THE LAMB SHIFT by PHILIP 0. KOCH SUBMITTED IN
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Stochastic Quantization of Fermionic Theories: Renormalization of the Massive Thirring Model
Instituto de Física Teórica IFT Universidade Estadual Paulista October/92 IFT-R043/92 Stochastic Quantization of Fermionic Theories: Renormalization of the Massive Thirring Model J.C.Brunelli Instituto de Física Teórica Universidade Estadual Paulista Rua Pamplona, 145 01405-900 - São Paulo, S.P. Brazil 'This work was supported by CNPq. Instituto de Física Teórica Universidade Estadual Paulista Rua Pamplona, 145 01405 - Sao Paulo, S.P. Brazil Telephone: 55 (11) 288-5643 Telefax: 55(11)36-3449 Telex: 55 (11) 31870 UJMFBR Electronic Address: [email protected] 47553::LIBRARY Stochastic Quantization of Fermionic Theories: 1. Introduction Renormalization of the Massive Thimng Model' The stochastic quantization method of Parisi-Wu1 (for a review see Ref. 2) when applied to fermionic theories usually requires the use of a Langevin system modified by the introduction of a kernel3 J. C. Brunelli (1.1a) InBtituto de Física Teórica (1.16) Universidade Estadual Paulista Rua Pamplona, 145 01405 - São Paulo - SP where BRAZIL l = 2Kah(x,x )8(t - ?). (1.2) Here tj)1 tp and the Gaussian noises rj, rj are independent Grassmann variables. K(xty) is the aforementioned kernel which ensures the proper equilibrium limit configuration for Accepted for publication in the International Journal of Modern Physics A. mas si ess theories. The specific form of the kernel is quite arbitrary but in what follows, we use K(x,y) = Sn(x-y)(-iX + ™)- Abstract In a number of cases, it has been verified that the stochastic quantization procedure does not bring new anomalies and that the equilibrium limit correctly reproduces the basic (jJsfsini g the Langevin approach for stochastic processes we study the renormalizability properties of the models considered4. -
The Lamb Shift Experiment in Muonic Hydrogen
The Lamb Shift Experiment in Muonic Hydrogen Dissertation submitted to the Physics Faculty of the Ludwig{Maximilians{University Munich by Aldo Sady Antognini from Bellinzona, Switzerland Munich, November 2005 1st Referee : Prof. Dr. Theodor W. H¨ansch 2nd Referee : Prof. Dr. Dietrich Habs Date of the Oral Examination : December 21, 2005 Even if I don't think, I am. Itsuo Tsuda Je suis ou` je ne pense pas, je pense ou` je ne suis pas. Jacques Lacan A mia mamma e mio papa` con tanto amore Abstract The subject of this thesis is the muonic hydrogen (µ−p) Lamb shift experiment being performed at the Paul Scherrer Institute, Switzerland. Its goal is to measure the 2S 2P − energy difference in µp atoms by laser spectroscopy and to deduce the proton root{mean{ −3 square (rms) charge radius rp with 10 precision, an order of magnitude better than presently known. This would make it possible to test bound{state quantum electrody- namics (QED) in hydrogen at the relative accuracy level of 10−7, and will lead to an improvement in the determination of the Rydberg constant by more than a factor of seven. Moreover it will represent a benchmark for QCD theories. The experiment is based on the measurement of the energy difference between the F=1 F=2 2S1=2 and 2P3=2 levels in µp atoms to a precision of 30 ppm, using a pulsed laser tunable at wavelengths around 6 µm. Negative muons from a unique low{energy muon beam are −1 stopped at a rate of 70 s in 0.6 hPa of H2 gas. -
Casimir Effect Mechanism of Pairing Between Fermions in the Vicinity of A
Casimir effect mechanism of pairing between fermions in the vicinity of a magnetic quantum critical point Yaroslav A. Kharkov1 and Oleg P. Sushkov1 1School of Physics, University of New South Wales, Sydney 2052, Australia We consider two immobile spin 1/2 fermions in a two-dimensional magnetic system that is close to the O(3) magnetic quantum critical point (QCP) which separates magnetically ordered and disordered phases. Focusing on the disordered phase in the vicinity of the QCP, we demonstrate that the criticality results in a strong long range attraction between the fermions, with potential V (r) 1/rν , ν 0.75, where r is separation between the fermions. The mechanism of the enhanced∝ − attraction≈ is similar to Casimir effect and corresponds to multi-magnon exchange processes between the fermions. While we consider a model system, the problem is originally motivated by recent establishment of magnetic QCP in hole doped cuprates under the superconducting dome at doping of about 10%. We suggest the mechanism of magnetic critical enhancement of pairing in cuprates. PACS numbers: 74.40.Kb, 75.50.Ee, 74.20.Mn I. INTRODUCTION in the frame of normal Fermi liquid picture (large Fermi surface). Within this approach electrons interact via ex- change of an antiferromagnetic (AF) fluctuation (param- In the present paper we study interaction between 11 fermions mediated by magnetic fluctuations in a vicin- agnon). The lightly doped AF Mott insulator approach, ity of magnetic quantum critical point. To address this instead, necessarily implies small Fermi surface. In this case holes interact/pair via exchange of the Goldstone generic problem we consider a specific model of two holes 12 injected into the bilayer antiferromagnet. -
TASI 2008 Lectures: Introduction to Supersymmetry And
TASI 2008 Lectures: Introduction to Supersymmetry and Supersymmetry Breaking Yuri Shirman Department of Physics and Astronomy University of California, Irvine, CA 92697. [email protected] Abstract These lectures, presented at TASI 08 school, provide an introduction to supersymmetry and supersymmetry breaking. We present basic formalism of supersymmetry, super- symmetric non-renormalization theorems, and summarize non-perturbative dynamics of supersymmetric QCD. We then turn to discussion of tree level, non-perturbative, and metastable supersymmetry breaking. We introduce Minimal Supersymmetric Standard Model and discuss soft parameters in the Lagrangian. Finally we discuss several mech- anisms for communicating the supersymmetry breaking between the hidden and visible sectors. arXiv:0907.0039v1 [hep-ph] 1 Jul 2009 Contents 1 Introduction 2 1.1 Motivation..................................... 2 1.2 Weylfermions................................... 4 1.3 Afirstlookatsupersymmetry . .. 5 2 Constructing supersymmetric Lagrangians 6 2.1 Wess-ZuminoModel ............................... 6 2.2 Superfieldformalism .............................. 8 2.3 VectorSuperfield ................................. 12 2.4 Supersymmetric U(1)gaugetheory ....................... 13 2.5 Non-abeliangaugetheory . .. 15 3 Non-renormalization theorems 16 3.1 R-symmetry.................................... 17 3.2 Superpotentialterms . .. .. .. 17 3.3 Gaugecouplingrenormalization . ..... 19 3.4 D-termrenormalization. ... 20 4 Non-perturbative dynamics in SUSY QCD 20 4.1 Affleck-Dine-Seiberg -
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. -
Renormalization and Effective Field Theory
Mathematical Surveys and Monographs Volume 170 Renormalization and Effective Field Theory Kevin Costello American Mathematical Society surv-170-costello-cov.indd 1 1/28/11 8:15 AM http://dx.doi.org/10.1090/surv/170 Renormalization and Effective Field Theory Mathematical Surveys and Monographs Volume 170 Renormalization and Effective Field Theory Kevin Costello American Mathematical Society Providence, Rhode Island EDITORIAL COMMITTEE Ralph L. Cohen, Chair MichaelA.Singer Eric M. Friedlander Benjamin Sudakov MichaelI.Weinstein 2010 Mathematics Subject Classification. Primary 81T13, 81T15, 81T17, 81T18, 81T20, 81T70. The author was partially supported by NSF grant 0706954 and an Alfred P. Sloan Fellowship. For additional information and updates on this book, visit www.ams.org/bookpages/surv-170 Library of Congress Cataloging-in-Publication Data Costello, Kevin. Renormalization and effective fieldtheory/KevinCostello. p. cm. — (Mathematical surveys and monographs ; v. 170) Includes bibliographical references. ISBN 978-0-8218-5288-0 (alk. paper) 1. Renormalization (Physics) 2. Quantum field theory. I. Title. QC174.17.R46C67 2011 530.143—dc22 2010047463 Copying and reprinting. Individual readers of this publication, and nonprofit libraries acting for them, are permitted to make fair use of the material, such as to copy a chapter for use in teaching or research. Permission is granted to quote brief passages from this publication in reviews, provided the customary acknowledgment of the source is given. Republication, systematic copying, or multiple reproduction of any material in this publication is permitted only under license from the American Mathematical Society. Requests for such permission should be addressed to the Acquisitions Department, American Mathematical Society, 201 Charles Street, Providence, Rhode Island 02904-2294 USA. -
Regularization and Renormalization of Non-Perturbative Quantum Electrodynamics Via the Dyson-Schwinger Equations
University of Adelaide School of Chemistry and Physics Doctor of Philosophy Regularization and Renormalization of Non-Perturbative Quantum Electrodynamics via the Dyson-Schwinger Equations by Tom Sizer Supervisors: Professor A. G. Williams and Dr A. Kızılers¨u March 2014 Contents 1 Introduction 1 1.1 Introduction................................... 1 1.2 Dyson-SchwingerEquations . .. .. 2 1.3 Renormalization................................. 4 1.4 Dynamical Chiral Symmetry Breaking . 5 1.5 ChapterOutline................................. 5 1.6 Notation..................................... 7 2 Canonical QED 9 2.1 Canonically Quantized QED . 9 2.2 FeynmanRules ................................. 12 2.3 Analysis of Divergences & Weinberg’s Theorem . 14 2.4 ElectronPropagatorandSelf-Energy . 17 2.5 PhotonPropagatorandPolarizationTensor . 18 2.6 ProperVertex.................................. 20 2.7 Ward-TakahashiIdentity . 21 2.8 Skeleton Expansion and Dyson-Schwinger Equations . 22 2.9 Renormalization................................. 25 2.10 RenormalizedPerturbationTheory . 27 2.11 Outline Proof of Renormalizability of QED . 28 3 Functional QED 31 3.1 FullGreen’sFunctions ............................. 31 3.2 GeneratingFunctionals............................. 33 3.3 AbstractDyson-SchwingerEquations . 34 3.4 Connected and One-Particle Irreducible Green’s Functions . 35 3.5 Euclidean Field Theory . 39 3.6 QEDviaFunctionalIntegrals . 40 3.7 Regularization.................................. 42 3.7.1 Cutoff Regularization . 42 3.7.2 Pauli-Villars Regularization . 42 i 3.7.3 Lattice Regularization . 43 3.7.4 Dimensional Regularization . 44 3.8 RenormalizationoftheDSEs ......................... 45 3.9 RenormalizationGroup............................. 49 3.10BrokenScaleInvariance ............................ 53 4 The Choice of Vertex 55 4.1 Unrenormalized Quenched Formalism . 55 4.2 RainbowQED.................................. 57 4.2.1 Self-Energy Derivations . 58 4.2.2 Analytic Approximations . 60 4.2.3 Numerical Solutions . 62 4.3 Rainbow QED with a 4-Fermion Interaction . -
General Quantization
General quantization David Ritz Finkelstein∗ October 29, 2018 Abstract Segal’s hypothesis that physical theories drift toward simple groups follows from a general quantum principle and suggests a general quantization process. I general- quantize the scalar meson field in Minkowski space-time to illustrate the process. The result is a finite quantum field theory over a quantum space-time with higher symmetry than the singular theory. Multiple quantification connects the levels of the theory. 1 Quantization as regularization Quantum theory began with ad hoc regularization prescriptions of Planck and Bohr to fit the weird behavior of the electromagnetic field and the nuclear atom and to handle infinities that blocked earlier theories. In 1924 Heisenberg discovered that one small change in algebra did both naturally. In the early 1930’s he suggested extending his algebraic method to space-time, to regularize field theory, inspiring the pioneering quantum space-time of Snyder [43]. Dirac’s historic quantization program for gravity also eliminated absolute space-time points from the quantum theory of gravity, leading Bergmann too to say that the world point itself possesses no physical reality [5, 6]. arXiv:quant-ph/0601002v2 22 Jan 2006 For many the infinities that still haunt physics cry for further and deeper quanti- zation, but there has been little agreement on exactly what and how far to quantize. According to Segal canonical quantization continued a drift of physical theory toward simple groups that special relativization began. He proposed on Darwinian grounds that further quantization should lead to simple groups [32]. Vilela Mendes initiated the work in that direction [37]. -
Proton Polarisability Contribution to the Lamb Shift in Muonic Hydrogen
Proton polarisability contribution to the Lamb shift in muonic hydrogen Mike Birse University of Manchester Work done in collaboration with Judith McGovern Eur. Phys. J. A 48 (2012) 120 Mike Birse Proton polarisability contribution to the Lamb shift Mainz, June 2014 The Lamb shift in muonic hydrogen Much larger than in electronic hydrogen: DEL = E(2p1) − E(2s1) ' +0:2 eV 2 2 Dominated by vacuum polarisation Much more sensitive to proton structure, in particular, its charge radius th 2 DEL = 206:0668(25) − 5:2275(10)hrEi meV Results of many years of effort by Borie, Pachucki, Indelicato, Jentschura and others; collated in Antognini et al, Ann Phys 331 (2013) 127 Mike Birse Proton polarisability contribution to the Lamb shift Mainz, June 2014 The Lamb shift in muonic hydrogen Much larger than in electronic hydrogen: DEL = E(2p1) − E(2s1) ' +0:2 eV 2 2 Dominated by vacuum polarisation Much more sensitive to proton structure, in particular, its charge radius th 2 DEL = 206:0668(25) − 5:2275(10)hrEi meV Results of many years of effort by Borie, Pachucki, Indelicato, Jentschura and others; collated in Antognini et al, Ann Phys 331 (2013) 127 Includes contribution from two-photon exchange DE2g = 33:2 ± 2:0 µeV Sensitive to polarisabilities of proton by virtual photons Mike Birse Proton polarisability contribution to the Lamb shift Mainz, June 2014 Two-photon exchange Integral over T µn(n;q2) – doubly-virtual Compton amplitude for proton Spin-averaged, forward scattering ! two independent tensor structures Common choice: qµqn 1 p · q p · q -
Arxiv:1809.04416V1 [Physics.Gen-Ph]
Path integral and Sommerfeld quantization Mikoto Matsuda1, ∗ and Takehisa Fujita2, † 1Japan Health and Medical technological college, Tokyo, Japan 2College of Science and Technology, Nihon University, Tokyo, Japan (Dated: September 13, 2018) The path integral formulation can reproduce the right energy spectrum of the harmonic oscillator potential, but it cannot resolve the Coulomb potential problem. This is because the path integral cannot properly take into account the boundary condition, which is due to the presence of the scattering states in the Coulomb potential system. On the other hand, the Sommerfeld quantization can reproduce the right energy spectrum of both harmonic oscillator and Coulomb potential cases since the boundary condition is effectively taken into account in this semiclassical treatment. The basic difference between the two schemes should be that no constraint is imposed on the wave function in the path integral while the Sommerfeld quantization rule is derived by requiring that the state vector should be a single-valued function. The limitation of the semiclassical method is also clarified in terms of the square well and δ(x) function potential models. PACS numbers: 25.85.-w,25.85.Ec I. INTRODUCTION Quantum field theory is the basis of modern theoretical physics and it is well established by now [1–4]. If the kinematics is non-relativistic, then one obtains the equation of quantum mechanics which is the Schr¨odinger equation. In this respect, if one solves the Schr¨odinger equation, then one can properly obtain the energy eigenvalue of the corresponding potential model . Historically, however, the energy eigenvalue is obtained without solving the Schr¨odinger equation, and the most interesting method is known as the Sommerfeld quantization rule which is the semiclassical method [5–8]. -
SECOND QUANTIZATION Lecture Notes with Course Quantum Theory
SECOND QUANTIZATION Lecture notes with course Quantum Theory Dr. P.J.H. Denteneer Fall 2008 2 SECOND QUANTIZATION x1. Introduction and history 3 x2. The N-boson system 4 x3. The many-boson system 5 x4. Identical spin-0 particles 8 x5. The N-fermion system 13 x6. The many-fermion system 14 1 x7. Identical spin- 2 particles 17 x8. Bose-Einstein and Fermi-Dirac distributions 19 Second Quantization 1. Introduction and history Second quantization is the standard formulation of quantum many-particle theory. It is important for use both in Quantum Field Theory (because a quantized field is a qm op- erator with many degrees of freedom) and in (Quantum) Condensed Matter Theory (since matter involves many particles). Identical (= indistinguishable) particles −! state of two particles must either be symmetric or anti-symmetric under exchange of the particles. 1 ja ⊗ biB = p (ja1 ⊗ b2i + ja2 ⊗ b1i) bosons; symmetric (1a) 2 1 ja ⊗ biF = p (ja1 ⊗ b2i − ja2 ⊗ b1i) fermions; anti − symmetric (1b) 2 Motivation: why do we need the \second quantization formalism"? (a) for practical reasons: computing matrix elements between N-particle symmetrized wave functions involves (N!)2 terms (integrals); see the symmetrized states below. (b) it will be extremely useful to have a formalism that can handle a non-fixed particle number N, as in the grand-canonical ensemble in Statistical Physics; especially if you want to describe processes in which particles are created and annihilated (as in typical high-energy physics accelerator experiments). So: both for Condensed Matter and High-Energy Physics this formalism is crucial! (c) To describe interactions the formalism to be introduced will be vastly superior to the wave-function- and Hilbert-space-descriptions. -
Feynman Quantization
3 FEYNMAN QUANTIZATION An introduction to path-integral techniques Introduction. By Richard Feynman (–), who—after a distinguished undergraduate career at MIT—had come in as a graduate student to Princeton, was deeply involved in a collaborative effort with John Wheeler (his thesis advisor) to shake the foundations of field theory. Though motivated by problems fundamental to quantum field theory, as it was then conceived, their work was entirely classical,1 and it advanced ideas so radicalas to resist all then-existing quantization techniques:2 new insight into the quantization process itself appeared to be called for. So it was that (at a beer party) Feynman asked Herbert Jehle (formerly a student of Schr¨odinger in Berlin, now a visitor at Princeton) whether he had ever encountered a quantum mechanical application of the “Principle of Least Action.” Jehle directed Feynman’s attention to an obscure paper by P. A. M. Dirac3 and to a brief passage in §32 of Dirac’s Principles of Quantum Mechanics 1 John Archibald Wheeler & Richard Phillips Feynman, “Interaction with the absorber as the mechanism of radiation,” Reviews of Modern Physics 17, 157 (1945); “Classical electrodynamics in terms of direct interparticle action,” Reviews of Modern Physics 21, 425 (1949). Those were (respectively) Part III and Part II of a projected series of papers, the other parts of which were never published. 2 See page 128 in J. Gleick, Genius: The Life & Science of Richard Feynman () for a popular account of the historical circumstances. 3 “The Lagrangian in quantum mechanics,” Physicalische Zeitschrift der Sowjetunion 3, 64 (1933). The paper is reprinted in J.