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Can We Rule out the Possibility of the Existence of an Additional Time Axis
Brian D. Koberlein Thomas J. Murray Time 2 ABSTRACT CAN WE RULE OUT THE POSSIBILITY THAT THERE IS MORE THAN ONE DIRECTION IN TIME? by Lynn Stephens The literature was examined to see if a proposal for the existence of additional time-like axes could be falsified. Some naïve large-time models are visualized and examined from the standpoint of simplicity and adequacy. Although the conclusion here is that the existence of additional time-like dimensions has not been ruled out, the idea is probably not falsifiable, as was first assumed. The possibility of multiple times has been dropped from active consideration by theorists less because of negative evidence than because it can lead to cumbersome models that introduce causality problems without providing any advantages over other models. Even though modern philosophers have made intriguing suggestions concerning the causality issue, usability and usefulness issues remain. Symmetry considerations from special relativity and from the conservation laws are used to identify restrictions on large-time models. In view of recent experimental findings, further research into Cramer’s transactional model is indicated. This document contains embedded graphic (.png and .jpg) and Apple Quick Time (.mov) files. The CD-ROM contains interactive Pacific Tech Graphing Calculator (.gcf) files. Time 3 NOTE TO THE READER The graphics in the PDF version of this document rely heavily on the use of color and will not print well in black and white. The CD-ROM attachment that comes with the paper version of this document includes: • The full-color PDF with QuickTime animation; • A PDF printable in black and white; • The original interactive Graphing Calculator files. -
Introductory Lectures on Quantum Field Theory
Introductory Lectures on Quantum Field Theory a b L. Álvarez-Gaumé ∗ and M.A. Vázquez-Mozo † a CERN, Geneva, Switzerland b Universidad de Salamanca, Salamanca, Spain Abstract In these lectures we present a few topics in quantum field theory in detail. Some of them are conceptual and some more practical. They have been se- lected because they appear frequently in current applications to particle physics and string theory. 1 Introduction These notes are based on lectures delivered by L.A.-G. at the 3rd CERN–Latin-American School of High- Energy Physics, Malargüe, Argentina, 27 February–12 March 2005, at the 5th CERN–Latin-American School of High-Energy Physics, Medellín, Colombia, 15–28 March 2009, and at the 6th CERN–Latin- American School of High-Energy Physics, Natal, Brazil, 23 March–5 April 2011. The audience on all three occasions was composed to a large extent of students in experimental high-energy physics with an important minority of theorists. In nearly ten hours it is quite difficult to give a reasonable introduction to a subject as vast as quantum field theory. For this reason the lectures were intended to provide a review of those parts of the subject to be used later by other lecturers. Although a cursory acquaintance with the subject of quantum field theory is helpful, the only requirement to follow the lectures is a working knowledge of quantum mechanics and special relativity. The guiding principle in choosing the topics presented (apart from serving as introductions to later courses) was to present some basic aspects of the theory that present conceptual subtleties. -
Clifford Algebra and the Interpretation of Quantum
In: J.S.R. Chisholm/A.K. Commons (Eds.), Cliord Algebras and their Applications in Mathematical Physics. Reidel, Dordrecht/Boston (1986), 321–346. CLIFFORD ALGEBRA AND THE INTERPRETATION OF QUANTUM MECHANICS David Hestenes ABSTRACT. The Dirac theory has a hidden geometric structure. This talk traces the concep- tual steps taken to uncover that structure and points out signicant implications for the interpre- tation of quantum mechanics. The unit imaginary in the Dirac equation is shown to represent the generator of rotations in a spacelike plane related to the spin. This implies a geometric interpreta- tion for the generator of electromagnetic gauge transformations as well as for the entire electroweak gauge group of the Weinberg-Salam model. The geometric structure also helps to reveal closer con- nections to classical theory than hitherto suspected, including exact classical solutions of the Dirac equation. 1. INTRODUCTION The interpretation of quantum mechanics has been vigorously and inconclusively debated since the inception of the theory. My purpose today is to call your attention to some crucial features of quantum mechanics which have been overlooked in the debate. I claim that the Pauli and Dirac algebras have a geometric interpretation which has been implicit in quantum mechanics all along. My aim will be to make that geometric interpretation explicit and show that it has nontrivial implications for the physical interpretation of quantum mechanics. Before getting started, I would like to apologize for what may appear to be excessive self-reference in this talk. I have been pursuing the theme of this talk for 25 years, but the road has been a lonely one where I have not met anyone travelling very far in the same direction. -
Simulating Physics with Computers
International Journal of Theoretical Physics, VoL 21, Nos. 6/7, 1982 Simulating Physics with Computers Richard P. Feynman Department of Physics, California Institute of Technology, Pasadena, California 91107 Received May 7, 1981 1. INTRODUCTION On the program it says this is a keynote speech--and I don't know what a keynote speech is. I do not intend in any way to suggest what should be in this meeting as a keynote of the subjects or anything like that. I have my own things to say and to talk about and there's no implication that anybody needs to talk about the same thing or anything like it. So what I want to talk about is what Mike Dertouzos suggested that nobody would talk about. I want to talk about the problem of simulating physics with computers and I mean that in a specific way which I am going to explain. The reason for doing this is something that I learned about from Ed Fredkin, and my entire interest in the subject has been inspired by him. It has to do with learning something about the possibilities of computers, and also something about possibilities in physics. If we suppose that we know all the physical laws perfectly, of course we don't have to pay any attention to computers. It's interesting anyway to entertain oneself with the idea that we've got something to learn about physical laws; and if I take a relaxed view here (after all I'm here and not at home) I'll admit that we don't understand everything. -
Dirac Notation Frank Rioux
Elements of Dirac Notation Frank Rioux In the early days of quantum theory, P. A. M. (Paul Adrian Maurice) Dirac created a powerful and concise formalism for it which is now referred to as Dirac notation or bra-ket (bracket ) notation. Two major mathematical traditions emerged in quantum mechanics: Heisenberg’s matrix mechanics and Schrödinger’s wave mechanics. These distinctly different computational approaches to quantum theory are formally equivalent, each with its particular strengths in certain applications. Heisenberg’s variation, as its name suggests, is based matrix and vector algebra, while Schrödinger’s approach requires integral and differential calculus. Dirac’s notation can be used in a first step in which the quantum mechanical calculation is described or set up. After this is done, one chooses either matrix or wave mechanics to complete the calculation, depending on which method is computationally the most expedient. Kets, Bras, and Bra-Ket Pairs In Dirac’s notation what is known is put in a ket, . So, for example, p expresses the fact that a particle has momentum p. It could also be more explicit: p = 2 , the particle has momentum equal to 2; x = 1.23 , the particle has position 1.23. Ψ represents a system in the state Q and is therefore called the state vector. The ket can also be interpreted as the initial state in some transition or event. The bra represents the final state or the language in which you wish to express the content of the ket . For example,x =Ψ.25 is the probability amplitude that a particle in state Q will be found at position x = .25. -
What Is the Dirac Equation?
What is the Dirac equation? M. Burak Erdo˘gan ∗ William R. Green y Ebru Toprak z July 15, 2021 at all times, and hence the model needs to be first or- der in time, [Tha92]. In addition, it should conserve In the early part of the 20th century huge advances the L2 norm of solutions. Dirac combined the quan- were made in theoretical physics that have led to tum mechanical notions of energy and momentum vast mathematical developments and exciting open operators E = i~@t, p = −i~rx with the relativis- 2 2 2 problems. Einstein's development of relativistic the- tic Pythagorean energy relation E = (cp) + (E0) 2 ory in the first decade was followed by Schr¨odinger's where E0 = mc is the rest energy. quantum mechanical theory in 1925. Einstein's the- Inserting the energy and momentum operators into ory could be used to describe bodies moving at great the energy relation leads to a Klein{Gordon equation speeds, while Schr¨odinger'stheory described the evo- 2 2 2 4 lution of very small particles. Both models break −~ tt = (−~ ∆x + m c ) : down when attempting to describe the evolution of The Klein{Gordon equation is second order, and does small particles moving at great speeds. In 1927, Paul not have an L2-conservation law. To remedy these Dirac sought to reconcile these theories and intro- shortcomings, Dirac sought to develop an operator1 duced the Dirac equation to describe relativitistic quantum mechanics. 2 Dm = −ic~α1@x1 − ic~α2@x2 − ic~α3@x3 + mc β Dirac's formulation of a hyperbolic system of par- tial differential equations has provided fundamental which could formally act as a square root of the Klein- 2 2 2 models and insights in a variety of fields from parti- Gordon operator, that is, satisfy Dm = −c ~ ∆ + 2 4 cle physics and quantum field theory to more recent m c . -
A Tale of Three Equations: Breit, Eddington-Gaunt, and Two-Body
View metadata, citation and similarA Tale papers of at Three core.ac.uk Equations: Breit, Eddington-Gaunt, and Two-Body Dirac brought to you by CORE Peter Van Alstine provided by CERN Document Server 12474 Sunny Glenn Drive, Moorpark, Ca. 90125 Horace W. Crater The University of Tennessee Space Institute Tullahoma,Tennessee 37388 G.Breit’s original paper of 1929 postulates the Breit equation as a correction to an earlier defective equation due to Eddington and Gaunt, containing a form of interaction suggested by Heisenberg and Pauli. We observe that manifestly covariant electromagnetic Two-Body Dirac equations previously obtained by us in the framework of Relativistic Constraint Mechanics reproduce the spectral results of the Breit equation but through an interaction structure that contains that of Eddington and Gaunt. By repeating for our equation the analysis that Breit used to demonstrate the superiority of his equation to that of Eddington and Gaunt, we show that the historically unfamiliar interaction structures of Two-Body Dirac equations (in Breit-like form) are just what is needed to correct the covariant Eddington Gaunt equation without resorting to Breit’s version of retardation. 1 I. INTRODUCTION Three score and seven years ago, Gregory Breit extended Dirac’s spin-1/2 wave equation to a system of two charged particles [1]. He formed his equation by summing two free-particle Dirac Hamiltonians with an interaction obtained by substituting Dirac α~’s for velocities in the semi-relativistic electrodynamic interaction of Darwin:. α 1 EΨ= α~ ·p~ +β m +α~ ·p~ +β m − [1 − (α~ · α~ + α~ · r~ˆ α ·rˆ)] Ψ. -
5 the Dirac Equation and Spinors
5 The Dirac Equation and Spinors In this section we develop the appropriate wavefunctions for fundamental fermions and bosons. 5.1 Notation Review The three dimension differential operator is : ∂ ∂ ∂ = , , (5.1) ∂x ∂y ∂z We can generalise this to four dimensions ∂µ: 1 ∂ ∂ ∂ ∂ ∂ = , , , (5.2) µ c ∂t ∂x ∂y ∂z 5.2 The Schr¨odinger Equation First consider a classical non-relativistic particle of mass m in a potential U. The energy-momentum relationship is: p2 E = + U (5.3) 2m we can substitute the differential operators: ∂ Eˆ i pˆ i (5.4) → ∂t →− to obtain the non-relativistic Schr¨odinger Equation (with = 1): ∂ψ 1 i = 2 + U ψ (5.5) ∂t −2m For U = 0, the free particle solutions are: iEt ψ(x, t) e− ψ(x) (5.6) ∝ and the probability density ρ and current j are given by: 2 i ρ = ψ(x) j = ψ∗ ψ ψ ψ∗ (5.7) | | −2m − with conservation of probability giving the continuity equation: ∂ρ + j =0, (5.8) ∂t · Or in Covariant notation: µ µ ∂µj = 0 with j =(ρ,j) (5.9) The Schr¨odinger equation is 1st order in ∂/∂t but second order in ∂/∂x. However, as we are going to be dealing with relativistic particles, space and time should be treated equally. 25 5.3 The Klein-Gordon Equation For a relativistic particle the energy-momentum relationship is: p p = p pµ = E2 p 2 = m2 (5.10) · µ − | | Substituting the equation (5.4), leads to the relativistic Klein-Gordon equation: ∂2 + 2 ψ = m2ψ (5.11) −∂t2 The free particle solutions are plane waves: ip x i(Et p x) ψ e− · = e− − · (5.12) ∝ The Klein-Gordon equation successfully describes spin 0 particles in relativistic quan- tum field theory. -
Arxiv:Hep-Ph/9412261V1 8 Dec 1994
IPNO/TH 94-85 How to obtain a covariant Breit type equation from relativistic Constraint Theory J. Mourad Laboratoire de Mod`eles de Physique Math´ematique, Universit´ede Tours, Parc de Grandmont, F-37200 Tours, France H. Sazdjian Division de Physique Th´eorique∗, Institut de Physique Nucl´eaire, Universit´eParis XI, F-91406 Orsay Cedex, France arXiv:hep-ph/9412261v1 8 Dec 1994 October 1994 ∗Unit´ede Recherche des Universit´es Paris 11 et Paris 6 associ´ee au CNRS. 1 Abstract It is shown that, by an appropriate modification of the structure of the interaction po- tential, the Breit equation can be incorporated into a set of two compatible manifestly covariant wave equations, derived from the general rules of Constraint Theory. The com- plementary equation to the covariant Breit type equation determines the evolution law in the relative time variable. The interaction potential can be systematically calculated in perturbation theory from Feynman diagrams. The normalization condition of the Breit wave function is determined. The wave equation is reduced, for general classes of poten- tial, to a single Pauli-Schr¨odinger type equation. As an application of the covariant Breit type equation, we exhibit massless pseudoscalar bound state solutions, corresponding to a particular class of confining potentials. PACS numbers : 03.65.Pm, 11.10.St, 12.39.Ki. 2 1 Introduction Historically, The Breit equation [1] represents the first attempt to describe the relativistic dynamics of two interacting fermion systems. It consists in summing the free Dirac hamiltonians of the two fermions and adding mutual and, eventually, external potentials. This equation, when applied to QED, with one-photon exchange diagram considered in the Coulomb gauge, and solved in the linearized approximation, provides the correct spectra to order α4 [1, 2] for various bound state problems. -
THE DIRAC OPERATOR 1. First Properties 1.1. Definition. Let X Be A
THE DIRAC OPERATOR AKHIL MATHEW 1. First properties 1.1. Definition. Let X be a Riemannian manifold. Then the tangent bundle TX is a bundle of real inner product spaces, and we can form the corresponding Clifford bundle Cliff(TX). By definition, the bundle Cliff(TX) is a vector bundle of Z=2-graded R-algebras such that the fiber Cliff(TX)x is just the Clifford algebra Cliff(TxX) (for the inner product structure on TxX). Definition 1. A Clifford module on X is a vector bundle V over X together with an action Cliff(TX) ⊗ V ! V which makes each fiber Vx into a module over the Clifford algebra Cliff(TxX). Suppose now that V is given a connection r. Definition 2. The Dirac operator D on V is defined in local coordinates by sending a section s of V to X Ds = ei:rei s; for feig a local orthonormal frame for TX and the multiplication being Clifford multiplication. It is easy to check that this definition is independent of the coordinate system. A more invariant way of defining it is to consider the composite of differential operators (1) V !r T ∗X ⊗ V ' TX ⊗ V,! Cliff(TX) ⊗ V ! V; where the first map is the connection, the second map is the isomorphism T ∗X ' TX determined by the Riemannian structure, the third map is the natural inclusion, and the fourth map is Clifford multiplication. The Dirac operator is clearly a first-order differential operator. We can work out its symbol fairly easily. The symbol1 of the connection r is ∗ Sym(r)(v; t) = iv ⊗ t; v 2 Vx; t 2 Tx X: All the other differential operators in (1) are just morphisms of vector bundles. -
P-Dirac Operators Craig A. Nolder Department of Mathematics, Florida State University, Tallahassee, Florida 32306-4510, USA
p-Dirac Operators Craig A. Nolder Department of Mathematics, Florida State University, Tallahassee, Florida 32306-4510, USA and John Ryan Department of Mathematics, University of Arkansas, Fayetteville, AR 72701, USA Abstract We introduce non-linear Dirac operators in Rn associated to the p-harmonic equation and we extend to other contexts including spin manifolds and the sphere. 1 Introduction Associated to each type of Laplacian one usually sees a first order lineariza- tion, to a Dirac operator. For instance associated to the Laplacian in Rn is the euclidean Dirac operator arising in Clifford analysis. For the Laplace- Beltrami operator associated to a Riemannian manifold there is the Hodge- Dirac operator d + d!, where d is the exterior derivative and d! is the Hodge codifferential which is the formal adjoint to d. Further, in reverse order, to the Atiyah-Singer-Dirac operator on a spin manifold there is the spinorial Laplacian. Also on Sn one has a conformal Dirac operator and the conformal Laplacian. See for instance [3, 5, 9, 11] for details. Besides the Laplacian in Rn there are also the non-linear operators re- ferred to as p-Laplacians. See for instance [7, 8, 10]. Despite being non-linear these second order operators posses properties very similar to the usual Lapla- cian in euclidean space. Further when p = 2 this operator corresponds to the usual Laplacian in euclidean space. Here we shall introduce a first order nonlinear differential operator which in the case p = 2 coincides with the euclidean Dirac operator. The confor- mal covariance of these operators are established. -
Solvable Two-Body Dirac Equation As a Potential Model of Light Mesons?
Symmetry, Integrability and Geometry: Methods and Applications SIGMA 4 (2008), 048, 19 pages Solvable Two-Body Dirac Equation as a Potential Model of Light Mesons? Askold DUVIRYAK Institute for Condensed Matter Physics of National Academy of Sciences of Ukraine, 1 Svientsitskii Str., UA–79011 Lviv, Ukraine E-mail: [email protected] Received October 29, 2007, in final form May 07, 2008; Published online May 30, 2008 Original article is available at http://www.emis.de/journals/SIGMA/2008/048/ Abstract. The two-body Dirac equation with general local potential is reduced to the pair of ordinary second-order differential equations for radial components of a wave function. The class of linear + Coulomb potentials with complicated spin-angular structure is found, for which the equation is exactly solvable. On this ground a relativistic potential model of light mesons is constructed and the mass spectrum is calculated. It is compared with experimental data. Key words: two body Dirac equation; Dirac oscillator; solvable model; Regge trajectories 2000 Mathematics Subject Classification: 81Q05; 34A05 1 Introduction It is well known that light meson spectra are structured into Regge trajectories which are approximately linear and degenerated due to a weak dependence of masses of resonances on their spin state. These features are reproduced well within the exactly solvable simple relativistic oscillator model (SROM) [1, 2, 3] describing two Klein–Gordon particles harmonically bound. Actually, mesons consist of quarks, i.e., spin-1/2 constituents. Thus potential models based on the Dirac equation are expected to be more appropriate for mesons spectroscopy. In recent years the two body Dirac equations (2BDE) in different formulations1 with various confining potentials are used as a relativistic constituent quark models [16, 17, 18, 19, 20, 21, 22, 23, 24, 25, 26].