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Representations of Certain Semidirect Product Groups* H
JOURNAL OF FUNCTIONAL ANALYSIS 19, 339-372 (1975) Representations of Certain Semidirect Product Groups* JOSEPH A. WOLF Department of Mathematics, University of California, Berkeley, California 94720 Communicated by the Editovs Received April I, 1974 We study a class of semidirect product groups G = N . U where N is a generalized Heisenberg group and U is a generalized indefinite unitary group. This class contains the Poincare group and the parabolic subgroups of the simple Lie groups of real rank 1. The unitary representations of G and (in the unimodular cases) the Plancherel formula for G are written out. The problem of computing Mackey obstructions is completely avoided by realizing the Fock representations of N on certain U-invariant holomorphic cohomology spaces. 1. INTRODUCTION AND SUMMARY In this paper we write out the irreducible unitary representations for a type of semidirect product group that includes the Poincare group and the parabolic subgroups of simple Lie groups of real rank 1. If F is one of the four finite dimensional real division algebras, the corresponding groups in question are the Np,Q,F . {U(p, 4; F) xF+}, where FP~*: right vector space F”+Q with hermitian form h(x, y) = i xiyi - y xipi ) 1 lJ+1 N p,p,F: Im F + F”q* with (w. , ~o)(w, 4 = (w, + 7.0+ Im h(z, ,4, z. + 4, U(p, Q; F): unitary group of Fp,q, F+: subgroup of the group generated by F-scalar multiplication on Fp>*. * Research partially supported by N.S.F. Grant GP-16651. 339 Copyright 0 1975 by Academic Press, Inc. -
SPINORS and SPACE–TIME ANISOTROPY
Sergiu Vacaru and Panayiotis Stavrinos SPINORS and SPACE{TIME ANISOTROPY University of Athens ————————————————— c Sergiu Vacaru and Panyiotis Stavrinos ii - i ABOUT THE BOOK This is the first monograph on the geometry of anisotropic spinor spaces and its applications in modern physics. The main subjects are the theory of grav- ity and matter fields in spaces provided with off–diagonal metrics and asso- ciated anholonomic frames and nonlinear connection structures, the algebra and geometry of distinguished anisotropic Clifford and spinor spaces, their extension to spaces of higher order anisotropy and the geometry of gravity and gauge theories with anisotropic spinor variables. The book summarizes the authors’ results and can be also considered as a pedagogical survey on the mentioned subjects. ii - iii ABOUT THE AUTHORS Sergiu Ion Vacaru was born in 1958 in the Republic of Moldova. He was educated at the Universities of the former URSS (in Tomsk, Moscow, Dubna and Kiev) and reveived his PhD in theoretical physics in 1994 at ”Al. I. Cuza” University, Ia¸si, Romania. He was employed as principal senior researcher, as- sociate and full professor and obtained a number of NATO/UNESCO grants and fellowships at various academic institutions in R. Moldova, Romania, Germany, United Kingdom, Italy, Portugal and USA. He has published in English two scientific monographs, a university text–book and more than hundred scientific works (in English, Russian and Romanian) on (super) gravity and string theories, extra–dimension and brane gravity, black hole physics and cosmolgy, exact solutions of Einstein equations, spinors and twistors, anistoropic stochastic and kinetic processes and thermodynamics in curved spaces, generalized Finsler (super) geometry and gauge gravity, quantum field and geometric methods in condensed matter physics. -
SEMISIMPLE WEAKLY SYMMETRIC PSEUDO–RIEMANNIAN MANIFOLDS 1. Introduction There Have Been a Number of Important Extensions of Th
SEMISIMPLE WEAKLY SYMMETRIC PSEUDO{RIEMANNIAN MANIFOLDS ZHIQI CHEN AND JOSEPH A. WOLF Abstract. We develop the classification of weakly symmetric pseudo{riemannian manifolds G=H where G is a semisimple Lie group and H is a reductive subgroup. We derive the classification from the cases where G is compact, and then we discuss the (isotropy) representation of H on the tangent space of G=H and the signature of the invariant pseudo{riemannian metric. As a consequence we obtain the classification of semisimple weakly symmetric manifolds of Lorentz signature (n − 1; 1) and trans{lorentzian signature (n − 2; 2). 1. Introduction There have been a number of important extensions of the theory of riemannian symmetric spaces. Weakly symmetric spaces, introduced by A. Selberg [8], play key roles in number theory, riemannian geometry and harmonic analysis. See [11]. Pseudo{riemannian symmetric spaces, including semisimple symmetric spaces, play central but complementary roles in number theory, differential geometry and relativity, Lie group representation theory and harmonic analysis. Much of the activity there has been on the Lorentz cases, which are of particular interest in physics. Here we study the classification of weakly symmetric pseudo{ riemannian manifolds G=H where G is a semisimple Lie group and H is a reductive subgroup. We apply the result to obtain explicit listings for metrics of riemannian (Table 5.1), lorentzian (Table 5.2) and trans{ lorentzian (Table 5.3) signature. The pseudo{riemannian symmetric case was analyzed extensively in the classical paper of M. Berger [1]. Our analysis in the weakly symmetric setting starts with the classifications of Kr¨amer[6], Brion [2], Mikityuk [7] and Yakimova [16, 17] for the weakly symmetric riemannian manifolds. -
SUPERSYMMETRY 1. Introduction the Purpose
SUPERSYMMETRY JOSH KANTOR 1. Introduction The purpose of these notes is to give a short and (overly?)simple description of supersymmetry for Mathematicians. Our description is far from complete and should be thought of as a first pass at the ideas that arise from supersymmetry. Fundamental to supersymmetry is the mathematics of Clifford algebras and spin groups. We will describe the mathematical results we are using but we refer the reader to the references for proofs. In particular [4], [1], and [5] all cover spinors nicely. 2. Spin and Clifford Algebras We will first review the definition of spin, spinors, and Clifford algebras. Let V be a vector space over R or C with some nondegenerate quadratic form. The clifford algebra of V , l(V ), is the algebra generated by V and 1, subject to the relations v v = v, vC 1, or equivalently v w + w v = 2 v, w . Note that elements of· l(V ) !can"b·e written as polynomials· in V · and this! giv"es a splitting l(V ) = l(VC )0 l(V )1. Here l(V )0 is the set of elements of l(V ) which can bCe writtenC as a linear⊕ C combinationC of products of even numbers ofCvectors from V , and l(V )1 is the set of elements which can be written as a linear combination of productsC of odd numbers of vectors from V . Note that more succinctly l(V ) is just the quotient of the tensor algebra of V by the ideal generated by v vC v, v 1. -
Should Metric Signature Matter in Clifford Algebra Formulations Of
Should Metric Signature Matter in Clifford Algebra Formulations of Physical Theories? ∗ William M. Pezzaglia Jr. † Department of Physics Santa Clara University Santa Clara, CA 95053 John J. Adams ‡ P.O. Box 808, L-399 Lawrence Livermore National Laboratory Livermore, CA 94550 February 4, 2008 Abstract Standard formulation is unable to distinguish between the (+++−) and (−−−+) spacetime metric signatures. However, the Clifford algebras associated with each are inequivalent, R(4) in the first case (real 4 by 4 matrices), H(2) in the latter (quaternionic 2 by 2). Multivector reformu- lations of Dirac theory by various authors look quite inequivalent pending the algebra assumed. It is not clear if this is mere artifact, or if there is a right/wrong choice as to which one describes reality. However, recently it has been shown that one can map from one signature to the other using a tilt transformation[8]. The broader question is that if the universe is arXiv:gr-qc/9704048v1 17 Apr 1997 signature blind, then perhaps a complete theory should be manifestly tilt covariant. A generalized multivector wave equation is proposed which is fully signature invariant in form, because it includes all the components of the algebra in the wavefunction (instead of restricting it to half) as well as all the possibilities for interaction terms. Summary of talk at the Special Session on Octonions and Clifford Algebras, at the 1997 Spring Western Sectional Meeting of the American Mathematical Society, Oregon State University, Corvallis, OR, 19-20 April 1997. ∗anonymous ftp://www.clifford.org/clf-alg/preprints/1995/pezz9502.latex †Email: [email protected] or [email protected] ‡Email: [email protected] 1 I. -
Pure Spinor Helicity Methods
Pure Spinor Helicity Methods Rutger Boels Niels Bohr International Academy, Copenhagen R.B., arXiv:0908.0738 [hep-th] Rutger Boels (NBIA) Pure Spinor Helicity Methods 15th String Workshop, Zürich 1 / 25 in books? Why you should pay attention, an experiment The greatest common denominator of the audience? Rutger Boels (NBIA) Pure Spinor Helicity Methods 15th String Workshop, Zürich 2 / 25 Why you should pay attention, an experiment The greatest common denominator of the audience in books? Rutger Boels (NBIA) Pure Spinor Helicity Methods 15th String Workshop, Zürich 2 / 25 Why you should pay attention, an experiment The greatest common denominator of the audience in books: Rutger Boels (NBIA) Pure Spinor Helicity Methods 15th String Workshop, Zürich 2 / 25 Why you should pay attention, an experiment The greatest common denominator of the audience in science books? Rutger Boels (NBIA) Pure Spinor Helicity Methods 15th String Workshop, Zürich 2 / 25 for all legs simultaneously pure spinor helicity methods: precise control over Poincaré and Susy quantum numbers Why you should pay attention subject: calculation of scattering amplitudes in D > 4 with many legs Rutger Boels (NBIA) Pure Spinor Helicity Methods 15th String Workshop, Zürich 3 / 25 for all legs simultaneously Why you should pay attention subject: calculation of scattering amplitudes in D > 4 with many legs pure spinor helicity methods: precise control over Poincaré and Susy quantum numbers Rutger Boels (NBIA) Pure Spinor Helicity Methods 15th String Workshop, Zürich 3 / 25 Why you -
The Dirac Equation in General Relativity, a Guide for Calculations
The Dirac equation in general relativity A guide for calculations Peter Collas1 and David Klein2 (September 7, 2018) Abstract In these informal lecture notes we outline different approaches used in doing calculations involving the Dirac equation in curved spacetime. We have tried to clarify the subject by carefully pointing out the various con- ventions used and by including several examples from textbooks and the existing literature. In addition some basic material has been included in the appendices. It is our hope that graduate students and other re- searchers will find these notes useful. arXiv:1809.02764v1 [gr-qc] 8 Sep 2018 1Department of Physics and Astronomy, California State University, Northridge, Northridge, CA 91330-8268. Email: [email protected]. 2Department of Mathematics and Interdisciplinary Research Institute for the Sci- ences, California State University, Northridge, Northridge, CA 91330-8313. Email: [email protected]. Contents 1 The spinorial covariant derivative3 1.1 The Fock-Ivanenko coefficients . .3 1.2 The Ricci rotation coefficient approach . .8 1.3 The electromagnetic interaction . .9 1.4 The Newman-Penrose formalism . 10 2 Examples 14 2.1 Schwarzschild spacetime N-P . 14 2.2 Schwarzschild spacetime F-I . 16 2.3 Nonfactorizable metric . 18 2.4 de Sitter spacetime, Fermi coordinates . 19 3 The Dirac equation in (1+1) GR 23 3.1 Introduction to (1+1) . 23 3.2 The Dirac equation in the Milne universe . 24 4 Scalar product 28 4.1 Conservation of j in SR . 28 4.2 The current density in GR . 29 4.3 The Scalar product in SR . -
Clifford Algebras and Spinors∗
Bulg. J. Phys. 38 (2011) 3–28 This paper is dedicated to the memory of Matey Mateev, a missing friend Clifford Algebras and Spinors∗ I. Todorov1,2, 1Institute for Nuclear Research and Nuclear Energy, Tsarigradsko Chaussee 72, BG-1784 Sofia, Bulgaria (permanent address) 2Theory Group, Physics Department, CERN, CH-1211 Geneva 23, Switzerland Received 9 March 2011 Abstract. Expository notes on Clifford algebras and spinors with a detailed discussion of Majorana, Weyl, and Dirac spinors. The paper is meant as a re- view of background material, needed, in particular, in now fashionable theoret- ical speculations on neutrino masses. It has a more mathematical flavour than the over twenty-six-year-old Introduction to Majorana masses [1] and includes historical notes and biographical data on past participants in the story. PACS codes: 03.65.Fd, 04.20.Gz 1 Quaternions, Grassmann and Clifford Algebras Clifford’s1 paper [2] on “geometric algebra” (published a year before his death) had two sources: Grassmann’s2 algebra and Hamilton’s3 quaternions whose ∗Lectures presented at the University of Sofia in October-November, 2010. Lecture notes pre- pared together with Dimitar Nedanovski (e-mail: [email protected]) and completed dur- ing the stay of the author at the ICTP, Trieste and at CERN, Geneva. 1William Kingdon Clifford (1845-1879) early appreciated the work of Lobachevsky and Rie- mann; he was the first to translate into English Riemann’s inaugural lecture On the hypotheses which lie at the bases of geometry. His view of the physical world as variation of curvature of space antici- pated Einstein’s general theory of relativity. -
The Unitary Representations of the Poincaré Group in Any Spacetime Dimension Abstract Contents
SciPost Physics Lecture Notes Submission The unitary representations of the Poincar´egroup in any spacetime dimension X. Bekaert1, N. Boulanger2 1 Institut Denis Poisson, Unit´emixte de Recherche 7013, Universit´ede Tours, Universit´e d'Orl´eans,CNRS, Parc de Grandmont, 37200 Tours (France) [email protected] 2 Service de Physique de l'Univers, Champs et Gravitation, Universit´ede Mons, UMONS Research Institute for Complex Systems, Place du Parc 20, 7000 Mons (Belgium) [email protected] December 31, 2020 1 Abstract 2 An extensive group-theoretical treatment of linear relativistic field equations 3 on Minkowski spacetime of arbitrary dimension D > 3 is presented. An exhaus- 4 tive treatment is performed of the two most important classes of unitary irre- 5 ducible representations of the Poincar´egroup, corresponding to massive and 6 massless fundamental particles. Covariant field equations are given for each 7 unitary irreducible representation of the Poincar´egroup with non-negative 8 mass-squared. 9 10 Contents 11 1 Group-theoretical preliminaries 2 12 1.1 Universal covering of the Lorentz group 2 13 1.2 The Poincar´egroup and algebra 3 14 1.3 ABC of unitary representations 4 15 2 Elementary particles as unitary irreducible representations of the isom- 16 etry group 5 17 3 Classification of the unitary representations 7 18 3.1 Induced representations 7 19 3.2 Orbits and stability subgroups 8 20 3.3 Classification 10 21 4 Tensorial representations and Young diagrams 12 22 4.1 Symmetric group 12 23 4.2 General linear -
Post-Linear Metric of a Compact Source of Matter
Post-linear metric of a compact source of matter Sven Zschocke Institute of Planetary Geodesy - Lohrmann Observatory, Dresden Technical University, Helmholtzstrasse 10, D-01069 Dresden, Germany The Multipolar Post-Minkowskian (MPM) formalism represents an approach for determining the metric density in the exterior of a compact source of matter. In the MPM formalism the metric density is given in harmonic coordinates and in terms of symmetric tracefree (STF) multipoles. In this investigation, the post-linear metric density of this formalism is used in order to determine the post-linear metric tensor in the exterior of a compact source of matter. The metric tensor is given in harmonic coordinates and in terms of STF multipoles. The post-linear metric coefficients are associated with an integration procedure. The integration of these post-linear metric coefficients is performed explicitly for the case of a stationary source, where the first multipoles (monopole and quadrupole) of the source are taken into account. These studies are a requirement for further investigations in the theory of light propagation aiming at highly precise astrometric measurements in the solar system, where the post-linear coefficients of the metric tensor of solar system bodies become relevant. I. INTRODUCTION Our motivation to consider the post-linear term in the metric perturbation (2) is triggered by the rapid progress The field equations of gravity [1, 2] represent a set in astrometric science, which has recently made the im- of ten coupled non-linear partial differential equations pressive advancement from the milli-arcsecond level [14{ 16] to the micro-arcsecond level [17{21] in angular mea- for the ten components of the metric tensor gαβ which governs the geometry of space-time. -
Hidden Exceptional Symmetry in the Pure Spinor Superstring
PHYSICAL REVIEW D 101, 026006 (2020) Hidden exceptional symmetry in the pure spinor superstring † R. Eager,1,* G. Lockhart,2, and E. Sharpe 3 1Kishine Koen, Yokohama 222-0034, Japan 2Institute for Theoretical Physics, University of Amsterdam, 1098 XH Amsterdam, The Netherlands 3Department of Physics, Virginia Tech, Blacksburg, Virginia 24061, USA (Received 12 November 2019; published 6 January 2020) The pure spinor formulation of superstring theory includes an interacting sector of central charge cλ ¼ 22, which can be realized as a curved βγ system on the cone over the orthogonal Grassmannian þ OG ð5; 10Þ. We find that the spectrum of the βγ system organizes into representations of the g ¼ e6 affine algebra at level −3, whose soð10Þ−3 ⊕ uð1Þ−4 subalgebra encodes the rotational and ghost symmetries of the system. As a consequence, the pure spinor partition function decomposes as a sum of affine e6 characters. We interpret this as an instance of a more general pattern of enhancements in curved βγ systems, which also includes the cases g ¼ soð8Þ and e7, corresponding to target spaces that are cones over the complex Grassmannian Grð2; 4Þ and the complex Cayley plane OP2. We identify these curved βγ systems with the chiral algebras of certain two-dimensional (2D) (0,2) conformal field theories arising from twisted compactification of 4D N ¼ 2 superconformal field theories on S2. DOI: 10.1103/PhysRevD.101.026006 I. INTRODUCTION Nevertheless, we find that the ghost sector partition function [2] can be expressed as a linear combination of The pure spinor formalism [1] is a reformulation of ðeˆ6Þ affine characters, superstring theory which has the virtue that it can be −3 ðˆ Þ ðˆ Þ quantized while preserving manifest covariance with Z ¼ χˆ e6 −3 − χˆ e6 −3 : ð2Þ respect to ten-dimensional super-Poincar´e symmetry. -
Twistors, Generalizations and Exceptional Structures
Twistors, Generalizations and Exceptional Structures Rold˜ao da Rocha∗ Jayme Vaz, Jr.† Abstract This paper is intended to describe twistors via the paravector model of Clifford algebras and to relate such description to conformal maps in the Clifford algebra over R4,1, besides pointing out some applications of the pure spinor formalism. We construct twistors in Minkowski spacetime as algebraic spinors associated with the Dirac-Clifford algebra C ⊗ Cℓ1,3 using one lower spacetime dimension than standard Clifford algebra formulations, since for this purpose the Clifford algebra over R4,1 is also used to describe conformal maps, instead of R2,4. It is possible to identify, via the pure spinor formalism, the twistor fiber in four, six and eight dimensions, respectively, with the coset 1 3 spaces SO(4)/(SU(2) × U(1)/Z2) ≃ CP , SO(6)/(SU(3) × U(1)/Z2) ≃ CP and SO(8)/(Spin(6) × Spin(2)/Z2). The last homogeneous space is closely re- lated to the SO(8) spinor decomposition preserving SO(8) symmetry in type IIB superstring theory. Indeed, aside the IIB superstring theory, there is no SO(8) spinor decomposition preserving SO(8) symmetry and, in this case, one can introduce distinct coordinates and conjugate momenta only if the Spin(8) symmetry is broken by a Spin(6)× Spin(2) subgroup of Spin(8). Also, it is re- viewed how to generalize the Penrose flagpole, illustrating the use of the pure arXiv:math-ph/0412037v2 25 Feb 2005 spinor formalism to construct a flagpole that is more general than the Pen- rose one, which arises when a defined parameter goes to zero.