The QED Coupling Constant for an Electron to Emit Or Absorb a Photon Is Shown to Be the Square Root of the Fine Structure Constant Α Shlomo Barak
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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. -
Coupling Constant Unification in Extensions of Standard Model
Coupling Constant Unification in Extensions of Standard Model Ling-Fong Li, and Feng Wu Department of Physics, Carnegie Mellon University, Pittsburgh, PA 15213 May 28, 2018 Abstract Unification of electromagnetic, weak, and strong coupling con- stants is studied in the extension of standard model with additional fermions and scalars. It is remarkable that this unification in the su- persymmetric extension of standard model yields a value of Weinberg angle which agrees very well with experiments. We discuss the other possibilities which can also give same result. One of the attractive features of the Grand Unified Theory is the con- arXiv:hep-ph/0304238v2 3 Jun 2003 vergence of the electromagnetic, weak and strong coupling constants at high energies and the prediction of the Weinberg angle[1],[3]. This lends a strong support to the supersymmetric extension of the Standard Model. This is because the Standard Model without the supersymmetry, the extrapolation of 3 coupling constants from the values measured at low energies to unifi- cation scale do not intercept at a single point while in the supersymmetric extension, the presence of additional particles, produces the convergence of coupling constants elegantly[4], or equivalently the prediction of the Wein- berg angle agrees with the experimental measurement very well[5]. This has become one of the cornerstone for believing the supersymmetric Standard 1 Model and the experimental search for the supersymmetry will be one of the main focus in the next round of new accelerators. In this paper we will explore the general possibilities of getting coupling constants unification by adding extra particles to the Standard Model[2] to see how unique is the Supersymmetric Standard Model in this respect[?]. -
The Massless Two-Loop Two-Point Function and Zeta Functions in Counterterms of Feynman Diagrams
The Massless Two-loop Two-point Function and Zeta Functions in Counterterms of Feynman Diagrams Dissertation zur Erlangung des Grades \Doktor der Naturwissenschaften" am Fachbereich Physik der Johannes-Gutenberg-Universit¨at in Mainz Isabella Bierenbaum geboren in Landau/Pfalz Mainz, Februar 2005 Datum der mundlic¨ hen Prufung:¨ 6. Juni 2005 D77 (Diss. Universit¨at Mainz) Contents 1 Introduction 1 2 Renormalization 3 2.1 General introduction . 3 2.2 Feynman diagrams and power counting . 5 2.3 Dimensional regularization . 9 2.4 Counterterms . 10 2.4.1 One-loop diagrams . 10 2.4.2 Multi-loop diagrams . 11 3 Hopf and Lie algebra 15 3.1 The Hopf algebras HR and HF G . 15 3.1.1 The Hopf algebra of rooted trees HR . 16 3.1.2 The Hopf algebra of Feynman graphs HF G . 20 3.1.3 Correspondence between HR, HF G, and ZFF . 20 3.2 Lie algebras . 24 4 The massless two-loop two-point function | an overview 27 4.1 General remarks . 27 4.2 Integer exponents νi | the triangle relation . 29 4.3 Non-integer exponents νi . 32 5 Nested sums 37 5.1 Nested sums . 38 5.1.1 From polylogarithms to multiple polylogarithms . 38 5.1.2 Algebraic relations: shuffle and quasi-shuffle . 41 5.2 nestedsums | the theory and some of its functions . 45 5.2.1 nestedsums | the general idea . 46 5.2.2 nestedsums | the four classes of functions . 48 6 The massless two-loop two-point function 53 6.1 The expansion of I^(2;5) . 53 6.1.1 Decomposition of I^(2;5) . -
Critical Coupling for Dynamical Chiral-Symmetry Breaking with an Infrared Finite Gluon Propagator *
BR9838528 Instituto de Fisica Teorica IFT Universidade Estadual Paulista November/96 IFT-P.050/96 Critical coupling for dynamical chiral-symmetry breaking with an infrared finite gluon propagator * A. A. Natale and P. S. Rodrigues da Silva Instituto de Fisica Teorica Universidade Estadual Paulista Rua Pamplona 145 01405-900 - Sao Paulo, S.P. Brazil *To appear in Phys. Lett. B t 2 9-04 Critical Coupling for Dynamical Chiral-Symmetry Breaking with an Infrared Finite Gluon Propagator A. A. Natale l and P. S. Rodrigues da Silva 2 •r Instituto de Fisica Teorica, Universidade Estadual Paulista Rua Pamplona, 145, 01405-900, Sao Paulo, SP Brazil Abstract We compute the critical coupling constant for the dynamical chiral- symmetry breaking in a model of quantum chromodynamics, solving numer- ically the quark self-energy using infrared finite gluon propagators found as solutions of the Schwinger-Dyson equation for the gluon, and one gluon prop- agator determined in numerical lattice simulations. The gluon mass scale screens the force responsible for the chiral breaking, and the transition occurs only for a larger critical coupling constant than the one obtained with the perturbative propagator. The critical coupling shows a great sensibility to the gluon mass scale variation, as well as to the functional form of the gluon propagator. 'e-mail: [email protected] 2e-mail: [email protected] 1 Introduction The idea that quarks obtain effective masses as a result of a dynamical breakdown of chiral symmetry (DBCS) has received a great deal of attention in the last years [1, 2]. One of the most common methods used to study the quark mass generation is to look for solutions of the Schwinger-Dyson equation for the fermionic propagator. -
Arxiv:1202.1557V1
The Heisenberg-Euler Effective Action: 75 years on ∗ Gerald V. Dunne Physics Department, University of Connecticut, Storrs, CT 06269-3046, USA On this 75th anniversary of the publication of the Heisenberg-Euler paper on the full non- perturbative one-loop effective action for quantum electrodynamics I review their paper and discuss some of the impact it has had on quantum field theory. I. HISTORICAL CONTEXT After the 1928 publication of Dirac’s work on his relativistic theory of the electron [1], Heisenberg immediately appreciated the significance of the new ”hole theory” picture of the quantum vacuum of quantum electrodynamics (QED). Following some confusion, in 1931 Dirac associated the holes with positively charged electrons [2]: A hole, if there were one, would be a new kind of particle, unknown to experimental physics, having the same mass and opposite charge to an electron. With the discovery of the positron in 1932, soon thereafter [but, interestingly, not immediately [3]], Dirac proposed at the 1933 Solvay Conference that the negative energy solutions [holes] should be identified with the positron [4]: Any state of negative energy which is not occupied represents a lack of uniformity and this must be shown by observation as a kind of hole. It is possible to assume that the positrons are these holes. Positron theory and QED was born, and Heisenberg began investigating positron theory in earnest, publishing two fundamental papers in 1934, formalizing the treatment of the quantum fluctuations inherent in this Dirac sea picture of the QED vacuum [5, 6]. It was soon realized that these quantum fluctuations would lead to quantum nonlinearities [6]: Halpern and Debye have already independently drawn attention to the fact that the Dirac theory of the positron leads to the scattering of light by light, even when the energy of the photons is not sufficient to create pairs. -
Vacuum Energy
Vacuum Energy Mark D. Roberts, 117 Queen’s Road, Wimbledon, London SW19 8NS, Email:[email protected] http://cosmology.mth.uct.ac.za/ roberts ∼ February 1, 2008 Eprint: hep-th/0012062 Comments: A comprehensive review of Vacuum Energy, which is an extended version of a poster presented at L¨uderitz (2000). This is not a review of the cosmolog- ical constant per se, but rather vacuum energy in general, my approach to the cosmological constant is not standard. Lots of very small changes and several additions for the second and third versions: constructive feedback still welcome, but the next version will be sometime in coming due to my sporadiac internet access. First Version 153 pages, 368 references. Second Version 161 pages, 399 references. arXiv:hep-th/0012062v3 22 Jul 2001 Third Version 167 pages, 412 references. The 1999 PACS Physics and Astronomy Classification Scheme: http://publish.aps.org/eprint/gateway/pacslist 11.10.+x, 04.62.+v, 98.80.-k, 03.70.+k; The 2000 Mathematical Classification Scheme: http://www.ams.org/msc 81T20, 83E99, 81Q99, 83F05. 3 KEYPHRASES: Vacuum Energy, Inertial Mass, Principle of Equivalence. 1 Abstract There appears to be three, perhaps related, ways of approaching the nature of vacuum energy. The first is to say that it is just the lowest energy state of a given, usually quantum, system. The second is to equate vacuum energy with the Casimir energy. The third is to note that an energy difference from a complete vacuum might have some long range effect, typically this energy difference is interpreted as the cosmological constant. -
1.3 Running Coupling and Renormalization 27
1.3 Running coupling and renormalization 27 1.3 Running coupling and renormalization In our discussion so far we have bypassed the problem of renormalization entirely. The need for renormalization is related to the behavior of a theory at infinitely large energies or infinitesimally small distances. In practice it becomes visible in the perturbative expansion of Green functions. Take for example the tadpole diagram in '4 theory, d4k i ; (1.76) (2π)4 k2 m2 Z − which diverges for k . As we will see below, renormalizability means that the ! 1 coupling constant of the theory (or the coupling constants, if there are several of them) has zero or positive mass dimension: d 0. This can be intuitively understood as g ≥ follows: if M is the mass scale introduced by the coupling g, then each additional vertex in the perturbation series contributes a factor (M=Λ)dg , where Λ is the intrinsic energy scale of the theory and appears for dimensional reasons. If d 0, these diagrams will g ≥ be suppressed in the UV (Λ ). If it is negative, they will become more and more ! 1 relevant and we will find divergences with higher and higher orders.8 Renormalizability. The renormalizability of a quantum field theory can be deter- mined from dimensional arguments. Consider φp theory in d dimensions: 1 g S = ddx ' + m2 ' + 'p : (1.77) − 2 p! Z The action must be dimensionless, hence the Lagrangian has mass dimension d. From the kinetic term we read off the mass dimension of the field, namely (d 2)=2. The − mass dimension of 'p is thus p (d 2)=2, so that the dimension of the coupling constant − must be d = d + p pd=2. -
(Supersymmetric) Grand Unification
J. Reuter SUSY GUTs Uppsala, 15.05.2008 (Supersymmetric) Grand Unification Jürgen Reuter Albert-Ludwigs-Universität Freiburg Uppsala, 15. May 2008 J. Reuter SUSY GUTs Uppsala, 15.05.2008 Literature – General SUSY: M. Drees, R. Godbole, P. Roy, Sparticles, World Scientific, 2004 – S. Martin, SUSY Primer, arXiv:hep-ph/9709356 – H. Georgi, Lie Algebras in Particle Physics, Harvard University Press, 1992 – R. Slansky, Group Theory for Unified Model Building, Phys. Rep. 79 (1981), 1. – R. Mohapatra, Unification and Supersymmetry, Springer, 1986 – P. Langacker, Grand Unified Theories, Phys. Rep. 72 (1981), 185. – P. Nath, P. Fileviez Perez, Proton Stability..., arXiv:hep-ph/0601023. – U. Amaldi, W. de Boer, H. Fürstenau, Comparison of grand unified theories with electroweak and strong coupling constants measured at LEP, Phys. Lett. B260, (1991), 447. J. Reuter SUSY GUTs Uppsala, 15.05.2008 The Standard Model (SM) – Theorist’s View Renormalizable Quantum Field Theory (only with Higgs!) based on SU(3)c × SU(2)w × U(1)Y non-simple gauge group ν u h+ L = Q = uc dc `c [νc ] L ` L d R R R R h0 L L Interactions: I Gauge IA (covariant derivatives in kinetic terms): X a a ∂µ −→ Dµ = ∂µ + i gkVµ T k I Yukawa IA: u d e ˆ n ˜ Y QLHuuR + Y QLHddR + Y LLHdeR +Y LLHuνR I Scalar self-IA: (H†H)(H†H)2 J. Reuter SUSY GUTs Uppsala, 15.05.2008 The group-theoretical bottom line Things to remember: Representations of SU(N) i j 2 I fundamental reps. φi ∼ N, ψ ∼ N, adjoint reps. -
Understanding the Fully Non-Perturbative Strong-Field Regime of QED Loi to Theory Frontier Phil H
Understanding the Fully Non-Perturbative Strong-Field Regime of QED LoI to Theory Frontier Phil H. Bucksbaum, Gerald V. Dunnea), Frederico Fiuza, Sebastian Meurenb), Michael E. Peskin, David A. Reis, Greger Torgrimsson, Glen White, and Vitaly Yakimenko (Dated: June 2020) Abstract: Although perturbative QED with small background fields is well-understood and well-tested, there is much less understanding of QED in the regime of strong fields. At 2 3 18 the Schwinger critical field, Ec = m c /e~ ∼ 10 V/m, the vacuum becomes unstable to 2/3 pair production. For stronger fields, such that α(E/Ec) > 1, QED perturbation theory breaks down. These regimes are relevant to environments found in high-energy astrophysics and to physics in the collisions of high-energy electron and heavy ion beams. We plan to investigate problems in beam simulation and basic QED theory related to QED at strong fields, to analyze experiments that can test QED in this regime, and to explore applications to astrophysics and particle physics. Perturbative QED is characterized by the vacuum electron/positron mass scale, m ∼ MeV, a large mass gap between fermions and the massless photon, and a very small coupling constant α = e2/(4π), which facilitates the perturbative expansion. For many quantities in fundamental lepton and atomic physics, the QED perturbation expansion is extremely accurate. Indeed, the precise agreement between theory and experiment for these quantities is a triumph of modern physics [1]. This picture changes profoundly in the√ presence of very strong background fields [2–8]. The back- ground field introduces a new mass scale eE∗, where E∗ is the rest-frame electric field experienced 2 by an electron/positron with charge ∓e. -
The Determination of the Strong Coupling Constant Arxiv
The Determination of the Strong Coupling Constant G¨unther Dissertori Institute for Particle Physics, ETH Zurich, Switzerland June 18, 2015 Abstract The strong coupling constant is one of the fundamental parame- ters of the standard model of particle physics. In this review I will briefly summarise the theoretical framework, within which the strong coupling constant is defined and how it is connected to measurable observables. Then I will give an historical overview of its experimen- tal determinations and discuss the current status and world average value. Among the many different techniques used to determine this coupling constant in the context of quantum chromodynamics, I will focus in particular on a number of measurements carried out at the Large Electron Positron Collider (LEP) and the Large Hadron Col- lider (LHC) at CERN. arXiv:1506.05407v1 [hep-ex] 17 Jun 2015 A contribution to: The Standard Theory up to the Higgs discovery - 60 years of CERN L. Maiani and G. Rolandi, eds. 1 1 Introduction The strong coupling constant, αs, is the only free parameter of the lagrangian of quantum chromodynamics (QCD), the theory of strong interactions, if we consider the quarkp masses as fixed. As such, this coupling constant, or equivalently gs = 4παs, is one of the three fundamental coupling constants of the standard model (SM) of particle physics. It is related to the SU(3)C colour part of the overall SU(3)C × SU(2)L × U(1)Y gauge symmetry of the SM. The other two constants g and g0 indicate the coupling strengths relevant for weak isospin and weak hypercharge, and can be rewritten in terms of 0 the Weinberg mixing angle tan θW = g =g and the fine-structure constant 2 α = e =(4π), where the electric charge is given by e = g sin θW. -
Feynman Diagrams Particle and Nuclear Physics
5. Feynman Diagrams Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 5. Feynman Diagrams 1 In this section... Introduction to Feynman diagrams. Anatomy of Feynman diagrams. Allowed vertices. General rules Dr. Tina Potter 5. Feynman Diagrams 2 Feynman Diagrams The results of calculations based on a single process in Time-Ordered Perturbation Theory (sometimes called old-fashioned, OFPT) depend on the reference frame. Richard Feynman 1965 Nobel Prize The sum of all time orderings is frame independent and provides the basis for our relativistic theory of Quantum Mechanics. A Feynman diagram represents the sum of all time orderings + = −−!time −−!time −−!time Dr. Tina Potter 5. Feynman Diagrams 3 Feynman Diagrams Each Feynman diagram represents a term in the perturbation theory expansion of the matrix element for an interaction. Normally, a full matrix element contains an infinite number of Feynman diagrams. Total amplitude Mfi = M1 + M2 + M3 + ::: 2 Total rateΓ fi = 2πjM1 + M2 + M3 + :::j ρ(E) Fermi's Golden Rule But each vertex gives a factor of g, so if g is small (i.e. the perturbation is small) only need the first few. (Lowest order = fewest vertices possible) 2 4 g g g 6 p e2 1 Example: QED g = e = 4πα ∼ 0:30, α = 4π ∼ 137 Dr. Tina Potter 5. Feynman Diagrams 4 Feynman Diagrams Perturbation Theory Calculating Matrix Elements from Perturbation Theory from first principles is cumbersome { so we dont usually use it. Need to do time-ordered sums of (on mass shell) particles whose production and decay does not conserve energy and momentum. Feynman Diagrams Represent the maths of Perturbation Theory with Feynman Diagrams in a very simple way (to arbitrary order, if couplings are small enough). -
1. Physical Constants 1
1. Physical constants 1 1. PHYSICAL CONSTANTS Table 1.1. Reviewed 2013 by P.J. Mohr (NIST). Mainly from the “CODATA Recommended Values of the Fundamental Physical Constants: 2010” by P.J. Mohr, B.N. Taylor, and D.B. Newell in Rev. Mod. Phys. 84, 1527 (2012). The last group of constants (beginning with the Fermi coupling constant) comes from the Particle Data Group. The figures in parentheses after the values give the 1-standard-deviation uncertainties in the last digits; the corresponding fractional uncertainties in parts per 109 (ppb) are given in the last column. This set of constants (aside from the last group) is recommended for international use by CODATA (the Committee on Data for Science and Technology). The full 2010 CODATA set of constants may be found at http://physics.nist.gov/constants. See also P.J. Mohr and D.B. Newell, “Resource Letter FC-1: The Physics of Fundamental Constants,” Am. J. Phys. 78, 338 (2010). Quantity Symbol, equation Value Uncertainty (ppb) speed of light in vacuum c 299 792 458 m s−1 exact∗ Planck constant h 6.626 069 57(29)×10−34 J s 44 Planck constant, reduced ~ ≡ h/2π 1.054 571 726(47)×10−34 J s 44 = 6.582 119 28(15)×10−22 MeVs 22 electron charge magnitude e 1.602 176 565(35)×10−19 C = 4.803 204 50(11)×10−10 esu 22,22 conversion constant ~c 197.326 9718(44) MeV fm 22 conversion constant (~c)2 0.389 379 338(17) GeV2 mbarn 44 2 −31 electron mass me 0.510 998 928(11) MeV/c = 9.109 382 91(40)×10 kg 22,44 2 −27 proton mass mp 938.272 046(21) MeV/c = 1.672 621 777(74)×10 kg 22,44 = 1.007 276 466 812(90) u = 1836.152 672 45(75) me 0.089, 0.41 2 deuteron mass md 1875.612 859(41) MeV/c 22 12 2 −27 unified atomic mass unit (u) (mass C atom)/12 = (1 g)/(NA mol) 931.494 061(21) MeV/c = 1.660 538 921(73)×10 kg 22,44 2 −12 −1 permittivity of free space ǫ0 =1/µ0c 8.854 187 817 .