 B. Relating Perturbative & Non-Perturbative II. Dimension Analysis: The Pythagorean Functions 7 Theorem 2 VIII. Extra Dimensions 7 III. An Infinite Line of Charge 3 A. E and V in arbitrary dimensions 7 A. Statement of the Problem 3 B. Scale invariance: 3 IX. Conclusions 8 IV. Cutoff Regularization: 4 Acknowledgment 8 arXiv:0812.3578v2 [hep-ph] 20 Aug 2017 A. Cutoff Regularization Computation 4 X. Appendix 8 B. Computation of E and δV 4 A. 3-Dimensions 8 C. -
Green-Schwarz Anomaly Cancellation
Green-Schwarz anomaly cancellation Paolo Di Vecchia Niels Bohr Instituttet, Copenhagen and Nordita, Stockholm Collège de France, 05.03.10 Paolo Di Vecchia (NBI+NO) GS anomaly cancellation Collège de France, 05.03.10 1 / 30 Plan of the talk 1 Introduction 2 A quick look at the abelian axial anomaly 3 Few words on forms 4 Anomaly cancellation in type IIB superstring theory 5 Anomaly cancellation in type I superstring 6 Conclusions Paolo Di Vecchia (NBI+NO) GS anomaly cancellation Collège de France, 05.03.10 2 / 30 Introduction I The theory of general relativity for gravity was formulated by Einstein in 1915. I It is a four-dimensional theory that extends the theory of special relativity. I While special relativity is invariant under the transformations of the Lorentz group, general relativity is invariant under an arbitrary change of coordinates. I In the twenties it was proposed by Theodor Kaluza and Oskar Klein to unify electromagnetism with gravity by starting from general relativity in a five-dimensional space-time and compactify the extra-dimension on a small circle. I In this way one obtains general relativity in four dimensions, a vector gauge field satisfying the Maxwell equations and a scalar. I This idea of extra dimensions was not pursued in the years after. I In the sixties and seventies, when I started to work in the physics of the elementary particles, everybody was strictly working in four dimensions. Paolo Di Vecchia (NBI+NO) GS anomaly cancellation Collège de France, 05.03.10 3 / 30 I Also the dual resonance model, being a model for hadrons, was obviously formulated in four dimensions. -
The Quantum Vacuum and the Cosmological Constant Problem
The Quantum Vacuum and the Cosmological Constant Problem S.E. Rugh∗and H. Zinkernagely To appear in Studies in History and Philosophy of Modern Physics Abstract - The cosmological constant problem arises at the intersection be- tween general relativity and quantum field theory, and is regarded as a fun- damental problem in modern physics. In this paper we describe the historical and conceptual origin of the cosmological constant problem which is intimately connected to the vacuum concept in quantum field theory. We critically dis- cuss how the problem rests on the notion of physically real vacuum energy, and which relations between general relativity and quantum field theory are assumed in order to make the problem well-defined. 1. Introduction Is empty space really empty? In the quantum field theories (QFT’s) which underlie modern particle physics, the notion of empty space has been replaced with that of a vacuum state, defined to be the ground (lowest energy density) state of a collection of quantum fields. A peculiar and truly quantum mechanical feature of the quantum fields is that they exhibit zero-point fluctuations everywhere in space, even in regions which are otherwise ‘empty’ (i.e. devoid of matter and radiation). These zero-point fluctuations of the quantum fields, as well as other ‘vacuum phenomena’ of quantum field theory, give rise to an enormous vacuum energy density ρvac. As we shall see, this vacuum energy density is believed to act as a contribution to the cosmological constant Λ appearing in Einstein’s field equations from 1917, 1 8πG R g R Λg = T (1) µν − 2 µν − µν c4 µν where Rµν and R refer to the curvature of spacetime, gµν is the metric, Tµν the energy-momentum tensor, G the gravitational constant, and c the speed of light. -
On the Regularization of Phase-Space Path Integral in Curved Manifolds
On the Regularization of Phase-Space Path Integral in Curved Manifolds Marco Falconi June 1, 2010 ......................................................................................................... Introduction n this work we discuss path integrals both in flat and curved space-time: in particular I we describe how to write the integral kernel of the time evolution operator (in a curved space time we describe the evolution with respect to a geodesic affine parameter, such as the proper time if the particle has a non-zero mass) in a path integral form, both in configuration and phase space. We briefly introduce a path integral formulation of Quantum Field Theo- ries, however we focus our attention mainly on quantum mechanical models. We develop the idea, originally due to Schwinger, to describe effective actions in quantum field theory as quantum mechanical path integrals of a fictitious particle with evolution dictated by a suitable Hamiltonian function. We will see that one could have obtained the same result as in field theory by first quantizing the particle which actually makes the loop of the Feynman graph corresponding to the effective action. In the second part we focus on a particle of mass m ≥ 0 that classically moves along a geodesic of curved space-time. Quantizing this model we will see that even if it is still possible to describe its evolution in the affine parameter by means of a path integral, the results obtained would be ambiguous unless we introduce suitable regularization schemes and related counterterms. This is, in fact, the key point of path integrals used in physics. Configuration space path integral needs different counterterms, depending on the reg- ularization scheme used, in order to give the same results at any perturbative order for the integral kernel of the evolution operator. -
Anomaly-Free Supergravities in Six Dimensions
Anomaly-Free Supergravities in Six Dimensions Ph.D. Thesis arXiv:hep-th/0611133v1 12 Nov 2006 Spyros D. Avramis National Technical University of Athens School of Applied Mathematics and Natural Sciences Department of Physics Spyros D. Avramis Anomaly-Free Supergravities in Six Dimensions Dissertation submitted to the Department of Physics of the National Technical University of Athens in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Physics. Thesis Advisor: Alex Kehagias Thesis Committee: Alex Kehagias Elias Kiritsis George Zoupanos K. Anagnostopoulos A.B. Lahanas E. Papantonopoulos N.D. Tracas Athens, February 2006 Abstract This thesis reviews minimal N = 2 chiral supergravities coupled to matter in six dimensions with emphasis on anomaly cancellation. In general, six-dimensional chiral supergravities suffer from gravitational, gauge and mixed anomalies which, being associated with the breakdown of local gauge symmetries, render the theories inconsistent at the quantum level. Consistency of the theory is restored if the anomalies of the theory cancel via the Green-Schwarz mechanism or generalizations thereof, in a similar manner as in the case of ten-dimensional N = 1 supergravi- ties. The anomaly cancellation conditions translate into a certain set of constraints for the gauge group of the theory as well as on its matter content. For the case of ungauged theories these constraints admit numerous solutions but, in the case of gauged theories, the allowed solutions are remarkably few. In this thesis, we examine these anomaly cancellation conditions in detail and we present all solutions to these conditions under certain restrictions on the allowed gauge groups and representations, imposed for practical reasons. -
Anomalies and the Standard Model of Particle Physics
Anomalies and the Standard Model of Particle Physics Nakarin Lohitsiri Supervisor: Professor David Tong Department of Applied Mathematics and Theoretical Physics University of Cambridge This dissertation is submitted for the degree of Doctor of Philosophy Trinity College August 2020 For my parents Declaration This dissertation is based on original research done by the author while he was a graduate student at the Department of Applied Mathematics and Theoretical Physics, University of Cambridge, between October 2016 and August 2020. The material in Chapters2 and5 is based on the work done by the author under the supervision of David Tong and has been partly published in References [97, 96], while Chapters3 and4 are based on research done in collaboration with Joe Davighi, part of which is published in References [53, 52]. Except for part of Chapter3 that has been previously submitted for a degree of doctor of philosophy by Joe Davighi at the University of Cambridge, no other part of this work has been submitted, or is being concurrently submitted, for a degree or other qualification at the University of Cambridge or any other university or similar institution. Nakarin Lohitsiri August 2020 Anomalies and the Standard Model of Particle Physics Nakarin Lohitsiri This dissertation aims to study quantum anomalies and some other aspects of the Standard Model of Particle physics. In any quantum gauge field theory, anomalies place a very restrictive condition on the matter content and the dynamics. The former is due to the cancellation of gauge anomalies while ’t Hooft anomaly matching constraints produce the latter. As the Standard Model, which is our most fundamental and most accurate description of particle physics, is constructed as a gauge field theory, it is also subject to these anomalies. -
Gauge Theory
Preprint typeset in JHEP style - HYPER VERSION 2018 Gauge Theory David Tong Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 OBA, UK http://www.damtp.cam.ac.uk/user/tong/gaugetheory.html [email protected] Contents 0. Introduction 1 1. Topics in Electromagnetism 3 1.1 Magnetic Monopoles 3 1.1.1 Dirac Quantisation 4 1.1.2 A Patchwork of Gauge Fields 6 1.1.3 Monopoles and Angular Momentum 8 1.2 The Theta Term 10 1.2.1 The Topological Insulator 11 1.2.2 A Mirage Monopole 14 1.2.3 The Witten Effect 16 1.2.4 Why θ is Periodic 18 1.2.5 Parity, Time-Reversal and θ = π 21 1.3 Further Reading 22 2. Yang-Mills Theory 26 2.1 Introducing Yang-Mills 26 2.1.1 The Action 29 2.1.2 Gauge Symmetry 31 2.1.3 Wilson Lines and Wilson Loops 33 2.2 The Theta Term 38 2.2.1 Canonical Quantisation of Yang-Mills 40 2.2.2 The Wavefunction and the Chern-Simons Functional 42 2.2.3 Analogies From Quantum Mechanics 47 2.3 Instantons 51 2.3.1 The Self-Dual Yang-Mills Equations 52 2.3.2 Tunnelling: Another Quantum Mechanics Analogy 56 2.3.3 Instanton Contributions to the Path Integral 58 2.4 The Flow to Strong Coupling 61 2.4.1 Anti-Screening and Paramagnetism 65 2.4.2 Computing the Beta Function 67 2.5 Electric Probes 74 2.5.1 Coulomb vs Confining 74 2.5.2 An Analogy: Flux Lines in a Superconductor 78 { 1 { 2.5.3 Wilson Loops Revisited 85 2.6 Magnetic Probes 88 2.6.1 't Hooft Lines 89 2.6.2 SU(N) vs SU(N)=ZN 92 2.6.3 What is the Gauge Group of the Standard Model? 97 2.7 Dynamical Matter 99 2.7.1 The Beta Function Revisited 100 2.7.2 The Infra-Red Phases of QCD-like Theories 102 2.7.3 The Higgs vs Confining Phase 105 2.8 't Hooft-Polyakov Monopoles 109 2.8.1 Monopole Solutions 112 2.8.2 The Witten Effect Again 114 2.9 Further Reading 115 3. -
The Casimir Effect
April 19th 2009 The Casimir Effect Version 3 A Comprehensive Exercise by Kyle Kingsbury Abstract The Casimir Effect is a small force on conducting surfaces which arises from quantum electrodynamics. Quantizing the electromagnetic field yields a small ground-state energy for each frequency. Summing over all frequencies implies the field has an infinite vacuum energy. Between conducting surfaces, this energy may be dependent on geometry, which gives rise to forces on the boundaries. This comprehensive exercise ex- plores the electromagnetic ground state energy and the consequent force between two conducting plates. Some extensions and generalizations of the Casimir force to other geometries and temperatures are dis- cussed. Finally, it offers a brief overview of experi- mental attempts to confirm the effect. Contents 1 Introduction 2 2 Quantizing the Electromagnetic Field 3 3 The Force Between Two Plates 6 3.1 Casimir's Derivation . 6 3.2 A Modern Derivation . 11 3.3 Other Regularization Techniques . 14 4 Atomic Geometry 14 4.1 Historical Context . 14 4.2 Atom-Plate Interactions . 15 4.3 Atom-Atom Interaction . 16 5 Geometry Dependence 16 5.1 A Spherical Shell . 17 5.2 Corners . 18 6 Temperature Dependence 19 6.1 Basic Thermodynamics . 19 6.2 Numerical Modeling . 20 7 Experimental Verification 22 7.1 Early Efforts . 22 7.2 Modern Experiments . 23 7.3 Optical Transparency . 25 7.4 Repulsive Forces . 26 7.5 Electrostatic Interactions . 26 8 Conclusion 27 Bibliography 28 1 1 Introduction Weird things happen in nature. Physicists, concerned with modeling and predicting the fundamen- tal dynamics that underlie the observable universe, frequently find themselves discussing things which|to our everyday physical intuition|might seem completely impossible, yet the physics works.