The Relation Between Classical and Quantum Electrodynamics
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Hendrik Antoon Lorentz's Struggle with Quantum Theory A. J
Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Archive for History of Exact Sciences ISSN 0003-9519 Volume 67 Number 2 Arch. Hist. Exact Sci. (2013) 67:149-170 DOI 10.1007/s00407-012-0107-8 1 23 Your article is published under the Creative Commons Attribution license which allows users to read, copy, distribute and make derivative works, as long as the author of the original work is cited. You may self- archive this article on your own website, an institutional repository or funder’s repository and make it publicly available immediately. 1 23 Arch. Hist. Exact Sci. (2013) 67:149–170 DOI 10.1007/s00407-012-0107-8 Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Received: 15 June 2012 / Published online: 24 July 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract A historical overview is given of the contributions of Hendrik Antoon Lorentz in quantum theory. Although especially his early work is valuable, the main importance of Lorentz’s work lies in the conceptual clarifications he provided and in his critique of the foundations of quantum theory. 1 Introduction The Dutch physicist Hendrik Antoon Lorentz (1853–1928) is generally viewed as an icon of classical, nineteenth-century physics—indeed, as one of the last masters of that era. Thus, it may come as a bit of a surprise that he also made important contribu- tions to quantum theory, the quintessential non-classical twentieth-century develop- ment in physics. The importance of Lorentz’s work lies not so much in his concrete contributions to the actual physics—although some of his early work was ground- breaking—but rather in the conceptual clarifications he provided and his critique of the foundations and interpretations of the new ideas. -
Quantum Field Theory*
Quantum Field Theory y Frank Wilczek Institute for Advanced Study, School of Natural Science, Olden Lane, Princeton, NJ 08540 I discuss the general principles underlying quantum eld theory, and attempt to identify its most profound consequences. The deep est of these consequences result from the in nite number of degrees of freedom invoked to implement lo cality.Imention a few of its most striking successes, b oth achieved and prosp ective. Possible limitation s of quantum eld theory are viewed in the light of its history. I. SURVEY Quantum eld theory is the framework in which the regnant theories of the electroweak and strong interactions, which together form the Standard Mo del, are formulated. Quantum electro dynamics (QED), b esides providing a com- plete foundation for atomic physics and chemistry, has supp orted calculations of physical quantities with unparalleled precision. The exp erimentally measured value of the magnetic dip ole moment of the muon, 11 (g 2) = 233 184 600 (1680) 10 ; (1) exp: for example, should b e compared with the theoretical prediction 11 (g 2) = 233 183 478 (308) 10 : (2) theor: In quantum chromo dynamics (QCD) we cannot, for the forseeable future, aspire to to comparable accuracy.Yet QCD provides di erent, and at least equally impressive, evidence for the validity of the basic principles of quantum eld theory. Indeed, b ecause in QCD the interactions are stronger, QCD manifests a wider variety of phenomena characteristic of quantum eld theory. These include esp ecially running of the e ective coupling with distance or energy scale and the phenomenon of con nement. -
Unification of the Maxwell- Einstein-Dirac Correspondence
Unification of the Maxwell- Einstein-Dirac Correspondence The Origin of Mass, Electric Charge and Magnetic Spin Author: Wim Vegt Country: The Netherlands Website: http://wimvegt.topworld.center Email: [email protected] Calculations: All Calculations in Mathematica 11.0 have been printed in a PDF File Index 1 “Unified 4-Dimensional Hyperspace 5 Equilibrium” beyond Einstein 4-Dimensional, Kaluza-Klein 5-Dimensional and Superstring 10- and 11 Dimensional Curved Hyperspaces 1.2 The 4th term in the Unified 4-Dimensional 12 Hyperspace Equilibrium Equation 1.3 The Impact of Gravity on Light 15 2.1 EM Radiation within a Cartesian Coordinate 23 System in the absence of Gravity 2.1.1 Laser Beam with a Gaussian division in the x-y 25 plane within a Cartesian Coordinate System in the absence of Gravity 2.2 EM Radiation within a Cartesian Coordinate 27 System under the influence of a Longitudinal Gravitational Field g 2.3 The Real Light Intensity of the Sun, measured in 31 our Solar System, including Electromagnetic Gravitational Conversion (EMGC) 2.4 The Boundaries of our Universe 35 2.5 The Origin of Dark Matter 37 3 Electromagnetic Radiation within a Spherical 40 Coordinate System 4 Confined Electromagnetic Radiation within a 42 Spherical Coordinate System through Electromagnetic-Gravitational Interaction 5 The fundamental conflict between Causality and 48 Probability 6 Confined Electromagnetic Radiation within a 51 Toroidal Coordinate System 7 Confined Electromagnetic Radiation within a 54 Toroidal Coordinate System through Electromagnetic-Gravitational -
The Emergence of a Classical World in Bohmian Mechanics
The Emergence of a Classical World in Bohmian Mechanics Davide Romano Lausanne, 02 May 2014 Structure of QM • Physical state of a quantum system: - (normalized) vector in Hilbert space: state-vector - Wavefunction: the state-vector expressed in the coordinate representation Structure of QM • Physical state of a quantum system: - (normalized) vector in Hilbert space: state-vector; - Wavefunction: the state-vector expressed in the coordinate representation; • Physical properties of the system (Observables): - Observable ↔ hermitian operator acting on the state-vector or the wavefunction; - Given a certain operator A, the quantum system has a definite physical property respect to A iff it is an eigenstate of A; - The only possible measurement’s results of the physical property corresponding to the operator A are the eigenvalues of A; - Why hermitian operators? They have a real spectrum of eigenvalues → the result of a measurement can be interpreted as a physical value. Structure of QM • In the general case, the state-vector of a system is expressed as a linear combination of the eigenstates of a generic operator that acts upon it: 퐴 Ψ = 푎 Ψ1 + 푏|Ψ2 • When we perform a measure of A on the system |Ψ , the latter randomly collapses or 2 2 in the state |Ψ1 with probability |푎| or in the state |Ψ2 with probability |푏| . Structure of QM • In the general case, the state-vector of a system is expressed as a linear combination of the eigenstates of a generic operator that acts upon it: 퐴 Ψ = 푎 Ψ1 + 푏|Ψ2 • When we perform a measure of A on the system |Ψ , the latter randomly collapses or 2 2 in the state |Ψ1 with probability |푎| or in the state |Ψ2 with probability |푏| . -
Aspects of Loop Quantum Gravity
Aspects of loop quantum gravity Alexander Nagen 23 September 2020 Submitted in partial fulfilment of the requirements for the degree of Master of Science of Imperial College London 1 Contents 1 Introduction 4 2 Classical theory 12 2.1 The ADM / initial-value formulation of GR . 12 2.2 Hamiltonian GR . 14 2.3 Ashtekar variables . 18 2.4 Reality conditions . 22 3 Quantisation 23 3.1 Holonomies . 23 3.2 The connection representation . 25 3.3 The loop representation . 25 3.4 Constraints and Hilbert spaces in canonical quantisation . 27 3.4.1 The kinematical Hilbert space . 27 3.4.2 Imposing the Gauss constraint . 29 3.4.3 Imposing the diffeomorphism constraint . 29 3.4.4 Imposing the Hamiltonian constraint . 31 3.4.5 The master constraint . 32 4 Aspects of canonical loop quantum gravity 35 4.1 Properties of spin networks . 35 4.2 The area operator . 36 4.3 The volume operator . 43 2 4.4 Geometry in loop quantum gravity . 46 5 Spin foams 48 5.1 The nature and origin of spin foams . 48 5.2 Spin foam models . 49 5.3 The BF model . 50 5.4 The Barrett-Crane model . 53 5.5 The EPRL model . 57 5.6 The spin foam - GFT correspondence . 59 6 Applications to black holes 61 6.1 Black hole entropy . 61 6.2 Hawking radiation . 65 7 Current topics 69 7.1 Fractal horizons . 69 7.2 Quantum-corrected black hole . 70 7.3 A model for Hawking radiation . 73 7.4 Effective spin-foam models . -
Quantum Mechanics As a Limiting Case of Classical Mechanics
View metadata, citation and similar papers at core.ac.uk brought to you by CORE Quantum Mechanics As A Limiting Case provided by CERN Document Server of Classical Mechanics Partha Ghose S. N. Bose National Centre for Basic Sciences Block JD, Sector III, Salt Lake, Calcutta 700 091, India In spite of its popularity, it has not been possible to vindicate the conven- tional wisdom that classical mechanics is a limiting case of quantum mechan- ics. The purpose of the present paper is to offer an alternative point of view in which quantum mechanics emerges as a limiting case of classical mechanics in which the classical system is decoupled from its environment. PACS no. 03.65.Bz 1 I. INTRODUCTION One of the most puzzling aspects of quantum mechanics is the quantum measurement problem which lies at the heart of all its interpretations. With- out a measuring device that functions classically, there are no ‘events’ in quantum mechanics which postulates that the wave function contains com- plete information of the system concerned and evolves linearly and unitarily in accordance with the Schr¨odinger equation. The system cannot be said to ‘possess’ physical properties like position and momentum irrespective of the context in which such properties are measured. The language of quantum mechanics is not that of realism. According to Bohr the classicality of a measuring device is fundamental and cannot be derived from quantum theory. In other words, the process of measurement cannot be analyzed within quantum theory itself. A simi- lar conclusion also follows from von Neumann’s approach [1]. -
On the Definition of the Renormalization Constants in Quantum Electrodynamics
On the Definition of the Renormalization Constants in Quantum Electrodynamics Autor(en): Källén, Gunnar Objekttyp: Article Zeitschrift: Helvetica Physica Acta Band(Jahr): 25(1952) Heft IV Erstellt am: Mar 18, 2014 Persistenter Link: http://dx.doi.org/10.5169/seals-112316 Nutzungsbedingungen Mit dem Zugriff auf den vorliegenden Inhalt gelten die Nutzungsbedingungen als akzeptiert. Die angebotenen Dokumente stehen für nicht-kommerzielle Zwecke in Lehre, Forschung und für die private Nutzung frei zur Verfügung. Einzelne Dateien oder Ausdrucke aus diesem Angebot können zusammen mit diesen Nutzungsbedingungen und unter deren Einhaltung weitergegeben werden. Die Speicherung von Teilen des elektronischen Angebots auf anderen Servern ist nur mit vorheriger schriftlicher Genehmigung möglich. Die Rechte für diese und andere Nutzungsarten der Inhalte liegen beim Herausgeber bzw. beim Verlag. Ein Dienst der ETH-Bibliothek Rämistrasse 101, 8092 Zürich, Schweiz [email protected] http://retro.seals.ch On the Definition of the Renormalization Constants in Quantum Electrodynamics by Gunnar Källen.*) Swiss Federal Institute of Technology, Zürich. (14.11.1952.) Summary. A formulation of quantum electrodynamics in terms of the renor- malized Heisenberg operators and the experimental mass and charge of the electron is given. The renormalization constants are implicitly defined and ex¬ pressed as integrals over finite functions in momentum space. No discussion of the convergence of these integrals or of the existence of rigorous solutions is given. Introduction. The renormalization method in quantum electrodynamics has been investigated by many authors, and it has been proved by Dyson1) that every term in a formal expansion in powers of the coupling constant of various expressions is a finite quantity. -
THE DEVELOPMENT of the SPACE-TIME VIEW of QUANTUM ELECTRODYNAMICS∗ by Richard P
THE DEVELOPMENT OF THE SPACE-TIME VIEW OF QUANTUM ELECTRODYNAMICS∗ by Richard P. Feynman California Institute of Technology, Pasadena, California Nobel Lecture, December 11, 1965. We have a habit in writing articles published in scientific journals to make the work as finished as possible, to cover all the tracks, to not worry about the blind alleys or to describe how you had the wrong idea first, and so on. So there isn’t any place to publish, in a dignified manner, what you actually did in order to get to do the work, although, there has been in these days, some interest in this kind of thing. Since winning the prize is a personal thing, I thought I could be excused in this particular situation, if I were to talk personally about my relationship to quantum electrodynamics, rather than to discuss the subject itself in a refined and finished fashion. Furthermore, since there are three people who have won the prize in physics, if they are all going to be talking about quantum electrodynamics itself, one might become bored with the subject. So, what I would like to tell you about today are the sequence of events, really the sequence of ideas, which occurred, and by which I finally came out the other end with an unsolved problem for which I ultimately received a prize. I realize that a truly scientific paper would be of greater value, but such a paper I could publish in regular journals. So, I shall use this Nobel Lecture as an opportunity to do something of less value, but which I cannot do elsewhere. -
Coherent States and the Classical Limit in Quantum Mechanics
Coherent States And The Classical Limit In Quantum Mechanics 0 ħ ¡! Bram Merten Radboud University Nijmegen Bachelor’s Thesis Mathematics/Physics 2018 Department Of Mathematical Physics Under Supervision of: Michael Mueger Abstract A thorough analysis is given of the academical paper titled "The Classical Limit for Quantum Mechanical Correlation Functions", written by the German physicist Klaus Hepp. This paper was published in 1974 in the journal of Communications in Mathematical Physics [1]. The part of the paper that is analyzed summarizes to the following: "Suppose expectation values of products of Weyl operators are translated in time by a quantum mechanical Hamiltonian and are in coherent states 1/2 1/2 centered in phase space around the coordinates ( ¡ ¼, ¡ »), where (¼,») is ħ ħ an element of classical phase space, then, after one takes the classical limit 0, the expectation values of products of Weyl operators become ħ ¡! exponentials of coordinate functions of the classical orbit in phase space." As will become clear in this thesis, authors tend to omit many non-trivial intermediate steps which I will precisely include. This could be of help to any undergraduate student who is willing to familiarize oneself with the reading of academical papers, but could also target any older student or professor who is doing research and interested in Klaus Hepp’s work. Preliminary chapters which will explain all the prerequisites to this paper are given as well. Table of Contents 0 Preface 1 1 Introduction 2 1.1 About Quantum Mechanics . .2 1.2 About The Wave function . .2 1.3 About The Correspondence of Classical and Quantum mechanics . -
Quantum Theory and the Structure of Space-Time
Quantum theory and the structure of space-time Tejinder Singh Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India ABSTRACT We argue that space and space-time emerge as a consequence of dynamical collapse of the wave function of macroscopic objects. Locality and separability are properties of our approximate, emergent universe. At the fundamental level, space-time is non-commutative, and dynamics is non-local and non-separable. I. SPACE-TIME IS NOT THE PERFECT ARENA FOR QUANTUM THEORY Space-time is absolute, in conventional classical physics. Its geometry is determined dy- namically by the distribution of classical objects in the universe. However, the underlying space-time manifold is an absolute given, providing the arena in which material bodies and fields exist. The same classical space-time arena is carried over to quantum mechanics and to quantum field theory, and it works beautifully there too. Well, almost! But not quite. In this essay we propose the thesis that the troubles of quantum theory arise because of the illegal carry-over of this classical arena. By troubles we mean the quantum measurement problem, the spooky action at a distance and the peculiar nature of quantum non-locality, the so-called problem of time in quantum theory, the extreme dependence of the theory on its classical limit, and the physical meaning of the wave function [1]. We elaborate on these in the next section. Then, in Section III, we propose that the correct arena for quantum theory is a non-commutative space-time: here there are no troubles. Classical space-time emerges as an approximation, as a consequence of dynamical collapse of the wave function. -
Path Integrals in Quantum Mechanics
Path Integrals in Quantum Mechanics Emma Wikberg Project work, 4p Department of Physics Stockholm University 23rd March 2006 Abstract The method of Path Integrals (PI’s) was developed by Richard Feynman in the 1940’s. It offers an alternate way to look at quantum mechanics (QM), which is equivalent to the Schrödinger formulation. As will be seen in this project work, many "elementary" problems are much more difficult to solve using path integrals than ordinary quantum mechanics. The benefits of path integrals tend to appear more clearly while using quantum field theory (QFT) and perturbation theory. However, one big advantage of Feynman’s formulation is a more intuitive way to interpret the basic equations than in ordinary quantum mechanics. Here we give a basic introduction to the path integral formulation, start- ing from the well known quantum mechanics as formulated by Schrödinger. We show that the two formulations are equivalent and discuss the quantum mechanical interpretations of the theory, as well as the classical limit. We also perform some explicit calculations by solving the free particle and the harmonic oscillator problems using path integrals. The energy eigenvalues of the harmonic oscillator is found by exploiting the connection between path integrals, statistical mechanics and imaginary time. Contents 1 Introduction and Outline 2 1.1 Introduction . 2 1.2 Outline . 2 2 Path Integrals from ordinary Quantum Mechanics 4 2.1 The Schrödinger equation and time evolution . 4 2.2 The propagator . 6 3 Equivalence to the Schrödinger Equation 8 3.1 From the Schrödinger equation to PI’s . 8 3.2 From PI’s to the Schrödinger equation . -
2. Classical Gases
2. Classical Gases Our goal in this section is to use the techniques of statistical mechanics to describe the dynamics of the simplest system: a gas. This means a bunch of particles, flying around in a box. Although much of the last section was formulated in the language of quantum mechanics, here we will revert back to classical mechanics. Nonetheless, a recurrent theme will be that the quantum world is never far behind: we’ll see several puzzles, both theoretical and experimental, which can only truly be resolved by turning on ~. 2.1 The Classical Partition Function For most of this section we will work in the canonical ensemble. We start by reformu- lating the idea of a partition function in classical mechanics. We’ll consider a simple system – a single particle of mass m moving in three dimensions in a potential V (~q ). The classical Hamiltonian of the system3 is the sum of kinetic and potential energy, p~ 2 H = + V (~q ) 2m We earlier defined the partition function (1.21) to be the sum over all quantum states of the system. Here we want to do something similar. In classical mechanics, the state of a system is determined by a point in phase space.Wemustspecifyboththeposition and momentum of each of the particles — only then do we have enough information to figure out what the system will do for all times in the future. This motivates the definition of the partition function for a single classical particle as the integration over phase space, 1 3 3 βH(p,q) Z = d qd pe− (2.1) 1 h3 Z The only slightly odd thing is the factor of 1/h3 that sits out front.