Hybrid Dirac Fields

Total Page:16

File Type:pdf, Size:1020Kb

Hybrid Dirac Fields Physics Letters B 567 (2003) 179–183 www.elsevier.com/locate/npe Hybrid Dirac fields O.W. Greenberg Center for Theoretical Physics, Department of Physics, University of Maryland, College Park, MD 20742-4111, USA Received 23 May 2003; accepted 25 June 2003 Editor: H. Georgi Abstract Hybrid Dirac fields are fields that are general superpositions of the annihilation and creation parts of four Dirac spin 1/2 ± fields, ψ( )(x;±m), whose annihilation and creation parts obey the Dirac equation with mass m and mass −m.Wediscuss a specific case of such fields, which has been called “homeotic”. We show for this case, as is true in general for hybrid Dirac fields (except the ordinary fields whose annihilation and creation parts both obey one or the other Dirac equation), that (1) any interacting theory violates both Lorentz covariance and causality, (2) the discrete transformations C,andCPT map the pair ¯ ψh(x) and ψh(x) into fields that are not linear combinations of this pair, and (3) the chiral projections of ψh(x) are sums of the usual Dirac fields with masses m and −m; on these chiral projections C,andCPT are defined in the usual way, their interactions do not violate CPT , and interactions of chiral projections are Lorentz covariant and causal. In short, the main claims concerning “homeotic” fields are incorrect. 2003 Published by Elsevier B.V. 1. Introduction fields. This type of field, with a specific choice given below, was considered in a recent paper by Barenboim Since a spin 1/2 field on which parity is defined can and Lykken [1] (BL) in connection with a proposed obey either of two Dirac equations model of CPT violation for neutrinos. They called their field a “homeotic” field. The purpose of this Let- (i/∂ − m)ψ(x; m) = 0 (1) ter is to study the properties of this type of field which, or for reasons stated above, I prefer to call a “hybrid (i/∂ + m)ψ(x;−m) = 0 (2) Dirac field”. BL proposed their “homeotic” field as a counter-example to my general theorem [2] that inter- and since the positive (annihilation) and negative (cre- acting fields that violate CPT symmetry necessarily ation) frequencies of a free field can be separated in a violate Lorentz covariance. I will show below that the Lorentz covariant way, one can consider a family of BL example does not violate CPT and that their inter- free “hybrid Dirac fields” which, with suitable nor- acting “homeotic” field violates both Lorentz covari- malizations, are linear combinations of the annihila- ance and causality. tion and creation parts of mass m and mass −m Dirac 2. The simplest representation of the BL field is E-mail address: [email protected] (+) (−) (O.W. Greenberg). ψh(x) = ψ (x; m) + ψ (x;−m), (3) 0370-2693/$ – see front matter 2003 Published by Elsevier B.V. doi:10.1016/j.physletb.2003.06.046 180 O.W. Greenberg / Physics Letters B 567 (2003) 179–183 where to be explicit and to establish notation, of the normalizations of the u and v spinors for the −m case may seem strange; however these normaliza- ψ(+)(x;±m) tions are consistent with the anticommutation relation 1 d3p for the −m field, with the positivity of energy (note = b(p,s)u(p,s;±m) 3/2 that the u†u normalization is positive for both the m (2π) 2Ep ± s and −m spinors) and with the relation between m and × − · exp( ip x), (4) −m fields via γ 5 given below. If I had started with − ψ( )(x;±m) the −m field rather than with the m field, I could have 3 chosen gammas so that the −muspinors would have 1 d p † = d (p, s)v(p, s;±m) positive normalization. (2π)3/2 2E p ±s (Other linear combinations of the positive and × exp(ip · x), (5) negative frequency parts of Dirac fields of mass m and − − ψ¯ ( )(x;±m) mass m also fall into the category of hybrid Dirac fields as do the usual Dirac fields, but in this Letter 1 d3p = b†(p, s)u(p,s¯ ;±m) I discuss only the example given above.) I follow the 3/2 (2π) 2Ep 0 = = ±s universal convention, [3,4] and [5], that the p Ep × exp(ip · x), (6) m2 + p2 in spinors is always the positive energy; ψ¯ (+)(x;±m) unfortunately BL violate this convention. 3 To see that my representation of ψh(x) is identical = 1 d p ¯ ;± with the BL field, calculate the anticommutator 3/2 d(p,s)v(p,s m) (2π) 2Ep ± s (+) [ψ (x), ψ¯ (y)]+ = (i/∂ + m) ∆ (x − y) × exp(−ip · x). (7) hα hβ x αβ (−) − (i/∂x − m)αβ ∆ (x − y), + ¯ (−) Note the difference between ψ( ) = ψ and (11) ¯ (+) (+) ψ , etc. To separate ψh(x) into ψ (x; m) (−) where and ψ (x;−m),use[(±i/∂x + m)/2m]ψh(x) = (±) ;± 3 ψ (x m); b(p,s), etc., can then be calculated in (+) = 1 d p − · ∆ (x) 3 exp( ip x), the usual way. The annihilation and creation operators (2π) 2Ep are normalized covariantly, − + ∆( )(x) = ∆( )(−x). (12) [ † ] = − + b(p,s),b (q, t) + 2Epδ(p q)δst, (8) This agrees with (2.14) of BL, (their D(x) = ∆( )(x)), etc., and the spinors obey except that their Dirac indices are transposed; how- ever, this differs from the Dirac result by the sign of (/p ∓ m)u(p, s;±m) = 0, (9) the second term proportional to m, not that of the first (/p ± m)v(p, s;±m) = 0, (10) term, as stated by BL. It is instructive to rewrite this result as with normalizations u(p,¯ s;±m)u(p, t;±m) = [ ¯ ]+ ±2mδst and v(p,s¯ ;±m)v(p, t;±m) =∓2mδst. ψhα(x), ψhβ (y) (1) I chose these normalizations so that going from = (i/∂x )αβ i∆(x − y)+ mδαβ ∆ (x − y), (13) ψ(±)(x;±m) to ψ(±)(x;∓m) is accomplished by = (+) − (−) (1) = (+) + (−) changing the sign of m. (This would not be the case where i∆(x) ∆ ∆ and ∆ ∆ ∆ , since this separates the local and nonlocal terms. if I had chosen uu¯ = δst, for example.) I use the same = (+) ; − (−) ; non-chiral Dirac matrices of [3] and [4] and the same In addition, i/∂ψh(x) m(ψ (x m) ψ (x − creation and annihilation operators for both the m and m)); it is straightforward to check that −m fields. With this choice of gamma matrices, the + − m ψ( )(x; m) − ψ( )(x;−m) muspinors have large upper two components and the − −muspinors have large lower two components, and = im 1 P dt ψh(t , x) (14) vice versa for the v spinors. The reversal of the signs π x0 − t O.W. Greenberg / Physics Letters B 567 (2003) 179–183 181 (provided the integral is defined suitably). Thus the the Lorentz covariance of the time-ordering in the present ψh obeys the equation of motion (2.7) of BL. Dyson series, and the Lorentz invariance of their In agreement with my result [2] and with BL, S-matrix are all incorrect and their interacting theory free, or generalized free, hybrid Dirac fields transform is neither Lorentz covariant nor causal. covariantly. This is connected with the existence of In contrast to my disagreement with the assertions θ(±p0) which exists for timelike momenta, but does concerning equal time commutation relations for the not exist for spacelike momenta. I also agree with BL currents and the Hamiltonian density, I agree with BL that the propagator of their field ψh(x) is not causal; it about the equal time commutation relations for the is also not covariant. chiral projections of the hybrid fields. The agreement From Eq. (1), (2), γ 5ψ(x;±m) obeys the Dirac here is because the chiral projections of the hybrid equation for ψ(x;∓m),soitisusefultoconsiderthe fields are sums of the usual Dirac fields with masses discrete transformation m and −m. These chiral projections are not hybrid (or homeotic) fields at all! M ; M† = ;− = 5 ; ψ(x m) ψ(x m) γ ψ(x m), (15) I agree with BL that parity and time reversal Mψ(x;−m)M† = ψ(x; m) = γ 5ψ(x;−m). (16) are realized in the usual way. BL assert that charge conjugation is realized in a different way than usual. − This shows that the m and m spinors are related This is incorrect. This assertion seems to be based on 5 by γ . the tacit assumption that C and CPT map the pair The calculation of the BL current is particularly ¯ ψh(x) and ψh(x) onto themselves. Unexpectedly, this simple for the space components. The result is is not the case. The discrete transformations C and i j CPT map the terms in ψh(x) into terms that are not J (x), J (y) − ¯ ¯ present in ψh(x) and map the terms in ψh(x) into ¯ i j = ψh(x)γ i/∂x i∆(x − y)γ ψh(y) terms that are not present in ψh(x). ¯ j i Although it is well known, I emphasize that the re- − ψh(y)γ i/∂y i∆(y − x)γ ψh(x) quirement that charge conjugation changes the sign + m −δij [ψ¯ (x)ψ (y) − ψ¯ (y)ψ (x)] h h h h of the field and the requirement that charge conjuga- ¯ ij ¯ ij − i[ψh(x)σ ψh(y) + ψh(y)σ ψh(x)] tion interchanges particle and antiparticle are equiva- lent [6–8]. Here is the standard argument concerning × ∆(1)(x − y). (17) charge conjugation [4].
Recommended publications
  • Part V Appendices a Vector Calculus
    Part V Appendices A Vector calculus It is often useful in physics⎛ ⎞ to describe the position of some object x ⎜ ⎟ using three numbers ⎝y⎠. This is what we call a vector v and de- z note by a little arrow above the letter. The three numbers are the components of the vector along the three coordinate axes. The first number tells us how far the vector in question goes in the x-direction, the second how far in the y-direction⎛ ⎞ and the third how far in the 0 ⎜ ⎟ z-direction. For example, w = ⎝4⎠ is a vector that points exclusively 0 in the y-direction. Vectors can be added ⎛ ⎞ ⎛ ⎞ ⎛ ⎞ v w v + w ⎜ x⎟ ⎜ x⎟ ⎜ x x⎟ = = → + = 1 v ⎝vy⎠ w ⎝wy⎠ v w ⎝vy + wy⎠ (A. ) vz wz vz + wy and multiplied ⎛ ⎞ ⎛ ⎞ v w ⎜ x⎟ ⎜ x⎟ · = · = + + 2 v w ⎝vy⎠ ⎝wy⎠ vxwx vywy vzwz. (A. ) vz wz The result of this multiplication is not a vector, but a number (= a scalar), hence the name: scalar product. The scalar product of a vec- tor with itself is directly related to its length: √ length(v)= v ·v. (A.3) Take note that we can’t simply write three quantities below each other between two brackets and expect it to be a vector. For example, © Springer International Publishing AG 2018 J. Schwichtenberg, Physics from Symmetry, Undergraduate Lecture Notes in Physics, https://doi.org/10.1007/978-3-319-66631-0 256 physics from symmetry let’s say we put the temperature T, the pressure P and the humidity H of a room between two brackets: ⎛ ⎞ T ⎜ ⎟ ⎝ P ⎠ .
    [Show full text]
  • The Chirality-Flow Method for Massive and Electroweak Amplitudes
    LU-TP 20-41 July 2020 The Chirality-Flow Method for Massive and Electroweak Amplitudes Joakim Alnefjord Department of Astronomy and Theoretical Physics, Lund University Master thesis supervised by Malin Sj¨odahl,Christian Reuschle, and Andrew Lifson Abstract In this thesis I extend the chirality-flow method to the full standard model at tree-level by including massive particles and electroweak interactions. The chirality-flow method is a new diagrammatic method for calculating Feynman diagrams that is based on the spinor- helicity formalism, that before this thesis was written had been worked out for massless QED and QCD at tree-level. I summarize what is known about massive spinor-helicity calculations and use this as the basis for the extended diagrammatic interpretation for massive particles. I use the Lorentz structure of the electroweak vertices to rewrite them in the chirality-flow picture. Popul¨arvetenskaplig beskrivning Det finns m˚angav¨agaratt g˚ai jakten efter en b¨attre f¨orst˚aelsef¨orv˚armateriella v¨arlds minsta best˚andsdelar,elementarpartiklarna. Vi kan bygga kraftigare och mer exakta par- tikelacceleratorer och d¨armedf¨orb¨attraden experimentella delen av partikelfysiken. Vi kan ocks˚af¨ors¨oka hitta nya teorier om hur v¨arldenfungerar, n˚agotsom i praktiken ¨ar v¨aldigt komplicerat. Vi kan ist¨alletfokusera p˚asmartare s¨attatt g¨orautr¨akningarinom dagens teoretiska ramar, vilket ¨arvad den h¨ar uppsatsen handlar om. Inom partikelfysiken ¨arvi ofta intresserade av att r¨aknaut s˚akallade ¨overg˚angsamplituder. Dessa kan exempelvis liknas med en sannolikhet att ett visst tillst˚andav partiklar ska ¨overg˚atill ett annat tillst˚andav andra partiklar vid en kollision i partikelacceleratorer.
    [Show full text]
  • Minimal Dark Matter Models with Radiative Neutrino Masses
    Master’s thesis Minimal dark matter models with radiative neutrino masses From Lagrangians to observables Simon May 1st June 2018 Advisors: Prof. Dr. Michael Klasen, Dr. Karol Kovařík Institut für Theoretische Physik Westfälische Wilhelms-Universität Münster Contents 1. Introduction 5 2. Experimental and observational evidence 7 2.1. Dark matter . 7 2.2. Neutrino oscillations . 14 3. Gauge theories and the Standard Model of particle physics 19 3.1. Mathematical background . 19 3.1.1. Group and representation theory . 19 3.1.2. Tensors . 27 3.2. Representations of the Lorentz group . 31 3.2.1. Scalars: The (0, 0) representation . 35 1 1 3.2.2. Weyl spinors: The ( 2 , 0) and (0, 2 ) representations . 36 1 1 3.2.3. Dirac spinors: The ( 2 , 0) ⊕ (0, 2 ) representation . 38 3.2.4. Majorana spinors . 40 1 1 3.2.5. Lorentz vectors: The ( 2 , 2 ) representation . 41 3.2.6. Field representations . 42 3.3. Two-component Weyl spinor formalism and van der Waerden notation 44 3.3.1. Definition . 44 3.3.2. Correspondence to the Dirac bispinor formalism . 47 3.4. The Standard Model . 49 3.4.1. Definition of the theory . 52 3.4.2. The Lagrangian . 54 4. Component notation for representations of SU(2) 57 4.1. SU(2) doublets . 59 4.1.1. Basic conventions and transformation of doublets . 60 4.1.2. Dual doublets and scalar product . 61 4.1.3. Transformation of dual doublets . 62 4.1.4. Adjoint doublets . 63 4.1.5. The question of transpose and conjugate doublets .
    [Show full text]
  • Lecture Notes Introduction to Supersymmetry and Supergravity
    Lecture notes Introduction to Supersymmetry and Supergravity Jan Louis Fachbereich Physik der Universit¨atHamburg, Luruper Chaussee 149, 22761 Hamburg, Germany ABSTRACT These lectures give a basic introduction to supersymmetry and supergravity. Lecture course given at the University of Hamburg, winter term 2015/16 January 25, 2016 Contents 1 The Supersymmetry Algebra 4 1.1 Review of Poincare Algebra . .4 1.2 Representations of the Lorentz Group . .5 1.3 Supersymmetry Algebra . .6 2 Representations of the supersymmetry algebra and the Chiral Multi- plet 7 2.1 Massive representations . .7 2.2 Massless representations . .8 2.3 The chiral multiplet in QFTs . .8 3 Superspace and the Chiral Multiplet 11 3.1 Basic set-up . 11 3.2 Chiral Multiplet . 12 3.3 Berezin integration . 13 3.4 R-symmetry . 14 4 Super Yang-Mills Theories 15 4.1 The Vector Multiplet in Superspace . 15 4.2 Non-Abelian vector multiplets . 17 5 Super YM Theories coupled to matter and the MSSM 18 5.1 Coupling to matter . 18 5.2 The minimal supersymmetric Standard Model (MSSM) . 19 5.2.1 The Spectrum . 19 5.2.2 The Lagrangian . 20 6 Spontaneous Supersymmetry Breaking 22 6.1 Order parameters of supersymmetry breaking . 22 6.2 Models for spontaneous supersymmetry breaking . 22 6.2.1 F-term breaking . 23 6.2.2 D-term breaking . 23 6.3 General considerations . 24 6.3.1 Fermion mass matrix and Goldstone's theorem for supersymmetry 24 6.3.2 Mass sum rules and the supertrace . 25 1 7 Non-renormalizable couplings 27 7.1 Non-linear σ-models .
    [Show full text]
  • Properties of an Alternative Off-Shell Formulation of 4D Supergravity
    S S symmetry Article Properties of an Alternative Off-Shell Formulation of 4D Supergravity Friedemann Brandt Institut für Theoretische Physik, Leibniz Universität Hannover, Appelstraße 2, 30167 Hannover, Germany; [email protected] Abstract: This article elaborates on an off-shell formulation of D = 4, N = 1 supergravity whose auxiliary fields comprise an antisymmetric tensor field without gauge degrees of freedom. In particular, the relation to new minimal supergravity, a supercovariant tensor calculus and the construction of invariant actions including matter fields are discussed. Keywords: supergravity; off-shell formulation; matter couplings; supercovariant tensor calculus; invariant actions; BRST transformations 1. Introduction In the basic formulation [1,2] of pure D = 4, N = 1 supergravity, the commutator algebra of local symmetry transformations closes only on-shell. This complicates various computations, such as the construction of couplings of the supergravity multiplet (i.e., the supersymmetry multiplet with the vierbein and the gravitino) to matter multiplets, of locally supersymmetric invariants with higher derivatives and of Faddeev–Popov terms. Fortunately, there are off-shell formulations of the theory with auxiliary fields that close Citation: Brandt, F. Properties of an the algebra of local symmetry transformations off-shell. Alternative Off-Shell Formulation of The best-known off-shell formulations of pure D = 4, N = 1 supergravity are the 4D Supergravity. Symmetry 2021, 13, so-called old minimal formulation [3,4] and the so-called new minimal formulation [5]. The 620. https://doi.org/10.3390/sym auxiliary fields of the new minimal supergravity multiplet are a real 2-form gauge potential 13040620 and a real vector field which is the gauge field of local R-transformations (“R-gauge field”).
    [Show full text]
  • Properties and Calculations of Multi Parton Processes Properties and Calculations of Multi Parton Processes Properties and Calculations of Multi Parton Processes
    PROPERTIES AND CALCULATIONS OF MULTI PARTON PROCESSES PROPERTIES AND CALCULATIONS OF MULTI PARTON PROCESSES PROPERTIES AND CALCULATIONS OF MULTI PARTON PROCESSES PROEFSCHRIFT TER VERKRIJGING VAN DE GRAAD VAN DOCTOR AAN DE RIJKSUNIVERSITEIT TE LEIDEN, OP GEZAG VAN DE RECTOR MAGNIFICUS DR. J.J.M. BEENAKKER, HOOG- LERAAR IN DE FACULTEIT DER WISKUNDE EN NATUUR- WETENSCHAPPEN, VOLGENS BESLUIT VAN HET COLLE- GE VAN DEKANEN TE VERDEDIGEN OP DONDERDAG 5 OKTOBER 1989 TE KLOKKE 15.15 UUR DOOR WALTER THEO GIELE GEBOREN TE DEN HAAG IN 1957 Promotie-commissie: Promotor : Prof. Dr. F.A. Bcrends Referent : Dr. W.L.G.A.M. van Neerven Overige leden : Prof. Dr. R. de Bruyn Ouboter Prof. Dr. J.M.J. van Leeuwen Prof. Dr. C.J.N. van den Mcijdenbrrg This investigation is part of the research program of the Stichting voor Funda- menteel Onderzoek der Materie (FOM) which is financially supported by the Ne- derlandse Organisatie voor Wctenschappelijk Onderzor-k (NWO). Contents I Outline 1 II Introduction 5 1 The theoretical model 5 2 A historical review of the calculations 9 III The helicity method 15 1 Introduction 15 2 The Weyl-van der Waerden implementation 1G 2.1 The formalism 16 2.2 The momentum vectors 17 2.3 The spin-i particles 19 2.4 The spin-1 particles 20 IV The recursion relations 25 1 Introduction 25 2 The gluon recursion relation 26 3 The spinorial recursion relation 34 4 From currents to amplitudes and cross sections 36 4.1 Scattering of n gluons 36 4.2 The process producing qq and n gluons 38 4.3 The process producing qq, n gluons and a vector boson ..
    [Show full text]
  • On the History of Unified Field Theories
    On the History of Unified Field Theories Hubert F. M. Goenner University of G¨ottingen Institut f¨urTheoretische Physik Tammannstr. 1 D-37077 G¨ottingen Germany email: [email protected] http://www.theorie.physik.uni-goettingen.de/~goenner Accepted on 14 January 2004 Published on 13 February 2004 http://relativity.livingreviews.org/lrr-2004-2 Living Reviews in Relativity Published by the Max Planck Institute for Gravitational Physics Albert Einstein Institute, Germany Abstract This article is intended to give a review of the history of the classical aspects of unified field theories in the 20th century. It includes brief technical descriptions of the theories suggested, short biographical notes concerning the scientists involved, and an extensive bibliography. The present first installment covers the time span between 1914 and 1933, i.e., when Einstein was living and working in Berlin – with occasional digressions into other periods. Thus, the main theme is the unification of the electromagnetic and gravitational fields augmented by short- lived attempts to include the matter field described by Schr¨odinger’s or Dirac’s equations. While my focus lies on the conceptual development of the field, by also paying attention to the interaction of various schools of mathematicians with the research done by physicists, some prosopocraphical remarks are included. c Max Planck Society and the authors. Further information on copyright is given at http://relativity.livingreviews.org/Info/Copyright/ For permission to reproduce the article please contact [email protected]. Article Amendments On author request a Living Reviews article can be amended to include errata and small additions to ensure that the most accurate and up-to-date information possible is provided.
    [Show full text]
  • Algebraic Solution for the Vector Potential in the Dirac Equation
    March 2001 UTAS-PHYS-01-02 Algebraic solution for the vector potential in the Dirac equation H S Booth∗, GLegg, PDJarvis School of Mathematics and Physics, University of Tasmania GPO Box 252-21, Hobart Tas 7001, Australia Abstract The Dirac equation for an electron in an external electromagnetic field can be regarded as a singular set of linear equations for the vector potential. Radford’s method of al- gebraically solving for the vector potential is reviewed, with attention to the additional constraints arising from non-maximality of the rank. The extension of the method to gen- arXiv:hep-th/0104216v1 25 Apr 2001 eral spacetimes is illustrated by examples in diverse dimensions with both c- and a-number wavefunctions. ∗Centre for Mathematics and its Applications, Australian National University. [email protected] 1 Introduction The Maxwell-Dirac equations are the coupled nonlinear partial differential equations which describe a classical electron interacting with an electromagnetic field. They are also the equations from which quantum electrodynamics is derived. Since the mathemat- ical foundations of the latter remain unclear, the Maxwell-Dirac equations continue to be of interest [1, 2, 3]. Recently Radford[4] handled the Maxwell-Dirac equations firstly by solving the Dirac equation for the electromagnetic potential in terms of the wavefunction and its derivatives, and then substituting this solution in the Maxwell equations. This approach subsequently led to some physically interesting results[5, 6, 7] (for a review see [8]). Despite the viability and potential importance of Radford’s algebraic solution, at least for the treatment of the equations of classical electrodynamics for electrons and photons, it appears that the method has not before appeared in this context.
    [Show full text]
  • Theory Heavy Quanta
    THEORY OF HEAVY QUANTA DOOR F. J. BELINFANTE «KOMT» ’S-GRAVENHAGE MARTINÜS NIJHOFF 1939 HR! BIBLIOTHEEK Universiteit Leiden GORLAEUS LABORATORIA 1 395 219 2 Postbus 9502 2300 RA LEIDEN Tel.: 071 -527 43 66 / 67 . 1 I t clcssëjfbcxb<jUs» THEORY OF HEAVY QUANTA PROEFSCHRIFT . L E I D E N THEORY OF HEAVY QUANTA PROEFSCHRIFT TER VERKRIJGING VAN DEN GRAAD VAN DOCTOR IN DE WIS- EN NATUURKUNDE AAN DE RIJKSUNIVER­ SITEIT TE LEIDEN, OP GEZAG VAN DEN RECTOR MAGNIFICUS D r FRED. MULLER, HOOGLEERAAR IN DE FACULTEIT DER LETTEREN EN WIJSBEGEERTE, VOOR DE FACULTEIT DER WIS- EN NATUURKUNDE TE VERDEDIGEN OP DINSDAG 10 OCTOBER 1939, DES NAMIDDAGS TE 4 UUR DOOR FREDERIK JOZEF BELINFANTE GEBOREN TE ’S-GRAVENHAGE ’S-GRAVENHAGE MARTINUS NIJHOFF 1939 'R .U N IV T (Bibliotheek) HEIDEN, PRINTED IN THE NETHERLANDS AAN MIJN OUDERS AAN MIJN VROUW CONTENTS VOORWOORD.............................................................................. XI CHAPTER I. UNDOR CALCULUS AND CHARGE-CONJUGATION. Zusammenfassung. Resumo .......................................... 1 § 1. Introduction........................................ 1 § 2. The Dirac wave-function (undor of the first rank). 2 § 3. Charge-conjugation of four-spinors....................... 7 § 4. Neutrettors of the first rank ........................ 10 § 5. Undors of the second r a n k ................................... 12 § 6. Covariant undor calculus .......... .......... 16 R eferences.................. 21 CHAPTER II. THE UNDOR EQUATION OF THE MESON FIELD. Zusammenfassung. Resum o..............................................22 § 1. The P r o c a-K emmer meson equation in undor n o ta tio n ............................................. 22 § 2. The generalized meson equation and the neutretto eq u atio n ....................................................................... 26 § 3. The charge-conjugated meson equation.................. 28 § 4. The charge current-density and the magnetic moment of mesons......................................................................29 § 5.
    [Show full text]
  • Counterpart of the Weyl Tensor for Rarita–Schwinger Type Fields
    Physics Letters B 767 (2017) 347–349 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Counterpart of the Weyl tensor for Rarita–Schwinger type fields Friedemann Brandt Institut für Theoretische Physik, Leibniz Universität Hannover, Appelstraße 2, 30167 Hannover, Germany a r t i c l e i n f o a b s t r a c t Article history: In dimensions larger than 3 a modified field strength for Rarita–Schwinger type fields is constructed Received 20 December 2016 whose components are not constrained by the field equations. In supergravity theories the result provides Received in revised form 19 January 2017 a modified (supercovariant) gravitino field strength related by supersymmetry to the (supercovariantized) Accepted 23 January 2017 Weyl tensor. In various cases, such as for free Rarita–Schwinger type gauge fields and for gravitino Available online 16 February 2017 fields in several supergravity theories, the modified field strength coincides on-shell with the usual field Editor: M. Cveticˇ strength. A corresponding result for first order derivatives of Dirac type spinor fields is also presented. © 2017 The Author. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3. This note relates to Rarita–Schwinger type fields in D dimen- fields of supersymmetry transformations and are termed gravitino sions with D > 3. The components of these fields are denoted by fields. The supersymmetry transformation of a gravitino field is ψ α where m = 1, ..., D is a vector index and α = 1, ..., 2 D/2 m α = α + is a spinor index, D/2 being the largest integer ≤ D/2.
    [Show full text]
  • Majorana Particles in Physics and Mathematics
    Majorana particles in physics and mathematics Hidde Hendriksen Centre for Theoretical Physics & Johann Bernoulli Institute Rijksuniversiteit Groningen A thesis submitted for the degree of Bachelor Physics and Mathematics June 2014 Abstract In 1937, the Italian physicist Ettore Majorana showed that there exist real solutions to the Dirac equation. This suggests the existence of the Majorana fermion, a neutral fermion that is equal to its antiparticle. Up until now, no Majorana fermions have been found. Recent developments in solid state physics have led to evidence that so-called Majorana zero modes can exist in superconductors. Sometimes these quasiparticles are also confusingly named \Majorana fermions". These modes or quasipar- ticles show some resemblance with the real Majorana fermions, however they are two completely different physical phenomena. This article math- ematically describes the differences between these two concepts by the use of different Clifford algebras. For the description of the Majorana spinor a Clifford algebra is used that satisfies a pseudo-Euclidean metric, appli- cable in a selection of space-time dimensions. The Majorana zero mode is described by a Clifford algebra that satisfies a purely Euclidean metric in the abstract space of zero modes. Furthermore the statistics of both entities is described, where Fermi-Dirac statistics applies to the Majorana fermion and non-Abelian anyonic statistics applies to the Majorana zero modes. Contents 1 The relation between the Dirac equation and the Clifford algebra 1 1.1 Constructing the Dirac equation . .1 1.1.1 The Schr¨odingerequation . .1 1.1.2 The Klein-Gordon equation . .2 1.1.3 The Dirac equation .
    [Show full text]
  • FERMILAB-PUB-96/445-T INTRODUCTION to SUPERSYMMETRY 1 Introduction “Never Mind, Lads. Same Time Tomorrow. We Must Get a Winner
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server FERMILAB-PUB-96/445-T INTRODUCTION TO SUPERSYMMETRY JOSEPH D. LYKKEN Fermi National Accelerator Laboratory P.O. Box 500 Batavia, IL 60510 These lectures give a self-contained introduction to supersymmetry from a modern perspective. Emphasis is placed on material essential to understanding duality. Topics include: central charges and BPS-saturated states, supersymmetric nonlin- ear sigma models, N=2 Yang-Mills theory, holomorphy and the N=2 Yang-Mills β function, supersymmetry in 2, 6, 10, and 11 spacetime dimensions. 1 Introduction “Never mind, lads. Same time tomorrow. We must get a winner one day.” – Peter Cook, as the doomsday prophet in “The End of the World”. Supersymmetry, along with its monozygotic sibling superstring theory, has become the dominant framework for formulating physics beyond the standard model. This despite the fact that, as of this morning, there is no unambiguous experimental evidence for either idea. Theorists find supersymmetry appealing for reasons which are both phenomenological and technical. In these lectures I will focus exclusively on the technical appeal. There are many good recent re- views of the phenomenology of supersymmetry. 1 Some good technical reviews are Wess and Bagger, 2 West, 3 and Sohnius. 4 The goal of these lectures is to provide the student with the technical back- ground requisite for the recent applications of duality ideas to supersymmetric gauge theories and superstrings. More specifically, if you absorb the material in these lectures, you will understand Section 2 of Seiberg and Witten, 5 and you will have a vague notion of why there might be such a thing as M-theory.
    [Show full text]