Renormalization of Fermion Mixing

Total Page:16

File Type:pdf, Size:1020Kb

Renormalization of Fermion Mixing Renormalization of Fermion Mixing Dissertation zur Erlangung des Grades ,^)oktor der Naturwissenschaften" am Fachbereich Physik der Johannes Gutenberg-Universitat in Mainz Roxana gchiopu geb. in Rimnicu Vilcea, Rumanien Mainz, den 11. Mai 2007 M'bZer (md ZoMg e^ougA, ZAe avocado w;H grow. Datum der miindlichen Pnifmig: 11. Mai 2007 Contents 1 Introduction and Motivation 1 2 Lagrange Density and Feynman Rules for Dirac and Majorana Fermions 5 2.1 Remarks on Conventions and Notations ................................................. 5 2.2 Lagrange Density Mass Term ................................................................. 6 2.2.1 Dirac Mass Term.......................................................................... 6 2.2.2 Majorana Mass Term.................................................................... 7 2.2.3 Dirac-Majorana Mass Term....................................................... 11 2.3 General Form for the Lagrange Density with Dirac and Majorana Fermions ...................................................................................................... 13 2.4 Feynman Rules......................................................................................... 15 2.4.1 Feynman Rules with Dirac Particles........................................... 16 2.4.2 Feynman Rules with Dirac and Majorana Particles................... 18 3 One-loop Fermion Self-Energies 23 3.1 General Expression for the Dirac Fermion Self-Energy .........................23 3.1.1 Diagrams with Vector Bosons ........................................................ 23 3.1.2 Diagrams with Scalar Bosons ........................................................ 28 3.1.3 Analysis of Divergent and Imaginary Parts....................................30 3.2 General Expressions for the Dirac and Majorana Fermion Self-Energies 31 3.2.1 Dirac Fermion Self-Energy .............................................................. 32 3.2.2 Majorana Fermion Self-Energy ........................................................ 34 3.3 Summary of Results for Fermion Self-Energies .....................................39 4 Divergences of Fermion Self-Energies 45 4.1 Analysis of the One-loop Fermion Propagator ..................................... 47 4.2 Imaginary Parts, Divergences and Gauge Dependence ............................ 55 5 Renormalization of the Free Fermionic Lagrangian 63 5.1 Renormalized Free Dirac Lagrangian ........................................................ 63 i CONTENTS 5.1.1 General Renormalized Free Lagrangian .....................................64 5.1.2 Hermitian Renormalized Free Lagrangian ..................................70 5.1.3 Re-diagonalized Maas Term Approach ........................................ 71 5.2 Renormalized Free Major ana Lagrangian .................................................. 80 5.2.1 General Renormalized Free Lagrangian .....................................80 5.2.2 Hermitian Renormalized Free Lagrangian ..................................85 5.2.3 Re-diagonalized Mass Term Approach ........................................86 5.3 Remarks on CPT Invariance ........................................................................88 6 Renormalization of the Interaction Lagrangian 93 6.1 Interaction Terms with Dirac Fermions ..................................................... 93 6.1.1 Interaction Terms with Vector Bosons ............................................94 6.1.2 Interaction Terms with Scalar Bosons ............................................98 6.2 Interaction Terms with Majorana Fermions ............................................. 100 6.3 Generic Fermion Interaction Terms..........................................................102 6.4 Feynman Rules Derived from the Renormalized Lagrange Density . 104 6.5 One-loop Corrections to Vertices................................................................107 7 Renormalization of the Quark Mixing Matrix 113 7.1 Corrections to the Quark-Antiquark-IV Vertex ....................................... 113 7.1.1 Corrections from the Renormalized Parameters ........................114 7.1.2 Corrections from the One-loop Diagrams....................................116 7.1.3 Discussion of the One-loop Renormalized Quark Mixing Matrix 119 7.2 Top Decay Rate ........................................................................................ 123 8 Neutrino Seesaw Mechanism and the Renormalization of the Mix­ ing Matrix 131 8.1 Seesaw Mass Term..................................................................................... 132 8.2 Lagrange Density for Seesaw Type I......................................................... 134 8.3 Lagrange Density for Seesaw Type II...................................................... 139 8.4 Model Restrictions and Field Renormalization Constants ..................... 145 8.5 Corrections to the Neutrino Mixing Matrix and Unitarity .....................149 8.6 Corrections to the Lepton-IV Vertex ...................................................... 150 8.7 Heavy Neutrino Decay Rate......................................................................156 9 Summary 159 A Dimensional Regularization 163 CONTENTS iii B One- and Two-point Integrals 165 B.l Definitions ....................................................................................................165 B. 2 Evaluation of the One- and Two-point Integrals ................................... 166 B.2.1 Complete Evaluation of Bo(p2; mi, mg).....................................168 B.2.2 Particular On-shell Cases for Eg, Ei and Their Derivatives . 171 B.2.3 Complete Evaluation of Eg and E^............................................. 172 C Matrix Manipulations for One-loop Calculations 175 C. l Matrix Inversion ........................................................................................175 C.2 Unitary Matrix ...........................................................................................176 C.3 Matrix Diagonalization .............................................................................. 177 Bibliography 183 Curriculum Vitae 184 IV CONTENTS Chapter 1 Introduction and Motivation The renormalization of the electroweak Standard Model has already a success­ ful history. In some of its sectors experimental measurements are sensitive to loop corrections and there, calculations with high precision are already mandatory. Sur­ prisingly, there are still open problems related to the renormalization of the quark sector starting with the one-loop corrections. The presence of the quark mixing matrix that needs to be renormalized and the presence of unstable particles raise difficulties in defining correct and complete renormalized parameters that preserve all symmetries of the Lagrangian. Going beyond the Standard Model, one has other models that allow for fermion mixing and there, a complete renormalization scheme is also required. For example, there are experimental evidences for neutrino oscillations and a model that describes the neutrino mixing has to be taken into account. One can also think of supersym ­ metric or other exotic particles. Mixing is present in the Standard Model for Dirac fermions (quarks), while beyond, it can involve also Majorana particles (possible candidates are neutrinos). The necessity of the renormalization for fermion mixing was already recognised in the late '70s [Sirlin]. In 1982, Aoki et al. [Aok82] were describing an on-shell renormalization scheme that led to a diagonal fermion propagator. This prescription was used in 1990 by Denner and Sack [Den90a] to calculate the one-loop counter terms of external legs and of the quark mixing matrix. It was the first attempt to provide an analytical result for a mixing matrix counter term. In the next decade, few articles followed, trying to use a similar prescription to calculate the counter term for quark or neutrino mixing matrices, for models with stable particles. In 1999, in [Gam99], a gauge parameter dependence problem was recognized in the renormalization prescription of [Den90a]. Starting from 2000 on, many authors tried to find a prescription that will have as result a renormalized fermion mixing matrix that is unitary, gauge parameter independent and that will lead to an UV-finite amplitude. These requirements were successfully accomplished for the corrections 1 2 1. Introduction and Motivation to the quark mixing matrix in [Den04], but treating ail quarks as stable particles. The difficult point remains the renormalization of the theory involving unstable particles. In [Esp02], it was shown that a correct on-shell renormalization scheme that accounts for unstable particles and that includes the absorptive contributions from the self-energies leads to wave function renormalization constants not related by hermiticity (i.e. the constant renormalizing the incoming fermion and the outgoing antifermion is different from the one that renormalizes the outgoing fermion and the incoming antifermion). The lack of hermiticity can destroy in this case the unitarity of the renormalized mixing matrix. The aim of this thesis is to provide a renormalization prescription for fermion mixing, in a general framework, a prescription that can be applied then to specific models. We base our calculations on a Lagrange density that describes generic in ­ teraction terms for Dirac and Majorana fermions, in models that allow for mixing. We also take into account the presence of unstable particles. The analysis of the renormalized Lagrangian is general, but the analytic formulas for the
Recommended publications
  • Effective Dirac Equations in Honeycomb Structures
    Effective Dirac equations in honeycomb structures Effective Dirac equations in honeycomb structures Young Researchers Seminar, CERMICS, Ecole des Ponts ParisTech William Borrelli CEREMADE, Universit´eParis Dauphine 11 April 2018 It is self-adjoint on L2(R2; C2) and the spectrum is given by σ(D0) = R; σ(D) = (−∞; −m] [ [m; +1) The domain of the operator and form domain are H1(R2; C2) and 1 2 2 H 2 (R ; C ), respectively. Remark The negative spectrum is associated with antiparticles, in relativistic theories. Effective Dirac equations in honeycomb structures Dirac in 2D The 2D Dirac operator The 2D Dirac operator is defined as D = D0 +mσ3 = −i(σ1@1 + σ2@2) + mσ3: (1) where σk are the Pauli matrices and m ≥ 0 is the mass of the particle. It acts on C2-valued spinors. The domain of the operator and form domain are H1(R2; C2) and 1 2 2 H 2 (R ; C ), respectively. Remark The negative spectrum is associated with antiparticles, in relativistic theories. Effective Dirac equations in honeycomb structures Dirac in 2D The 2D Dirac operator The 2D Dirac operator is defined as D = D0 +mσ3 = −i(σ1@1 + σ2@2) + mσ3: (1) where σk are the Pauli matrices and m ≥ 0 is the mass of the particle. It acts on C2-valued spinors. It is self-adjoint on L2(R2; C2) and the spectrum is given by σ(D0) = R; σ(D) = (−∞; −m] [ [m; +1) Effective Dirac equations in honeycomb structures Dirac in 2D The 2D Dirac operator The 2D Dirac operator is defined as D = D0 +mσ3 = −i(σ1@1 + σ2@2) + mσ3: (1) where σk are the Pauli matrices and m ≥ 0 is the mass of the particle.
    [Show full text]
  • Majorana Fermions in Condensed Matter Physics: the 1D Nanowire Case
    Majorana Fermions in Condensed Matter Physics: The 1D Nanowire Case Philip Haupt, Hirsh Kamakari, Edward Thoeng, Aswin Vishnuradhan Department of Physics and Astronomy, University of British Columbia, Vancouver, B.C., V6T 1Z1, Canada (Dated: November 24, 2018) Majorana fermions are fermions that are their own antiparticles. Although they remain elusive as elementary particles (how they were originally proposed), they have rapidly gained interest in condensed matter physics as emergent quasiparticles in certain systems like topological supercon- ductors. In this article, we briefly review the necessary theory and discuss the \recipe" to create Majorana particles. We then consider existing experimental realisations and their methodologies. I. MOTIVATION A). Kitaev used a simplified quantum wire model to show Ettore Majorana, in 1937, postulated the existence of how Majorana modes might manifest as an emergent an elementary particle which is its own antiparticle, so phenomena, which we will now discuss. Consider 1- called Majorana fermions [1]. It is predicted that the neu- dimensional tight binding chain with spinless fermions trinos are one such elementary particle, which is yet to and p-orbital hopping. The use of unphysical spinless be detected via extremely rare neutrino-less double beta- fermions calls into question the validity of the model, decay. The research on Majorana fermions in the past but, as has been subsequently realised, in the presence few years, however, have gained momentum in the com- of strong spin orbit coupling it is possible for electrons pletely different field of condensed matter physics. Arti- to be approximated as spinless in the presence of spin- ficially engineered low-dimensional nanostructures which orbit coupling as well as a Zeeman field [9].
    [Show full text]
  • $ Z $ Boson Mediated Dark Matter Beyond the Effective Theory
    MCTP-16-27 FERMILAB-PUB-16-534-T Z boson mediated dark matter beyond the effective theory John Kearney Theoretical Physics Department, Fermi National Accelerator Laboratory, Batavia, IL 60510 USA Nicholas Orlofsky and Aaron Pierce Michigan Center for Theoretical Physics (MCTP) Department of Physics, University of Michigan, Ann Arbor, MI 48109 (Dated: April 11, 2017) Direct detection bounds are beginning to constrain a very simple model of weakly interacting dark matter|a Majorana fermion with a coupling to the Z boson. In a particularly straightforward gauge-invariant realization, this coupling is introduced via a higher-dimensional operator. While attractive in its simplicity, this model generically induces a large ρ parameter. An ultraviolet completion that avoids an overly large contribution to ρ is the singlet-doublet model. We revisit this model, focusing on the Higgs blind spot region of parameter space where spin-independent interactions are absent. This model successfully reproduces dark matter with direct detection mediated by the Z boson, but whose cosmology may depend on additional couplings and states. Future direct detection experiments should effectively probe a significant portion of this parameter space, aside from a small coannihilating region. As such, Z-mediated thermal dark matter as realized in the singlet-doublet model represents an interesting target for future searches. I. INTRODUCTION Z, and their spin-dependent (SD) couplings, which at tree level arise from exchange of the Z. The latest bounds on SI scattering arise from PandaX Weakly interacting massive particles (WIMPs) re- [1] and LUX [2]. DM that interacts with the Z main an attractive thermal dark matter (DM) can- boson via vectorial couplings, g (¯χγ χ)Zµ, is very didate.
    [Show full text]
  • 2 Lecture 1: Spinors, Their Properties and Spinor Prodcuts
    2 Lecture 1: spinors, their properties and spinor prodcuts Consider a theory of a single massless Dirac fermion . The Lagrangian is = ¯ i@ˆ . (2.1) L ⇣ ⌘ The Dirac equation is i@ˆ =0, (2.2) which, in momentum space becomes pUˆ (p)=0, pVˆ (p)=0, (2.3) depending on whether we take positive-energy(particle) or negative-energy (anti-particle) solutions of the Dirac equation. Therefore, in the massless case no di↵erence appears in equations for paprticles and anti-particles. Finding one solution is therefore sufficient. The algebra is simplified if we take γ matrices in Weyl repreentation where µ µ 0 σ γ = µ . (2.4) " σ¯ 0 # and σµ =(1,~σ) andσ ¯µ =(1, ~ ). The Pauli matrices are − 01 0 i 10 σ = ,σ= − ,σ= . (2.5) 1 10 2 i 0 3 0 1 " # " # " − # The matrix γ5 is taken to be 10 γ5 = − . (2.6) " 01# We can use the matrix γ5 to construct projection operators on to upper and lower parts of the four-component spinors U and V . The projection operators are 1 γ 1+γ Pˆ = − 5 , Pˆ = 5 . (2.7) L 2 R 2 Let us write u (p) U(p)= L , (2.8) uR(p) ! where uL(p) and uR(p) are two-component spinors. Since µ 0 pµσ pˆ = µ , (2.9) " pµσ¯ 0(p) # andpU ˆ (p) = 0, the two-component spinors satisfy the following (Weyl) equations µ µ pµσ uR(p)=0,pµσ¯ uL(p)=0. (2.10) –3– Suppose that we have a left handed spinor uL(p) that satisfies the Weyl equation.
    [Show full text]
  • The Bound States of Dirac Equation with a Scalar Potential
    THE BOUND STATES OF DIRAC EQUATION WITH A SCALAR POTENTIAL BY VATSAL DWIVEDI THESIS Submitted in partial fulfillment of the requirements for the degree of Master of Science in Applied Mathematics in the Graduate College of the University of Illinois at Urbana-Champaign, 2015 Urbana, Illinois Adviser: Professor Jared Bronski Abstract We study the bound states of the 1 + 1 dimensional Dirac equation with a scalar potential, which can also be interpreted as a position dependent \mass", analytically as well as numerically. We derive a Pr¨ufer-like representation for the Dirac equation, which can be used to derive a condition for the existence of bound states in terms of the fixed point of the nonlinear Pr¨uferequation for the angle variable. Another condition was derived by interpreting the Dirac equation as a Hamiltonian flow on R4 and a shooting argument for the induced flow on the space of Lagrangian planes of R4, following a similar calculation by Jones (Ergodic Theor Dyn Syst, 8 (1988) 119-138). The two conditions are shown to be equivalent, and used to compute the bound states analytically and numerically, as well as to derive a Calogero-like upper bound on the number of bound states. The analytic computations are also compared to the bound states computed using techniques from supersymmetric quantum mechanics. ii Acknowledgments In the eternity that is the grad school, this project has been what one might call an impulsive endeavor. In the 6 months from its inception to its conclusion, it has, without doubt, greatly benefited from quite a few individuals, as well as entities, around me, to whom I owe my sincere regards and gratitude.
    [Show full text]
  • Electrical Probes of the Non-Abelian Spin Liquid in Kitaev Materials
    PHYSICAL REVIEW X 10, 031014 (2020) Electrical Probes of the Non-Abelian Spin Liquid in Kitaev Materials David Aasen,1,2 Roger S. K. Mong,3,4 Benjamin M. Hunt,5,4 David Mandrus ,6,7 and Jason Alicea 8,9 1Microsoft Quantum, Microsoft Station Q, University of California, Santa Barbara, California 93106-6105 USA 2Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106, USA 3Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA 4Pittsburgh Quantum Institute, Pittsburgh, Pennsylvania 15260, USA 5Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213, USA 6Department of Materials Science and Engineering, University of Tennessee, Knoxville, Tennessee 37996, USA 7Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA 8Department of Physics and Institute for Quantum Information and Matter, California Institute of Technology, Pasadena, California 91125, USA 9Walter Burke Institute for Theoretical Physics, California Institute of Technology, Pasadena, California 91125, USA (Received 5 March 2020; revised 12 May 2020; accepted 19 May 2020; published 17 July 2020) Recent thermal-conductivity measurements evidence a magnetic-field-induced non-Abelian spin-liquid phase in the Kitaev material α-RuCl3. Although the platform is a good Mott insulator, we propose experiments that electrically probe the spin liquid’s hallmark chiral Majorana edge state and bulk anyons, including their exotic exchange statistics. We specifically introduce circuits that exploit interfaces between electrically active systems and Kitaev materials to “perfectly” convert electrons from the former into emergent fermions in the latter—thereby enabling variations of transport probes invented for topological superconductors and fractional quantum-Hall states.
    [Show full text]
  • Introduction to Supersymmetry
    Introduction to Supersymmetry Pre-SUSY Summer School Corpus Christi, Texas May 15-18, 2019 Stephen P. Martin Northern Illinois University [email protected] 1 Topics: Why: Motivation for supersymmetry (SUSY) • What: SUSY Lagrangians, SUSY breaking and the Minimal • Supersymmetric Standard Model, superpartner decays Who: Sorry, not covered. • For some more details and a slightly better attempt at proper referencing: A supersymmetry primer, hep-ph/9709356, version 7, January 2016 • TASI 2011 lectures notes: two-component fermion notation and • supersymmetry, arXiv:1205.4076. If you find corrections, please do let me know! 2 Lecture 1: Motivation and Introduction to Supersymmetry Motivation: The Hierarchy Problem • Supermultiplets • Particle content of the Minimal Supersymmetric Standard Model • (MSSM) Need for “soft” breaking of supersymmetry • The Wess-Zumino Model • 3 People have cited many reasons why extensions of the Standard Model might involve supersymmetry (SUSY). Some of them are: A possible cold dark matter particle • A light Higgs boson, M = 125 GeV • h Unification of gauge couplings • Mathematical elegance, beauty • ⋆ “What does that even mean? No such thing!” – Some modern pundits ⋆ “We beg to differ.” – Einstein, Dirac, . However, for me, the single compelling reason is: The Hierarchy Problem • 4 An analogy: Coulomb self-energy correction to the electron’s mass A point-like electron would have an infinite classical electrostatic energy. Instead, suppose the electron is a solid sphere of uniform charge density and radius R. An undergraduate problem gives: 3e2 ∆ECoulomb = 20πǫ0R 2 Interpreting this as a correction ∆me = ∆ECoulomb/c to the electron mass: 15 0.86 10− meters m = m + (1 MeV/c2) × .
    [Show full text]
  • Toward (Finally!) Ruling out Z and Higgs Mediated Dark Matter Models
    IFIC/16-66 FERMILAB-PUB-16-370-A Prepared for submission to JCAP Toward (Finally!) Ruling Out Z and Higgs Mediated Dark Matter Models Miguel Escudero,a;b Asher Berlin,c Dan Hooperb;d;e and Meng-Xiang Lind aInstituto de F´ısicaCorpuscular (IFIC); CSIC-Universitat de Val`encia; Apartado de Correos 22085; E-46071 Valencia; Spain bFermi National Accelerator Laboratory, Center for Particle Astrophysics, Batavia, IL 60510 cUniversity of Chicago, Department of Physics, Chicago, IL 60637 dUniversity of Chicago, Department of Astronomy and Astrophysics, Chicago, IL 60637 eUniversity of Chicago, Kavli Institute for Cosmological Physics, Chicago, IL 60637 E-mail: miguel.escudero@ific.uv.es, [email protected], [email protected], [email protected] Abstract. In recent years, direct detection, indirect detection, and collider experiments have placed increasingly stringent constraints on particle dark matter, exploring much of the parameter space associated with the WIMP paradigm. In this paper, we focus on the subset of WIMP models in which the dark matter annihilates in the early universe through couplings to either the Standard Model Z or the Standard Model Higgs boson. Considering fermionic, scalar, and vector dark matter candidates within a model-independent context, we find that the overwhelming majority of these dark matter candidates are already ruled out by existing experiments. In the case of Z mediated dark matter, the only scenarios that are not currently excluded are those in which the dark matter is a fermion with an axial coupling and with a mass either within a few GeV of the Z resonance (mDM m =2) or ' Z greater than 200 GeV, or with a vector coupling and with mDM > 6 TeV.
    [Show full text]
  • Spin-1/2 Fermions in Quantum Field Theory
    Spin-1/2 fermions in quantum field theory µ First, recall that 4-vectors transform under Lorentz transformations, Λ ν, as p′ µ = Λµ pν, where Λ SO(3,1) satisfies Λµ g Λρ = g .∗ A Lorentz ν ∈ ν µρ λ νλ transformation corresponds to a rotation by θ about an axis nˆ [θ~ θnˆ] and ≡ a boost, ζ~ = vˆ tanh−1 ~v , where ~v is the corresponding velocity. Under the | | same Lorentz transformation, a generic field transforms as: ′ ′ Φ (x )= MR(Λ)Φ(x) , where M exp iθ~·J~ iζ~·K~ are N N representation matrices of R ≡ − − × 1 1 the Lorentz group. Defining J~+ (J~ + iK~ ) and J~− (J~ iK~ ), ≡ 2 ≡ 2 − i j ijk k i j [J± , J±]= iǫ J± , [J± , J∓] = 0 . Thus, the representations of the Lorentz algebra are characterized by (j1,j2), 1 1 where the ji are half-integers. (0, 0) is a scalar and (2, 2) is a four-vector. Of 1 1 interest to us here are the spinor representations (2, 0) and (0, 2). ∗ In our conventions, gµν = diag(1 , −1 , −1 , −1). (1, 0): M = exp i θ~·~σ 1ζ~·~σ , butalso (M −1)T = iσ2M(iσ2)−1 2 −2 − 2 (0, 1): [M −1]† = exp i θ~·~σ + 1ζ~·~σ , butalso M ∗ = iσ2[M −1]†(iσ2)−1 2 −2 2 since (iσ2)~σ(iσ2)−1 = ~σ∗ = ~σT − − Transformation laws of 2-component fields ′ β ξα = Mα ξβ , ′ α −1 T α β ξ = [(M ) ] β ξ , ′† α˙ −1 † α˙ † β˙ ξ = [(M ) ] β˙ ξ , ˙ ξ′† =[M ∗] βξ† .
    [Show full text]
  • Arxiv:1003.1912V2 [Hep-Ph] 30 Jun 2010 Fermion and Complex Vector Boson Dark Matter Are Also Disfavored, Except for Very Specific Choices of Quantum Numbers
    Preprint typeset in JHEP style - HYPER VERSION UMD-PP-10-004 RUNHETC-2010-07 A Classification of Dark Matter Candidates with Primarily Spin-Dependent Interactions with Matter Prateek Agrawal Maryland Center for Fundamental Physics, Department of Physics, University of Maryland, College Park, MD 20742 Zackaria Chacko Maryland Center for Fundamental Physics, Department of Physics, University of Maryland, College Park, MD 20742 Can Kilic Department of Physics and Astronomy, Rutgers University, Piscataway NJ 08854 Rashmish K. Mishra Maryland Center for Fundamental Physics, Department of Physics, University of Maryland, College Park, MD 20742 Abstract: We perform a model-independent classification of Weakly Interacting Massive Particle (WIMP) dark matter candidates that have the property that their scattering off nucleons is dominated by spin-dependent interactions. We study renormalizable theories where the scattering of dark matter is elastic and arises at tree-level. We show that if the WIMP-nucleon cross section is dominated by spin-dependent interactions the natural dark matter candidates are either Majorana fermions or real vector bosons, so that the dark matter particle is its own anti-particle. In such a scenario, scalar dark matter is disfavored. Dirac arXiv:1003.1912v2 [hep-ph] 30 Jun 2010 fermion and complex vector boson dark matter are also disfavored, except for very specific choices of quantum numbers. We further establish that any such theory must contain either new particles close to the weak scale with Standard Model quantum numbers, or alternatively, a Z0 gauge boson with mass at or below the TeV scale. In the region of parameter space that is of interest to current direct detection experiments, these particles naturally lie in a mass range that is kinematically accessible to the Large Hadron Collider (LHC).
    [Show full text]
  • Arxiv:1702.04624V3 [Cond-Mat.Str-El]
    Type-III and IV interacting Weyl points J. Nissinen1 and G.E. Volovik1, 2 1Low Temperature Laboratory, Aalto University, P.O. Box 15100, FI-00076 Aalto, Finland 2Landau Institute for Theoretical Physics, acad. Semyonov av., 1a, 142432, Chernogolovka, Russia (Dated: July 7, 2017) 3+1-dimensional Weyl fermions in interacting systems are described by effective quasi-relativistic µ Green’s functions parametrized by a 16 element matrix eα in an expansion around the Weyl point. µ The matrix eα can be naturally identified as an effective tetrad field for the fermions. The corre- spondence between the tetrad field and an effective quasi-relativistic metric gµν governing the Weyl fermions allows for the possibility to simulate different classes of metric fields emerging in general relativity in interacting Weyl semimetals. According to this correspondence, there can be four types 00 of Weyl fermions, depending on the signs of the components g and g00 of the effective metric. In addition to the conventional type-I fermions with a tilted Weyl cone and type-II fermions with an 00 overtilted Weyl cone for g > 0 and respectively g00 > 0 or g00 < 0, we find additional “type-III” 00 and “type-IV” Weyl fermions with instabilities (complex frequencies) for g < 0 and g00 > 0 or g00 < 0, respectively. While the type-I and type-II Weyl points allow us to simulate the black hole event horizon at an interface where g00 changes sign, the type-III Weyl point leads to effective spacetimes with closed timelike curves. PACS numbers: I. INTRODUCTION Weyl fermions1 are massless fermions whose masslessness (gaplessness) is topologically protected2–5.
    [Show full text]
  • Jhep04(2019)150
    Published for SISSA by Springer Received: January 21, 2019 Revised: March 15, 2019 Accepted: April 16, 2019 Published: April 24, 2019 Variational analysis of low-lying states in supersymmetric Yang-Mills theory JHEP04(2019)150 Sajid Ali,a;b Georg Bergner,c;a Henning Gerber,a Simon Kuberski,a Istvan Montvay,d Gernot M¨unster,a Stefano Piemontee and Philipp Sciorf aInstitute for Theoretical Physics, University of M¨unster, Wilhelm-Klemm-Str. 9, D-48149 M¨unster,Germany bDepartment of Physics, Government College University Lahore, Lahore 54000, Pakistan cInstitute for Theoretical Physics, University of Jena, Max-Wien-Platz 1, D-07743 Jena, Germany dDeutsches Elektronen-Synchrotron DESY, Notkestr. 85, D-22607 Hamburg, Germany eInstitute for Theoretical Physics, University of Regensburg, Universit¨atsstr.31, D-93040 Regensburg, Germany f Faculty of Physics, University of Bielefeld, Universit¨atsstr.25, D-33615 Bielefeld, Germany E-mail: [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected], [email protected] Abstract: We have calculated the masses of bound states numerically in N = 1 su- persymmetric Yang-Mills theory with gauge group SU(2). Using the suitably optimised variational method with an operator basis consisting of smeared Wilson loops and mesonic operators, we are able to obtain the masses of the ground states and first excited states in the scalar, pseudoscalar and spin-½ sectors. Extrapolated to the continuum limit, the corresponding particles appear to be approximately mass degenerate and to fit into the predicted chiral supermultiplets.
    [Show full text]