Non Perturbative Effective Potentials of Quantum Oscillators

Total Page:16

File Type:pdf, Size:1020Kb

Non Perturbative Effective Potentials of Quantum Oscillators PRAMANA © Printed in India Vol. 42, No. 4, __journal of April 1994 physics pp. 285-297 Non perturbative effective potentials of quantum oscillators ROSE P IGNATIUS and K BABU JOSEPH Department of Physics, Cochin University of Science and Technology, Kochi 682 022, India MS received 23 July 1993 Abstract. Non perturbative analogues of the Gaussian effective potential (GEP) are defined for quantum oscillators obeying q--or (q,p)--deformed commutation relations. These are called the non perturbative q-effective potential (NPcEP) and the non perturbative qp effective potential (NP EP), in the respective cases. A system-specific effective potential (SSEP) is also introduced by'~eans of an additional minimization with respect to the q or q and p parameters. The method is applied to q and (q, p) oscillators of the quartic and sextic types. The SSEP in the case of ground states of the q-oscillators corresponds to q = I, which is the ordinary bosonic limit. A potential shape transition that involves the conversion of a double well to a single well or vice versa, is seen to exist in the case of quantum oscillators sitting in a double well potential. Keywords. Quantum groups; q-oscillator; non-perturbative effective potential; anharmonic oscillators. PACS Nos 02.20; 03.65; !i.10; 12.40 1. Introduction Quantum groups and quantum algebras have been receiving considerable attention in recent years [1-6]. Some of these investigations focus on quantum group modified quantum mechanics. In reference 6, for example, the spectrum of a q-anharmonic oscillator with quartic interaction has been studied using first order perturbation theory. There is a logical need to apply the non perturbative approach to such systems that are generically known as quantum oscillators. It is clear by now that the Gaussian effective potential (GEP) provides a powerful method for accounting the effect of quantum fluctuations on the classical potential [7]. A non perturbative technique enables one to perform systematic approximations in quantum mechanics as well as quantum field theory [7-9]. In this work we formulate a non perturbative q--or (q,p)--analogue of GEP with the help of appropriate quantum oscillator commutation relations that depend on a single parameter q, or two parameters q, p. The resulting quantity is called the non perturbative q-effective potential (NPqEP) or the non perturbative (q,p)--effective potential (NPqpEP), as the case may be. In the original version of GEP there is a positive mass parameter with respect to which the potential is minimized. When a quantum oscillator algebra is employed, the quantum parameters such as q, p can serve as additional parameters in the potential, suggesting a more elaborate scheme of minimization. The end product of the minimization procedure is termed the system-specific effective potential (SSEP). Following Barnes and Ghandour [10] the renormalized mass m u2 and coupling constant ~R are calculated directly from the NPqEP. 285 Rose P Ignatius and K Babu Joseph We study three kinds of quantum oscillator systems: quartic coupled quantum oscillators in a single well and in a double well, and sextic coupled quantum oscillators. Several interesting aspects emerge from these analyses. For example, for the ground state of a quartic or sextic anharmonic q-oscillator, the NPqEP is a minimum corresponding to q = 1 and a maximum corresponding to q = - 1. The renormalized mass mx turns out to be a maximum at q = I. Since mR has the physical significance of being the first excitation energy, these observations seem to cast ordinary (q = 1) quantum mechanics in a new perspective. For the X4-anharmonic (q, p)-oscillator, NPqpEP yields a minimum only if 2 or h vanishes. In the case of quartic q or (q, p)- oscillator in a double well potential, critical values exist for q or q as well as p, for which the double well degenerates into a single well. Results for quantum oscillators with sextic interaction also exhibit some interesting features. This paper is organized into five sections• In § 2 the concept of NPqEP, NPqpEP and SSEP are introduced• Quartic quantum oscillators in single and double well are discussed in § 3. Sextic quantum oscillators constitute the theme of§ 4 and concluding remarks comprise § 5. 2. Non perturbative effective potentials It is well-known that quantum fluctuations modify the classical potential energy, the zero point energy being the prime example. To discuss these effects in the framework of q-deformed quantum mechanics, we seek generalizations of position and momentum operators, X and P, in the form (h~ '/2 X=Xo+\-~] (a¢+a~) (I) P = ~-(2hf~)l/2(a¢ - a~ ) (2) where Xo is a classical c-number and a¢ and a~" are annihilation and creation operators, respectively, with the set ~ = Ill, q]. Here fl denotes a variational parameter having the dimension of mass or frequency that appears in the original q = 1 formulation of the GEP [7], and q is a quantum deformation parameter. For q = 1 the standard definitions of X and P are recovered. We impose the q-commutation relation: a~a~ -- qa~ a~ = q-N¢ (3) where N¢ is the number operator which is not assumed to be the same as a~ a~. In terms of X and P the q-commutation relation reads IX, P] = ih[q -n' + (q - 1)a~ a¢]. (4) Although, in principle, q could be real or complex, consistency of(4) with the assumption that X and P are simultaneously hermitian, constrains q to be a real parameter. The number operator N¢ is required to satisfy the commutation relations: [ae, Ne] = a t, (5) [a~, N~] = - a~. (6) 286 Pramana - J. Phys., Vol. 42, No. 4, April 1994 Quantum oscillators The number eigenstates [n)g are defined by the relation N¢ln)~ = nln)~ (7) where n = 0, 1, 2... The ground state 10)~ is assumed to be annihilated by a~: a¢10)¢ = 0. (8) The nth excited state In)¢ is obtained from 10)¢ by operating a~, n times: (a.t )" ,^. In)¢ = ([n]!)a/21" u )¢ (9) where the q-factorial [n]! is In]! = In]In- 1]... [11 with _q-a. [A] = qAq_ q- t The action of a¢ and a~" on the eigenkets In)~ is postulated as follows: a¢ln)¢ = [nlX/2ln - 1)~, (10) a~ln)~= [n+ 1]l/2ln + 1)e (11) The GEP is customarily defined [71 in the following fashion: V6(Xo) = min Vo(Xo, f~), = min (~01HI~>, (12) t'l where Xo = (¢,1X1¢,) and the lowest variational state I~') is a Gaussian, / fl \u,,. F - fl -I o>o. When q is real and q > 1, a q-analogue of the Gaussian function has been defined, [11] but its explicit form is not required here. We merely assume that the lowest variational trial state 1~')¢ depends on fl as well as q, and the excited states can be generated therefrom by applying a~ as many times as necessary. The NP~EP, with respect to any state kb)¢ is defined as follows: V~(Xo) = min Vq(So,t~) ___ rain ¢(~01H1~)¢. (14) fl Studies in quantum group phenomenoiogy [121 indicate the possibility of a given system being associated with a particular q value. This motivates one to define the Pramana - J. Phys., Vol. 42, No. 4, April 1994 287 Rose P Ignatius and K Babu Joseph SSqEP as follows: V(Xo) = min V(Xo, O, (15) ~ min ¢<g, IHl~>¢. n.q If the two-parameter quantum algebra characterising a (q. p)-oscillator is used [131 then the relevant commutation relations are a~a~ - qa: a, = p-t~.. (16) a,a + _ p-I a~ a. = qS.. (17) where the set t/== Eft. q. P]. A (q. p)-deformed number I-A'l~.pis defined by the relation qa _ p-A [A],I.p = q-p - 1 It is clear that the q-oscillator corresponds to the particular case where q--p. By analogy with the NPqEP, one defines the NP~pEP by the relation, V~,(Xo) = min Vq.,(Xodl). (18) Q --= min ,<¢IHi~>,. n The system-specific V(Xo). denoted SSqpEP. is defined as V(Xo) = min V(Xo, ~1), (19) wI = rain ~<~,lnl~,>,. ,q,p The renormalized mass mR and renormalized coupling constant 2R (in the quartic case) are obtained by differentiating the effective potential: = \ dX- o Ao- o' (20) )-R ---- ~ ~ • (21) 4. \ dX o }Xo- o It is clear that both m R2 and ,1.R depend on the quantum parameter(s), mR can be interpreted as the difference between the first excited state and ground state energies while 2R denotes the amplitude for a transition from the state II> to 13> under the action of coupling 2X 4 [101. 288 Puma - J. Phys., VoL 42, No. 4, April 1994 Quantum oscillators 3. Quartic quantum oscillators 3.1 Single well The Hamiltonian representing a quartic quantum (single well) oscillator is H = ½p" + ½m'X ~ + ,ix'. (22) If the system is a q-oscillator, then its NPqEP can be evaluated using the method developed in the preceding section. The expectation value of H for the nth eigenstate is written as (nlHln)= ~ K~X~o (23) l=0,2,4 where K0 = 4(In] + In + l]) tim 2 + ~-~([n] + [n + q) +2 ([n+ l][n+ 2] + [n+132 + 2[n][n+ l] + [hi 2 + [n][n -- 1]) K 2 = ½m2 + 31([n] + In + 13) K4 = i. The condition for the potential to be a minimum with respect to fl is the cubic equation Aft 3 + Bfi + C = 0, (24) where A = In] + In + 13, B = - (m 2 + 121X~]), C = - 2h1([n + 1][n + 2] + [n + 132 + 2[n + lien3 + [n] 2 + [n3En - 1]). Of the three roots of (24), the largest positive one, designated as fi, is to be employed for setting up the effective potential.
Recommended publications
  • Radiative Corrections in Curved Spacetime and Physical Implications to the Power Spectrum and Trispectrum for Different Inflationary Models
    Radiative Corrections in Curved Spacetime and Physical Implications to the Power Spectrum and Trispectrum for different Inflationary Models Dissertation zur Erlangung des mathematisch-naturwissenschaftlichen Doktorgrades Doctor rerum naturalium der Georg-August-Universit¨atG¨ottingen Im Promotionsprogramm PROPHYS der Georg-August University School of Science (GAUSS) vorgelegt von Simone Dresti aus Locarno G¨ottingen,2018 Betreuungsausschuss: Prof. Dr. Laura Covi, Institut f¨urTheoretische Physik, Universit¨atG¨ottingen Prof. Dr. Karl-Henning Rehren, Institut f¨urTheoretische Physik, Universit¨atG¨ottingen Prof. Dr. Dorothea Bahns, Mathematisches Institut, Universit¨atG¨ottingen Miglieder der Prufungskommission:¨ Referentin: Prof. Dr. Laura Covi, Institut f¨urTheoretische Physik, Universit¨atG¨ottingen Korreferentin: Prof. Dr. Dorothea Bahns, Mathematisches Institut, Universit¨atG¨ottingen Weitere Mitglieder der Prufungskommission:¨ Prof. Dr. Karl-Henning Rehren, Institut f¨urTheoretische Physik, Universit¨atG¨ottingen Prof. Dr. Stefan Kehrein, Institut f¨urTheoretische Physik, Universit¨atG¨ottingen Prof. Dr. Jens Niemeyer, Institut f¨urAstrophysik, Universit¨atG¨ottingen Prof. Dr. Ariane Frey, II. Physikalisches Institut, Universit¨atG¨ottingen Tag der mundlichen¨ Prufung:¨ Mittwoch, 23. Mai 2018 Ai miei nonni Marina, Palmira e Pierino iv ABSTRACT In a quantum field theory with a time-dependent background, as in an expanding uni- verse, the time-translational symmetry is broken. We therefore expect loop corrections to cosmological observables to be time-dependent after renormalization for interacting fields. In this thesis we compute and discuss such radiative corrections to the primordial spectrum and higher order spectra in simple inflationary models. We investigate both massless and massive virtual fields, and we disentangle the time dependence caused by the background and by the initial state that is set to the Bunch-Davies vacuum at the beginning of inflation.
    [Show full text]
  • Scalar Quantum Electrodynamics
    A complex system that works is invariably found to have evolved from a simple system that works. John Gall 17 Scalar Quantum Electrodynamics In nature, there exist scalar particles which are charged and are therefore coupled to the electromagnetic field. In three spatial dimensions, an important nonrelativistic example is provided by superconductors. The phenomenon of zero resistance at low temperature can be explained by the formation of so-called Cooper pairs of electrons of opposite momentum and spin. These behave like bosons of spin zero and charge q =2e, which are held together in some metals by the electron-phonon interaction. Many important predictions of experimental data can be derived from the Ginzburg- Landau theory of superconductivity [1]. The relativistic generalization of this theory to four spacetime dimensions is of great importance in elementary particle physics. In that form it is known as scalar quantum electrodynamics (scalar QED). 17.1 Action and Generating Functional The Ginzburg-Landau theory is a three-dimensional euclidean quantum field theory containing a complex scalar field ϕ(x)= ϕ1(x)+ iϕ2(x) (17.1) coupled to a magnetic vector potential A. The scalar field describes bound states of pairs of electrons, which arise in a superconductor at low temperatures due to an attraction coming from elastic forces. The detailed mechanism will not be of interest here; we only note that the pairs are bound in an s-wave and a spin singlet state of charge q =2e. Ignoring for a moment the magnetic interactions, the ensemble of these bound states may be described, in the neighborhood of the superconductive 4 transition temperature Tc, by a complex scalar field theory of the ϕ -type, by a euclidean action 2 3 1 m g 2 E = d x ∇ϕ∗∇ϕ + ϕ∗ϕ + (ϕ∗ϕ) .
    [Show full text]
  • Asymptotically Flat, Spherical, Self-Interacting Scalar, Dirac and Proca Stars
    S S symmetry Article Asymptotically Flat, Spherical, Self-Interacting Scalar, Dirac and Proca Stars Carlos A. R. Herdeiro and Eugen Radu * Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications (CIDMA), Campus de Santiago, 3810-183 Aveiro, Portugal; [email protected] * Correspondence: [email protected] Received: 14 November 2020; Accepted: 1 December 2020; Published: 8 December 2020 Abstract: We present a comparative analysis of the self-gravitating solitons that arise in the Einstein–Klein–Gordon, Einstein–Dirac, and Einstein–Proca models, for the particular case of static, spherically symmetric spacetimes. Differently from the previous study by Herdeiro, Pombo and Radu in 2017, the matter fields possess suitable self-interacting terms in the Lagrangians, which allow for the existence of Q-ball-type solutions for these models in the flat spacetime limit. In spite of this important difference, our analysis shows that the high degree of universality that was observed by Herdeiro, Pombo and Radu remains, and various spin-independent common patterns are observed. Keywords: solitons; boson stars; Dirac stars 1. Introduction and Motivation 1.1. General Remarks The (modern) idea of solitons, as extended particle-like configurations, can be traced back (at least) to Lord Kelvin, around one and half centuries ago, who proposed that atoms are made of vortex knots [1]. However, the first explicit example of solitons in a relativistic field theory was found by Skyrme [2,3], (almost) one hundred years later. The latter, dubbed Skyrmions, exist in a model with four (real) scalars that are subject to a constraint.
    [Show full text]
  • A Solvable Tensor Field Theory Arxiv:1903.02907V2 [Math-Ph]
    A Solvable Tensor Field Theory R. Pascalie∗ Universit´ede Bordeaux, LaBRI, CNRS UMR 5800, Talence, France, EU Mathematisches Institut der Westf¨alischen Wilhelms-Universit¨at,M¨unster,Germany, EU August 3, 2020 Abstract We solve the closed Schwinger-Dyson equation for the 2-point function of a tensor field theory with a quartic melonic interaction, in terms of Lambert's W-function, using a perturbative expansion and Lagrange-B¨urmannresummation. Higher-point functions are then obtained recursively. 1 Introduction Tensor models have regained a considerable interest since the discovery of their large N limit (see [1], [2], [3] or the book [4]). Recently, tensor models have been related in [5] and [6], to the Sachdev-Ye-Kitaev model [7], [8], [9], [10], which is a promising toy-model for understanding black holes through holography (see also [11], [12], the lectures [13] and the review [14]). In this paper we study a specific type of tensor field theory (TFT) 1. More precisely, we consider a U(N)-invariant tensor models whose kinetic part is modified to include a Laplacian- like operator (this operator is a discrete Laplacian in the Fourier transformed space of the tensor index space). This type of tensor model has originally been used to implement renormalization techniques for tensor models (see [16], the review [17] or the thesis [18] and references within) and has also been studied as an SYK-like TFT [19]. Recently, the functional Renormalization Group (FRG) as been used in [20] to investigate the existence of a universal continuum limit in tensor models, see also the review [21].
    [Show full text]
  • Arxiv:2003.01034V1 [Hep-Th] 2 Mar 2020 Im Oe.Frta Esntelna Oe a Etogta Ge a Large As the Thought in Be Solved Be Can Can Model Models Linear These the One
    Inhomogeneous states in two dimensional linear sigma model at large N A. Pikalov1,2∗ 1Moscow Institute of Physics and Technology, Dolgoprudny 141700, Russia 2Institute for Theoretical and Experimental Physics, Moscow, Russia (Dated: March 3, 2020) In this note we consider inhomogeneous solutions of two-dimensional linear sigma model in the large N limit. These solutions are similar to the ones found recently in two-dimensional CP N sigma model. The solution exists only for some range of coupling constant. We calculate energy of the solutions as function of parameters of the model and show that at some value of the coupling constant it changes sign signaling a possible phase transition. The case of the nonlinear model at finite temperature is also discussed. The free energy of the inhomogeneous solution is shown to change sign at some critical temperature. I. INTRODUCTION Two-dimensional linear sigma model is a theory of N real scalar fields and quartic O(N) symmetric interaction. The model has two dimensionful parameters: mass of the particles and coupling constant. In the limit of infinite coupling one can obtain the nonlinear O(N) arXiv:2003.01034v1 [hep-th] 2 Mar 2020 sigma model. For that reason the linear model can be thought as a generalization of the nonlinear one. These models can be solved in the large N limit, see [1] for a review. In turn O(N) sigma model is quite similar to the CP N sigma model. Recently the large N CP N sigma model was considered on a finite interval with various boundary conditions [2–8] and on circle [9–12].
    [Show full text]
  • Physics 215C: Particles and Fields Spring 2019
    Physics 215C: Particles and Fields Spring 2019 Lecturer: McGreevy These lecture notes live here. Please email corrections to mcgreevy at physics dot ucsd dot edu. Last updated: 2021/04/20, 14:28:40 1 Contents 0.1 Introductory remarks for the third quarter................4 0.2 Sources and acknowledgement.......................7 0.3 Conventions.................................8 1 Anomalies9 2 Effective field theory 20 2.1 A parable on integrating out degrees of freedom............. 20 2.2 Introduction to effective field theory.................... 25 2.3 The color of the sky............................. 30 2.4 Fermi theory of Weak Interactions..................... 32 2.5 Loops in EFT................................ 33 2.6 The Standard Model as an EFT...................... 39 2.7 Superconductors.............................. 42 2.8 Effective field theory of Fermi surfaces.................. 47 3 Geometric and topological terms in field theory actions 58 3.1 Coherent state path integrals for bosons................. 58 3.2 Coherent state path integral for fermions................. 66 3.3 Path integrals for spin systems....................... 73 3.4 Topological terms from integrating out fermions............. 86 3.5 Pions..................................... 89 4 Field theory of spin systems 99 4.1 Transverse-Field Ising Model........................ 99 4.2 Ferromagnets and antiferromagnets..................... 131 4.3 The beta function for 2d non-linear sigma models............ 136 4.4 CP1 representation and large-N ...................... 138 5 Duality 148 5.1 XY transition from superfluid to Mott insulator, and T-duality..... 148 6 Conformal field theory 158 6.1 The stress tensor and conformal invariance (abstract CFT)....... 160 6.2 Radial quantization............................. 166 6.3 Back to general dimensions......................... 172 7 Duality, part 2 179 7.1 (2+1)-d XY is dual to (2+1)d electrodynamics.............
    [Show full text]
  • Adiabatic Limits and Renormalization in Quantum Spacetime
    DOTTORATO DI RICERCA IN MATEMATICA XXXII CICLO DEL CORSO DI DOTTORATO Adiabatic limits and renormalization in quantum spacetime Aleksei Bykov A.A. 2019/2020 Docente Guida/Tutor: Prof. D. Guido Relatore: Prof. G. Morsella Coordinatore: Prof. A. Braides Contents 1 Introduction 4 2 Doplicher-Fredenhagen-Roberts Quantum Spacetime 11 2.1 Construction and basic facts . 11 2.2 Quantum fields on the DFR QST and the role of Qµν . 12 2.2.1 More general quantum fields in DFR QST . 13 2.3 Optimally localised states and the quantum diagonal map . 17 3 Perturbation theory for QFT and its non-local generalization 21 3.1 Hamiltonian perturbation theory . 22 3.1.1 Ordinary QFT . 22 3.1.2 Non-local case: fixing HI ............................. 26 3.1.3 Hamiltonian approach: fixing Hint ........................ 35 3.2 Lagrangian perturbation theories . 38 3.3 Yang-Feldman quantizaion . 41 3.4 LSZ reduction . 41 4 Feynman rules for non-local Hamiltonian Perturbation theory 45 5 Lagrangian reformulation of the Hamiltonian Feynman rules 52 6 Corrected propagator 57 7 Adiabatic limit 61 7.1 Weak adiabatic limit and the LSZ reduction . 61 7.1.1 Existence of the weak adiabatic limit . 61 7.1.2 Feynman rules from LSZ reduction . 64 7.2 Strong adiabatic limit . 65 8 Renormalization 68 8.1 Formal renormalization . 68 8.2 The physical renormalization . 71 8.2.1 Dispersion relation renormalisation . 72 8.2.2 Field strength renormalization . 72 8.3 Conluding remarks on renormalisation . 73 9 Conclusions 75 9.1 Summary of the main results . 75 9.2 Outline of further directions .
    [Show full text]
  • The Higgs Trilinear Coupling and the Scale of New Physics
    The Higgs Trilinear Coupling and the Scale of New Physics Spencer Chang Department of Physics and Institute of Theoretical Science University of Oregon, Eugene, Oregon 97403 and Department of Physics National Taiwan University, Taipei, Taiwan 10617, ROC Markus A. Luty Center for Quantum Mathematics and Physics (QMAP) University of California, Davis, California 95616 Abstract We consider modifications of the Higgs potential due to new physics at high energy scales. These upset delicate cancellations predicted by the Standard Model for processes involving Higgs bosons and longitudinal gauge bosons, and lead to a breakdown of the theory at high energies. We focus on modifications of the Higgs trilinear coupling and use the violation of tree- level unitarity as an estimate of the scale where the theory breaks down. We obtain a completely model-independent bound of <∼ 13 TeV for an order-1 modification of the trilinear. We argue that this bound can be saturated only in fine-tuned models, and the scale of new physics is likely to be much lower. The most stringent bounds are obtained from amplitudes involving multiparticle states that are not conventional scattering states. Our results arXiv:1902.05556v2 [hep-ph] 31 Mar 2020 show that a future determination of the Higgs cubic coupling can point to a well-defined scale of new physics that can be targeted and explored at future colliders. 1 Introduction Many of the couplings of the 125 GeV Higgs boson to gauge bosons and fermions have been measured at the 10% level and agree with the predictions of the Standard Model [1, 2].
    [Show full text]
  • Homework 8 – Due Friday, Nov 17Th – 8A,8B,8C
    Homework 8 – due Friday, Nov 17th – 8A,8B,8C (8A) Field redefinitions and scattering Consider a seemingly complicated theory with the basic complex scalar field B (note that |x|2 = x∗x): g L = |(∂ B)(1 + gB)|2 − m2|B + B2|2 µ 2 1. Divide the Lagrangian for B into a free part and interaction terms. Compute the elastic N + N¯ → N + N¯ scattering amplitude in the tree level approximation, imagining that you follow the LSZ formula. Tree level means that there are no loops and therefore you don’t need any counterterms. However, you will need a g2 vertex diagram as well as a diagram with two g cubic vertices. Also, you will need derivative interactions. With derivative interactions, it is not true that L = −H, and also, there are problems with commuting the time-derivatives through the normal-ordering symbol. Believe me that these two problems cancel and can be collectively ignored, as will be clear from Feynman’s path integral formulation later. Assume L = −H and be sloppy about permuting the T , ∂µ symbols. 2. Now pretend that someone brings you a secret message that says: g ψ = B + B2 2 Using this field redefinition, guess what is the Lagrangian for ψ – it is very simple! – and verify it by an actual calculation. What is the scattering amplitude for ψ quanta? This question should be supersimple. Use this simple answer as a hint to fix any combinatorial errors in the calculation with B if you have errors. 3. If you do the same calculation in the B variables or the ψ variables, will the off-shell Green’s functions of B and those of ψ be equal (yes/no)? Should they be (yes/no)? Should the on-shell amplitudes be equal (yes/no)? Comment: An advantage of the LSZ formalism is that it doesn’t matter whether you assign a field like B or a field like ψ to the particle.
    [Show full text]
  • Lectures on Quantum Field Theory
    Lectures on Quantum Field Theory Aleksandar R. Bogojevi´c1 Institute of Physics P. O. Box 57 11000 Belgrade, Yugoslavia March, 1998 1Email: [email protected] ii Contents 1 Linearity and Combinatorics 1 1.1 Schwinger–DysonEquations. 1 1.2 GeneratingFunctionals. 3 1.3 FreeFieldTheory ........................... 6 2 Further Combinatoric Structure 7 2.1 ClassicalFieldTheory ......................... 7 2.2 TheEffectiveAction .......................... 8 2.3 PathIntegrals.............................. 10 3 Using the Path Integral 15 3.1 Semi-ClassicalExpansion . 15 3.2 WardIdentities ............................. 18 4 Fermions 21 4.1 GrassmannNumbers.......................... 21 5 Euclidean Field Theory 27 5.1 Thermodynamics ............................ 30 5.2 WickRotation ............................. 31 6 Ferromagnets and Phase Transitions 33 6.1 ModelsofFerromagnets . 33 6.2 TheMeanFieldApproximation. 34 6.3 TransferMatrices............................ 35 6.4 Landau–Ginsburg Theory . 36 6.5 TowardsLoopExpansion . 38 7 The Propagator 41 7.1 ScalarPropagator ........................... 41 7.2 RandomWalk.............................. 43 iii iv CONTENTS 8 The Propagator Continued 47 8.1 The Yukawa Potential . 47 8.2 VirtualParticles ............................ 49 9 From Operators to Path Integrals 53 9.1 HamiltonianPathIntegral. 53 9.2 LagrangianPathIntegral . 55 9.3 QuantumFieldTheory. 57 10 Path Integral Surprises 59 10.1 Paths that don’t Contribute . 59 10.2 Lagrangian Measure from SD Equations . 62 11 Classical Symmetry 67 11.1 NoetherTechnique . 67 11.2 Energy-Momentum Tensors Galore . 70 12 Symmetry Breaking 73 12.1 GoldstoneBosons............................ 73 12.2 TheHiggsMechanism . 77 13 Effective Action to One Loop 81 13.1 TheEffectivePotential. 81 13.2 The O(N)Model............................ 86 14 Solitons 89 14.1 Perturbative vs. Semi-Classical . 89 14.2 ClassicalSolitons ............................ 90 14.3 The φ4 Kink .............................
    [Show full text]
  • Quantum Field Theory and Particle Physics
    Quantum Field Theory and Particle Physics Badis Ydri Département de Physique, Faculté des Sciences Université d’Annaba Annaba, Algerie 2 YDRI QFT Contents 1 Introduction and References 1 I Path Integrals, Gauge Fields and Renormalization Group 3 2 Path Integral Quantization of Scalar Fields 5 2.1 FeynmanPathIntegral. .. .. .. .. .. .. .. .. .. .. .. 5 2.2 ScalarFieldTheory............................... 9 2.2.1 PathIntegral .............................. 9 2.2.2 The Free 2 Point Function . 12 − 2.2.3 Lattice Regularization . 13 2.3 TheEffectiveAction .............................. 16 2.3.1 Formalism................................ 16 2.3.2 Perturbation Theory . 20 2.3.3 Analogy with Statistical Mechanics . 22 2.4 The O(N) Model................................ 23 2.4.1 The 2 Point and 4 Point Proper Vertices . 24 − − 2.4.2 Momentum Space Feynman Graphs . 25 2.4.3 Cut-off Regularization . 27 2.4.4 Renormalization at 1 Loop...................... 29 − 2.5 Two-Loop Calculations . 31 2.5.1 The Effective Action at 2 Loop ................... 31 − 2.5.2 The Linear Sigma Model at 2 Loop ................. 32 − 2.5.3 The 2 Loop Renormalization of the 2 Point Proper Vertex . 35 − − 2.5.4 The 2 Loop Renormalization of the 4 Point Proper Vertex . 40 − − 2.6 Renormalized Perturbation Theory . 42 2.7 Effective Potential and Dimensional Regularization . .......... 45 2.8 Spontaneous Symmetry Breaking . 49 2.8.1 Example: The O(N) Model ...................... 49 2.8.2 Glodstone’s Theorem . 55 3 Path Integral Quantization of Dirac and Vector Fields 57 3.1 FreeDiracField ................................ 57 3.1.1 Canonical Quantization . 57 3.1.2 Fermionic Path Integral and Grassmann Numbers . 58 4 YDRI QFT 3.1.3 The Electron Propagator .
    [Show full text]
  • The Standard Model of Particle Physics and Beyond
    Context Relativity - gauge theories The Standard Model of particle physics Beyond the Standard Model Summary The Standard Model of particle physics and beyond. Benjamin Fuks & Michel Rausch de Traubenberg IPHC Strasbourg / University of Strasbourg. [email protected] & [email protected] Slides available on http://www.cern.ch/fuks/esc.php 6-13 July 2011 The Standard Model of particle physics and beyond. Benjamin Fuks & Michel Rausch de Traubenberg - 1 Context Relativity - gauge theories The Standard Model of particle physics Beyond the Standard Model Summary Outline. 1 Context. 2 Special relativity and gauge theories. Action and symmetries. Poincar´eand Lorentz algebras and their representations. Relativistic wave equations. Gauge symmetries - Yang-Mills theories - symmetry breaking. 3 Construction of the Standard Model. Quantum Electrodynamics (QED). Scattering theory - Calculation of a squared matrix element. Weak interactions. The electroweak theory. Quantum Chromodynamics. 4 Beyond the Standard Model of particle physics. The Standard Model: advantages and open questions. Grand unified theories. Supersymmetry. Extra-dimensional theories. String theory. 5 Summary. The Standard Model of particle physics and beyond. Benjamin Fuks & Michel Rausch de Traubenberg - 2 Context Relativity - gauge theories The Standard Model of particle physics Beyond the Standard Model Summary Building blocks describing matter. Atom compositness. * Neutrons. * Protons. * Electrons. Proton and neutron compositness. * Naively: up and down quarks. * In reality: dynamical objects made of • Valence and sea quarks. • Gluons [see below...]. Beta decays. − * n ! p + e +ν ¯e . * Needs for a neutrino. The Standard Model of particle physics and beyond. Benjamin Fuks & Michel Rausch de Traubenberg - 3 Context Relativity - gauge theories The Standard Model of particle physics Beyond the Standard Model Summary Three families of fermionic particles [Why three?].
    [Show full text]