4 Transformations and Symmetries
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Rotation and Spin and Position Operators in Relativistic Gravity and Quantum Electrodynamics
Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 4 December 2019 doi:10.20944/preprints201912.0044.v1 Peer-reviewed version available at Universe 2020, 6, 24; doi:10.3390/universe6020024 1 Review 2 Rotation and Spin and Position Operators in 3 Relativistic Gravity and Quantum Electrodynamics 4 R.F. O’Connell 5 Department of Physics and Astronomy, Louisiana State University; Baton Rouge, LA 70803-4001, USA 6 Correspondence: [email protected]; 225-578-6848 7 Abstract: First, we examine how spin is treated in special relativity and the necessity of introducing 8 spin supplementary conditions (SSC) and how they are related to the choice of a center-of-mass of a 9 spinning particle. Next, we discuss quantum electrodynamics and the Foldy-Wouthuysen 10 transformation which we note is a position operator identical to the Pryce-Newton-Wigner position 11 operator. The classical version of the operators are shown to be essential for the treatment of 12 classical relativistic particles in general relativity, of special interest being the case of binary 13 systems (black holes/neutron stars) which emit gravitational radiation. 14 Keywords: rotation; spin; position operators 15 16 I.Introduction 17 Rotation effects in relativistic systems involve many new concepts not needed in 18 non-relativistic classical physics. Some of these are quantum mechanical (where the emphasis is on 19 “spin”). Thus, our emphasis will be on quantum electrodynamics (QED) and both special and 20 general relativity. Also, as in [1] , we often use “spin” in the generic sense of meaning “internal” spin 21 in the case of an elementary particle and “rotation” in the case of an elementary particle. -
Chapter 5 ANGULAR MOMENTUM and ROTATIONS
Chapter 5 ANGULAR MOMENTUM AND ROTATIONS In classical mechanics the total angular momentum L~ of an isolated system about any …xed point is conserved. The existence of a conserved vector L~ associated with such a system is itself a consequence of the fact that the associated Hamiltonian (or Lagrangian) is invariant under rotations, i.e., if the coordinates and momenta of the entire system are rotated “rigidly” about some point, the energy of the system is unchanged and, more importantly, is the same function of the dynamical variables as it was before the rotation. Such a circumstance would not apply, e.g., to a system lying in an externally imposed gravitational …eld pointing in some speci…c direction. Thus, the invariance of an isolated system under rotations ultimately arises from the fact that, in the absence of external …elds of this sort, space is isotropic; it behaves the same way in all directions. Not surprisingly, therefore, in quantum mechanics the individual Cartesian com- ponents Li of the total angular momentum operator L~ of an isolated system are also constants of the motion. The di¤erent components of L~ are not, however, compatible quantum observables. Indeed, as we will see the operators representing the components of angular momentum along di¤erent directions do not generally commute with one an- other. Thus, the vector operator L~ is not, strictly speaking, an observable, since it does not have a complete basis of eigenstates (which would have to be simultaneous eigenstates of all of its non-commuting components). This lack of commutivity often seems, at …rst encounter, as somewhat of a nuisance but, in fact, it intimately re‡ects the underlying structure of the three dimensional space in which we are immersed, and has its source in the fact that rotations in three dimensions about di¤erent axes do not commute with one another. -
Lecture 1 – Symmetries & Conservation
LECTURE 1 – SYMMETRIES & CONSERVATION Contents • Symmetries & Transformations • Transformations in Quantum Mechanics • Generators • Symmetry in Quantum Mechanics • Conservations Laws in Classical Mechanics • Parity Messages • Symmetries give rise to conserved quantities . Symmetries & Conservation Laws Lecture 1, page1 Symmetry & Transformations Systems contain Symmetry if they are unchanged by a Transformation . This symmetry is often due to an absence of an absolute reference and corresponds to the concept of indistinguishability . It will turn out that symmetries are often associated with conserved quantities . Transformations may be: Active: Active • Move object • More physical Passive: • Change “description” Eg. Change Coordinate Frame • More mathematical Passive Symmetries & Conservation Laws Lecture 1, page2 We will consider two classes of Transformation: Space-time : • Translations in (x,t) } Poincaré Transformations • Rotations and Lorentz Boosts } • Parity in (x,t) (Reflections) Internal : associated with quantum numbers Translations: x → 'x = x − ∆ x t → 't = t − ∆ t Rotations (e.g. about z-axis): x → 'x = x cos θz + y sin θz & y → 'y = −x sin θz + y cos θz Lorentz (e.g. along x-axis): x → x' = γ(x − βt) & t → t' = γ(t − βx) Parity: x → x' = −x t → t' = −t For physical laws to be useful, they should exhibit a certain generality, especially under symmetry transformations. In particular, we should expect invariance of the laws to change of the status of the observer – all observers should have the same laws, even if the evaluation of measurables is different. Put differently, the laws of physics applied by different observers should lead to the same observations. It is this principle which led to the formulation of Special Relativity. -
Representations of U(2O) and the Value of the Fine Structure Constant
Symmetry, Integrability and Geometry: Methods and Applications Vol. 1 (2005), Paper 028, 8 pages Representations of U(2∞) and the Value of the Fine Structure Constant William H. KLINK Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa, USA E-mail: [email protected] Received September 28, 2005, in final form December 17, 2005; Published online December 25, 2005 Original article is available at http://www.emis.de/journals/SIGMA/2005/Paper028/ Abstract. A relativistic quantum mechanics is formulated in which all of the interactions are in the four-momentum operator and Lorentz transformations are kinematic. Interactions are introduced through vertices, which are bilinear in fermion and antifermion creation and annihilation operators, and linear in boson creation and annihilation operators. The fermion- antifermion operators generate a unitary Lie algebra, whose representations are fixed by a first order Casimir operator (corresponding to baryon number or charge). Eigenvectors and eigenvalues of the four-momentum operator are analyzed and exact solutions in the strong coupling limit are sketched. A simple model shows how the fine structure constant might be determined for the QED vertex. Key words: point form relativistic quantum mechanics; antisymmetric representations of infinite unitary groups; semidirect sum of unitary with Heisenberg algebra 2000 Mathematics Subject Classification: 22D10; 81R10; 81T27 1 Introduction With the exception of QCD and gravitational self couplings, all of the fundamental particle interaction Hamiltonians have the form of bilinears in fermion and antifermion creation and annihilation operators times terms linear in boson creation and annihilation operators. For example QED is a theory bilinear in electron and positron creation and annihilation operators and linear in photon creation and annihilation operators. -
Second Quantization
Chapter 1 Second Quantization 1.1 Creation and Annihilation Operators in Quan- tum Mechanics We will begin with a quick review of creation and annihilation operators in the non-relativistic linear harmonic oscillator. Let a and a† be two operators acting on an abstract Hilbert space of states, and satisfying the commutation relation a,a† = 1 (1.1) where by “1” we mean the identity operator of this Hilbert space. The operators a and a† are not self-adjoint but are the adjoint of each other. Let α be a state which we will take to be an eigenvector of the Hermitian operators| ia†a with eigenvalue α which is a real number, a†a α = α α (1.2) | i | i Hence, α = α a†a α = a α 2 0 (1.3) h | | i k | ik ≥ where we used the fundamental axiom of Quantum Mechanics that the norm of all states in the physical Hilbert space is positive. As a result, the eigenvalues α of the eigenstates of a†a must be non-negative real numbers. Furthermore, since for all operators A, B and C [AB, C]= A [B, C] + [A, C] B (1.4) we get a†a,a = a (1.5) − † † † a a,a = a (1.6) 1 2 CHAPTER 1. SECOND QUANTIZATION i.e., a and a† are “eigen-operators” of a†a. Hence, a†a a = a a†a 1 (1.7) − † † † † a a a = a a a +1 (1.8) Consequently we find a†a a α = a a†a 1 α = (α 1) a α (1.9) | i − | i − | i Hence the state aα is an eigenstate of a†a with eigenvalue α 1, provided a α = 0. -
Angular Momentum 23.1 Classical Description
Physics 342 Lecture 23 Angular Momentum Lecture 23 Physics 342 Quantum Mechanics I Monday, March 31st, 2008 We know how to obtain the energy of Hydrogen using the Hamiltonian op- erator { but given a particular En, there is degeneracy { many n`m(r; θ; φ) have the same energy. What we would like is a set of operators that allow us to determine ` and m. The angular momentum operator L^, and in partic- 2 ular the combination L and Lz provide precisely the additional Hermitian observables we need. 23.1 Classical Description Going back to our Hamiltonian for a central potential, we have p · p H = + U(r): (23.1) 2 m It is clear from the dependence of U on the radial distance only, that angular momentum should be conserved in this setting. Remember the definition: L = r × p; (23.2) and we can write this in indexed notation which is slightly easier to work with using the Levi-Civita symbol, defined as (in three dimensions) 8 < 1 for (ijk) an even permutation of (123). ijk = −1 for an odd permutation (23.3) : 0 otherwise Then we can write 3 3 X X Li = ijk rj pk = ijk rj pk (23.4) j=1 k=1 1 of 9 23.2. QUANTUM COMMUTATORS Lecture 23 where the sum over j and k is implied in the second equality (this is Einstein summation notation). There are three numbers here, Li for i = 1; 2; 3, we associate with Lx, Ly, and Lz, the individual components of angular momentum about the three spatial axes. -
The Homology Theory of the Closed Geodesic Problem
J. DIFFERENTIAL GEOMETRY 11 (1976) 633-644 THE HOMOLOGY THEORY OF THE CLOSED GEODESIC PROBLEM MICHELINE VIGUE-POIRRIER & DENNIS SULLIVAN The problem—does every closed Riemannian manifold of dimension greater than one have infinitely many geometrically distinct periodic geodesies—has received much attention. An affirmative answer is easy to obtain if the funda- mental group of the manifold has infinitely many conjugacy classes, (up to powers). One merely needs to look at the closed curve representations with minimal length. In this paper we consider the opposite case of a finite fundamental group and show by using algebraic calculations and the work of Gromoll-Meyer [2] that the answer is again affirmative if the real cohomology ring of the manifold or any of its covers requires at least two generators. The calculations are based on a method of the second author sketched in [6], and he wishes to acknowledge the motivation provided by conversations with Gromoll in 1967 who pointed out the surprising fact that the available tech- niques of algebraic topology loop spaces, spectral sequences, and so forth seemed inadequate to handle the "rational problem" of calculating the Betti numbers of the space of all closed curves on a manifold. He also acknowledges the help given by John Morgan in understanding what goes on here. The Gromoll-Meyer theorem which uses nongeneric Morse theory asserts the following. Let Λ(M) denote the space of all maps of the circle S1 into M (not based). Then there are infinitely many geometrically distinct periodic geodesies in any metric on M // the Betti numbers of Λ(M) are unbounded. -
Hamilton Equations, Commutator, and Energy Conservation †
quantum reports Article Hamilton Equations, Commutator, and Energy Conservation † Weng Cho Chew 1,* , Aiyin Y. Liu 2 , Carlos Salazar-Lazaro 3 , Dong-Yeop Na 1 and Wei E. I. Sha 4 1 College of Engineering, Purdue University, West Lafayette, IN 47907, USA; [email protected] 2 College of Engineering, University of Illinois at Urbana-Champaign, Urbana, IL 61820, USA; [email protected] 3 Physics Department, University of Illinois at Urbana-Champaign, Urbana, IL 61820, USA; [email protected] 4 College of Information Science and Electronic Engineering, Zhejiang University, Hangzhou 310058, China; [email protected] * Correspondence: [email protected] † Based on the talk presented at the 40th Progress In Electromagnetics Research Symposium (PIERS, Toyama, Japan, 1–4 August 2018). Received: 12 September 2019; Accepted: 3 December 2019; Published: 9 December 2019 Abstract: We show that the classical Hamilton equations of motion can be derived from the energy conservation condition. A similar argument is shown to carry to the quantum formulation of Hamiltonian dynamics. Hence, showing a striking similarity between the quantum formulation and the classical formulation. Furthermore, it is shown that the fundamental commutator can be derived from the Heisenberg equations of motion and the quantum Hamilton equations of motion. Also, that the Heisenberg equations of motion can be derived from the Schrödinger equation for the quantum state, which is the fundamental postulate. These results are shown to have important bearing for deriving the quantum Maxwell’s equations. Keywords: quantum mechanics; commutator relations; Heisenberg picture 1. Introduction In quantum theory, a classical observable, which is modeled by a real scalar variable, is replaced by a quantum operator, which is analogous to an infinite-dimensional matrix operator. -
10 Group Theory and Standard Model
Physics 129b Lecture 18 Caltech, 03/05/20 10 Group Theory and Standard Model Group theory played a big role in the development of the Standard model, which explains the origin of all fundamental particles we see in nature. In order to understand how that works, we need to learn about a new Lie group: SU(3). 10.1 SU(3) and more about Lie groups SU(3) is the group of special (det U = 1) unitary (UU y = I) matrices of dimension three. What are the generators of SU(3)? If we want three dimensional matrices X such that U = eiθX is unitary (eigenvalues of absolute value 1), then X need to be Hermitian (real eigenvalue). Moreover, if U has determinant 1, X has to be traceless. Therefore, the generators of SU(3) are the set of traceless Hermitian matrices of dimension 3. Let's count how many independent parameters we need to characterize this set of matrices (what is the dimension of the Lie algebra). 3 × 3 complex matrices contains 18 real parameters. If it is to be Hermitian, then the number of parameters reduces by a half to 9. If we further impose traceless-ness, then the number of parameter reduces to 8. Therefore, the generator of SU(3) forms an 8 dimensional vector space. We can choose a basis for this eight dimensional vector space as 00 1 01 00 −i 01 01 0 01 00 0 11 λ1 = @1 0 0A ; λ2 = @i 0 0A ; λ3 = @0 −1 0A ; λ4 = @0 0 0A (1) 0 0 0 0 0 0 0 0 0 1 0 0 00 0 −i1 00 0 01 00 0 0 1 01 0 0 1 1 λ5 = @0 0 0 A ; λ6 = @0 0 1A ; λ7 = @0 0 −iA ; λ8 = p @0 1 0 A (2) i 0 0 0 1 0 0 i 0 3 0 0 −2 They are called the Gell-Mann matrices. -
Lecture 8 Symmetries, Conserved Quantities, and the Labeling of States Angular Momentum
Lecture 8 Symmetries, conserved quantities, and the labeling of states Angular Momentum Today’s Program: 1. Symmetries and conserved quantities – labeling of states 2. Ehrenfest Theorem – the greatest theorem of all times (in Prof. Anikeeva’s opinion) 3. Angular momentum in QM ˆ2 ˆ 4. Finding the eigenfunctions of L and Lz - the spherical harmonics. Questions you will by able to answer by the end of today’s lecture 1. How are constants of motion used to label states? 2. How to use Ehrenfest theorem to determine whether the physical quantity is a constant of motion (i.e. does not change in time)? 3. What is the connection between symmetries and constant of motion? 4. What are the properties of “conservative systems”? 5. What is the dispersion relation for a free particle, why are E and k used as labels? 6. How to derive the orbital angular momentum observable? 7. How to check if a given vector observable is in fact an angular momentum? References: 1. Introductory Quantum and Statistical Mechanics, Hagelstein, Senturia, Orlando. 2. Principles of Quantum Mechanics, Shankar. 3. http://mathworld.wolfram.com/SphericalHarmonic.html 1 Symmetries, conserved quantities and constants of motion – how do we identify and label states (good quantum numbers) The connection between symmetries and conserved quantities: In the previous section we showed that the Hamiltonian function plays a major role in our understanding of quantum mechanics using it we could find both the eigenfunctions of the Hamiltonian and the time evolution of the system. What do we mean by when we say an object is symmetric?�What we mean is that if we take the object perform a particular operation on it and then compare the result to the initial situation they are indistinguishable.�When one speaks of a symmetry it is critical to state symmetric with respect to which operation. -
Derivation of the Momentum Operator
Physics H7C May 12, 2019 Derivation of the Momentum Operator c Joel C. Corbo, 2008 This set of notes describes one way of deriving the expression for the position-space representation of the momentum operator in quantum mechanics. First of all, we need to meet a new mathematical friend, the Dirac delta function δ(x − x0), which is defined by its action when integrated against any function f(x): Z 1 δ(x − x0)f(x)dx = f(x0): (1) −∞ In particular, for f(x) = 1, we have Z 1 δ(x − x0)dx = 1: (2) −∞ Speaking roughly, one can say that δ(x−x0) is a \function" that diverges at the point x = x0 but is zero for all other x, such that the \area" under it is 1. We can construct some interesting integrals using the Dirac delta function. For example, using Eq. (1), we find 1 1 Z −ipx 1 −ipy p δ(x − y)e ~ dx = p e ~ : (3) 2π −∞ 2π Notice that this has the form of a Fourier transform: 1 Z 1 F (k) = p f(x)e−ikxdx (4a) 2π −∞ 1 Z 1 f(x) = p F (k)eikxdk; (4b) 2π −∞ where F (k) is the Fourier transform of f(x). This means we can rewrite Eq. (3) as Z 1 1 ip (x−y) e ~ dx = δ(x − y): (5) 2π −∞ 1 Derivation of the Momentum Operator That's enough math; let's start talking physics. The expectation value of the position of a particle, in the position representation (that is, in terms of the position- space wavefunction) is given by Z 1 hxi = ∗(x)x (x)dx: (6) −∞ Similarly, the expectation value of the momentum of a particle, in the momentum representation (that is, in terms of the momentum-space wavefunction) is given by Z 1 hpi = φ∗(p)pφ(p)dp: (7) −∞ Let's try to calculate the expectation value of the momentum of a particle in the position representation (that is, in terms of (x), not φ(p)). -
The Position Operator Revisited Annales De L’I
ANNALES DE L’I. H. P., SECTION A H. BACRY The position operator revisited Annales de l’I. H. P., section A, tome 49, no 2 (1988), p. 245-255 <http://www.numdam.org/item?id=AIHPA_1988__49_2_245_0> © Gauthier-Villars, 1988, tous droits réservés. L’accès aux archives de la revue « Annales de l’I. H. P., section A » implique l’accord avec les conditions générales d’utilisation (http://www.numdam. org/conditions). Toute utilisation commerciale ou impression systématique est constitutive d’une infraction pénale. Toute copie ou impression de ce fichier doit contenir la présente mention de copyright. Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques http://www.numdam.org/ .