Quarks and Gluons in the Phase Diagram of Quantum Chromodynamics
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Lectures on Quantum Field Theory
QUANTUM FIELD THEORY Notes taken from a course of R. E. Borcherds, Fall 2001, Berkeley Richard E. Borcherds, Mathematics department, Evans Hall, UC Berkeley, CA 94720, U.S.A. e–mail: [email protected] home page: www.math.berkeley.edu/~reb Alex Barnard, Mathematics department, Evans Hall, UC Berkeley, CA 94720, U.S.A. e–mail: [email protected] home page: www.math.berkeley.edu/~barnard Contents 1 Introduction 4 1.1 Life Cycle of a Theoretical Physicist . ....... 4 1.2 Historical Survey of the Standard Model . ....... 5 1.3 SomeProblemswithNeutrinos . ... 9 1.4 Elementary Particles in the Standard Model . ........ 10 2 Lagrangians 11 arXiv:math-ph/0204014v1 8 Apr 2002 2.1 WhatisaLagrangian?.............................. 11 2.2 Examples ...................................... 11 2.3 The General Euler–Lagrange Equation . ...... 13 3 Symmetries and Currents 14 3.1 ObviousSymmetries ............................... 14 3.2 Not–So–ObviousSymmetries . 16 3.3 TheElectromagneticField. 17 1 3.4 Converting Classical Field Theory to Homological Algebra........... 19 4 Feynman Path Integrals 21 4.1 Finite Dimensional Integrals . ...... 21 4.2 TheFreeFieldCase ................................ 22 4.3 Free Field Green’s Functions . 23 4.4 TheNon-FreeCase................................. 24 5 0-Dimensional QFT 25 5.1 BorelSummation.................................. 28 5.2 OtherGraphSums................................. 28 5.3 TheClassicalField............................... 29 5.4 TheEffectiveAction ............................... 31 6 Distributions and Propagators 35 6.1 EuclideanPropagators . 36 6.2 LorentzianPropagators . 38 6.3 Wavefronts and Distribution Products . ....... 40 7 Higher Dimensional QFT 44 7.1 AnExample..................................... 44 7.2 Renormalisation Prescriptions . ....... 45 7.3 FiniteRenormalisations . 47 7.4 A Group Structure on Finite Renormalisations . ........ 50 7.5 More Conditions on Renormalisation Prescriptions . -
An Alternate Constructive Approach to the 43 Quantum Field Theory, and A
ANNALES DE L’I. H. P., SECTION A ALAN D. SOKAL 4 An alternate constructive approach to the j3 quantum 4 field theory, and a possible destructive approach to j4 Annales de l’I. H. P., section A, tome 37, no 4 (1982), p. 317-398 <http://www.numdam.org/item?id=AIHPA_1982__37_4_317_0> © Gauthier-Villars, 1982, tous droits réservés. L’accès aux archives de la revue « Annales de l’I. H. P., section A » implique l’accord avec les conditions générales d’utilisation (http://www.numdam. org/conditions). Toute utilisation commerciale ou impression systématique est constitutive d’une infraction pénale. Toute copie ou impression de ce fichier doit contenir la présente mention de copyright. Article numérisé dans le cadre du programme Numérisation de documents anciens mathématiques http://www.numdam.org/ Ann. Inst. Henri Poincaré, Vol. XXXVII, n° 4, 1982 317 An alternate constructive approach to the 03C643 quantum field theory, and a possible destructive approach to 03C644 (*) Alan D. SOKAL Courant Institute of Mathematical Sciences New York University, 251 Mercer Street, New York, New York 10012, USA ABSTRACT. - I study the construction of cp4 quantum field theories by means of lattice approximations. It is easy to prove the existence of the continuum limit (by subsequences) ; the key question is whether this limit is something other than a (generalized) free field. I use correlation inequalities, infrared bounds and field equations to investigate this question. For space-time dimension d less than four, I give a simple proof that the continuum-limit theory is indeed nontrivial ; it relies, however, on a conjec- tured correlation inequality closely related to the T6 conjecture of Glimm and Jaffe. -
University of California Santa Cruz Quantum
UNIVERSITY OF CALIFORNIA SANTA CRUZ QUANTUM GRAVITY AND COSMOLOGY A dissertation submitted in partial satisfaction of the requirements for the degree of DOCTOR OF PHILOSOPHY in PHYSICS by Lorenzo Mannelli September 2005 The Dissertation of Lorenzo Mannelli is approved: Professor Tom Banks, Chair Professor Michael Dine Professor Anthony Aguirre Lisa C. Sloan Vice Provost and Dean of Graduate Studies °c 2005 Lorenzo Mannelli Contents List of Figures vi Abstract vii Dedication viii Acknowledgments ix I The Holographic Principle 1 1 Introduction 2 2 Entropy Bounds for Black Holes 6 2.1 Black Holes Thermodynamics ........................ 6 2.1.1 Area Theorem ............................ 7 2.1.2 No-hair Theorem ........................... 7 2.2 Bekenstein Entropy and the Generalized Second Law ........... 8 2.2.1 Hawking Radiation .......................... 10 2.2.2 Bekenstein Bound: Geroch Process . 12 2.2.3 Spherical Entropy Bound: Susskind Process . 12 2.2.4 Relation to the Bekenstein Bound . 13 3 Degrees of Freedom and Entropy 15 3.1 Degrees of Freedom .............................. 15 3.1.1 Fundamental System ......................... 16 3.2 Complexity According to Local Field Theory . 16 3.3 Complexity According to the Spherical Entropy Bound . 18 3.4 Why Local Field Theory Gives the Wrong Answer . 19 4 The Covariant Entropy Bound 20 4.1 Light-Sheets .................................. 20 iii 4.1.1 The Raychaudhuri Equation .................... 20 4.1.2 Orthogonal Null Hypersurfaces ................... 24 4.1.3 Light-sheet Selection ......................... 26 4.1.4 Light-sheet Termination ....................... 28 4.2 Entropy on a Light-Sheet .......................... 29 4.3 Formulation of the Covariant Entropy Bound . 30 5 Quantum Field Theory in Curved Spacetime 32 5.1 Scalar Field Quantization ......................... -
Renormalization: an Advanced Overview
ITP-UU-14/04 SPIN-14/04 HU-Mathematik-2014-01 HU-EP-14/01 Renormalization: an advanced overview Razvan Gurau1;2, Vincent Rivasseau3;2 and Alessandro Sfondrini4;5 1. CPHT - UMR 7644, CNRS, Ecole´ Polytechnique, 91128 Palaiseau cedex, France 2. Perimeter Institute for Theoretical Physics, 31 Caroline St. N, N2L 2Y5, Waterloo, ON, Canada 3. LPT - UMR 8627, CNRS, Universit´eParis 11, 91405 Orsay Cedex, France 4. Institute for Theoretical Physics and Spinoza Institute, Utrecht University, 3508 TD Utrecht, The Netherlands 5. Inst. f¨urMathematik & Inst. f¨urPhysik, Humboldt-Universit¨atzu Berlin IRIS Geb¨aude,Zum Grossen Windkanal 6, 12489 Berlin, Germany [email protected], [email protected], [email protected] Abstract We present several approaches to renormalization in QFT: the multi-scale analysis in perturbative renormalization, the functional methods `ala Wet- terich equation, and the loop-vertex expansion in non-perturbative renor- malization. While each of these is quite well-established, they go beyond standard QFT textbook material, and may be little-known to specialists of each other approach. This review is aimed at bridging this gap. Contents 1 Introduction 2 1.1 Axioms for an Euclidean quantum field theory . .3 4 1.2 The φd field theory . .5 1.3 Contents and plan of the review . .6 2 Useful tools 7 2.1 Graphs and combinatorial maps . .7 2.1.1 Generalities . .7 2.1.2 Forests, trees and plane trees . .9 2.1.3 Incidence, degree, adjacency and Laplacian matrices . 11 2.1.4 The symmetry factor . 13 2.2 Graph polynomials . -
Quantum Mechanics Propagator
Quantum Mechanics_propagator This article is about Quantum field theory. For plant propagation, see Plant propagation. In Quantum mechanics and quantum field theory, the propagator gives the probability amplitude for a particle to travel from one place to another in a given time, or to travel with a certain energy and momentum. In Feynman diagrams, which calculate the rate of collisions in quantum field theory, virtual particles contribute their propagator to the rate of the scattering event described by the diagram. They also can be viewed as the inverse of the wave operator appropriate to the particle, and are therefore often called Green's functions. Non-relativistic propagators In non-relativistic quantum mechanics the propagator gives the probability amplitude for a particle to travel from one spatial point at one time to another spatial point at a later time. It is the Green's function (fundamental solution) for the Schrödinger equation. This means that, if a system has Hamiltonian H, then the appropriate propagator is a function satisfying where Hx denotes the Hamiltonian written in terms of the x coordinates, δ(x)denotes the Dirac delta-function, Θ(x) is the Heaviside step function and K(x,t;x',t')is the kernel of the differential operator in question, often referred to as the propagator instead of G in this context, and henceforth in this article. This propagator can also be written as where Û(t,t' ) is the unitary time-evolution operator for the system taking states at time t to states at time t'. The quantum mechanical propagator may also be found by using a path integral, where the boundary conditions of the path integral include q(t)=x, q(t')=x' . -
Stochastic Gravity: Theory and Applications
Stochastic Gravity: Theory and Applications Bei Lok Hu Department of Physics University of Maryland College Park, Maryland 20742-4111 U.S.A. email: [email protected] http://www.physics.umd.edu/people/faculty/hu.html Enric Verdaguer Departament de Fisica Fonamental and C.E.R. in Astrophysics, Particles and Cosmology Universitat de Barcelona Av. Diagonal 647 08028 Barcelona Spain email: verdague@ffn.ub.es Accepted on 27 February 2004 Published on 11 March 2004 http://www.livingreviews.org/lrr-2004-3 Living Reviews in Relativity Published by the Max Planck Institute for Gravitational Physics Albert Einstein Institute, Germany Abstract Whereas semiclassical gravity is based on the semiclassical Einstein equation with sources given by the expectation value of the stress-energy tensor of quantum fields, stochastic semi- classical gravity is based on the Einstein–Langevin equation, which has in addition sources due to the noise kernel. The noise kernel is the vacuum expectation value of the (operator- valued) stress-energy bi-tensor which describes the fluctuations of quantum matter fields in curved spacetimes. In the first part, we describe the fundamentals of this new theory via two approaches: the axiomatic and the functional. The axiomatic approach is useful to see the structure of the theory from the framework of semiclassical gravity, showing the link from the mean value of the stress-energy tensor to their correlation functions. The functional approach uses the Feynman–Vernon influence functional and the Schwinger–Keldysh closed-time-path effective action methods which are convenient for computations. It also brings out the open systems concepts and the statistical and stochastic contents of the theory such as dissipation, fluctuations, noise, and decoherence. -
Euclidean Quantum Field Theory As Classical Statistical Mechanics
The P(d),Euclidean quantum field theory as classical statistical mechanics By F. GUERRA,L. ROSEN,and B. SIMON Part I of this paper including the Bibliography appeared at the end of the preceding issue of this journal. Part I1 I\'. Lattice Markov fields To date in constructive field theory, two types of ultraviolet cutoffs have been used [32]: 1) A smeared field, i.e., g(x) is replaced by $,(x) = \ h(x - y)$(y)dy, where h is some smooth positive approximation to the delta function; 2) Box and sharp momentum cutoff, i.e., g(x) is replaced by the periodic field Q~,~(X),which is obtained by approximating the Fourier integral defining g(x) by a finite Fourier sum. In this section we wish to introduce a new cutoff method in which Rd (space-imaginary time) is replaced by a lattice and the Laplacian A in the Euclidean propagator is approximated by a finite difference operator. The effect of this approximation is to replace the measure (11.25) by a perturbed Gaussian measure in a finite number of variables, q,, . ., q,, each associated with a lattice point: where the P, are semibounded polynomials and B is a positive-definite N x N matrix with nonpositive off-diagonal entries. There are two main advantages to this approximation which play a key role in our proof of correlation inequalities (5 V): First, it is locality preserving in the sense that U(g) is approximated by a sum C P,(q,) in which each term involves the field q, at only a single lattice point. -
Winter 2017/18)
Thorsten Ohl 2018-02-07 14:05:03 +0100 subject to change! i Relativistic Quantum Field Theory (Winter 2017/18) Thorsten Ohl Institut f¨urTheoretische Physik und Astrophysik Universit¨atW¨urzburg D-97070 W¨urzburg Personal Manuscript! Use at your own peril! git commit: c8138b2 Thorsten Ohl 2018-02-07 14:05:03 +0100 subject to change! i Abstract 1. Symmetrien 2. Relativistische Einteilchenzust¨ande 3. Langrangeformalismus f¨urFelder 4. Feldquantisierung 5. Streutheorie und S-Matrix 6. Eichprinzip und Wechselwirkung 7. St¨orungstheorie 8. Feynman-Regeln 9. Quantenelektrodynamische Prozesse in Born-N¨aherung 10. Strahlungskorrekturen (optional) 11. Renormierung (optional) Thorsten Ohl 2018-02-07 14:05:03 +0100 subject to change! i Contents 1 Introduction1 Lecture 01: Tue, 17. 10. 2017 1.1 Limitations of Quantum Mechanics (QM).......... 1 1.2 (Special) Relativistic Quantum Field Theory (QFT)..... 2 1.3 Limitations of QFT...................... 3 2 Symmetries4 2.1 Principles ofQM....................... 4 2.2 Symmetries inQM....................... 6 2.3 Groups............................. 6 Lecture 02: Wed, 18. 10. 2017 2.3.1 Lie Groups....................... 7 2.3.2 Lie Algebras...................... 8 2.3.3 Homomorphisms.................... 8 2.3.4 Representations.................... 9 2.4 Infinitesimal Generators.................... 10 2.4.1 Unitary and Conjugate Representations........ 12 Lecture 03: Tue, 24. 10. 2017 2.5 SO(3) and SU(2) ........................ 13 2.5.1 O(3) and SO(3) .................... 13 2.5.2 SU(2) .......................... 15 2.5.3 SU(2) ! SO(3) .................... 16 2.5.4 SO(3) and SU(2) Representations........... 17 Lecture 04: Wed, 25. 10. 2017 2.6 Lorentz- and Poincar´e-Group................ -
Lorentzian Methods in Conformal Field Theory
Lorentzian methods in Conformal Field Theory by Slava Rychkov IHES & ENS Table of contents 1 Motivation . 1 2 Introduction to Euclidean CFT in d > 2 . 2 2.1 Conformal invariance . 2 2.2 Constraints on correlation functions . 4 2.3 Operator product expansion (OPE) and crossing . 5 2.4 Cutting and gluing picture . 7 2.5 Evidence for the validity of bootstrap axioms . 7 3 Other axiomatic schemes . 9 3.1 Wightman axioms . 9 3.2 Analytic continuation of Wightman functions . 10 3.2.1 Relation to random distributions . 14 3.3 Osterwalder-Schrader theorem . 14 3.3.1 Some ideas about the proof . 15 3.3.2 Check of growth condition for gaussian scalar field . 16 4 Towards CFT Osterwalder-Schrader theorem . 16 4.1 What do we need to show . 16 4.2 2pt and 3pt function examples . 17 4.3 Vladimirov's theorem . 18 5 The 4pt function . 20 5.1 The coordinate . 22 5.1.1 Powerlaw bound on the approach 1 . 24 5.2 General 2d case . j. .j !. 25 5.3 General case . 27 Bibliography . 30 1 Motivation In recent years there was a huge progress in our understanding and applications of conformal fields theories in d >2 dimensions, thanks to the revival of the conformal bootstrap [1]. Much of this work is in the Euclidean space, but also the Minkowski space makes its appearance and actually has a lot of applications. This raises the following two puzzles. 1 2 Section 2 Q1.Why is this useful? 3d CFTs make predictions to second-order thermody- namic phase transitions in 3d systems (e.g. -
INFORMATION– CONSCIOUSNESS– REALITY How a New Understanding of the Universe Can Help Answer Age-Old Questions of Existence the FRONTIERS COLLECTION
THE FRONTIERS COLLECTION James B. Glattfelder INFORMATION– CONSCIOUSNESS– REALITY How a New Understanding of the Universe Can Help Answer Age-Old Questions of Existence THE FRONTIERS COLLECTION Series editors Avshalom C. Elitzur, Iyar, Israel Institute of Advanced Research, Rehovot, Israel Zeeya Merali, Foundational Questions Institute, Decatur, GA, USA Thanu Padmanabhan, Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune, India Maximilian Schlosshauer, Department of Physics, University of Portland, Portland, OR, USA Mark P. Silverman, Department of Physics, Trinity College, Hartford, CT, USA Jack A. Tuszynski, Department of Physics, University of Alberta, Edmonton, AB, Canada Rüdiger Vaas, Redaktion Astronomie, Physik, bild der wissenschaft, Leinfelden-Echterdingen, Germany THE FRONTIERS COLLECTION The books in this collection are devoted to challenging and open problems at the forefront of modern science and scholarship, including related philosophical debates. In contrast to typical research monographs, however, they strive to present their topics in a manner accessible also to scientifically literate non-specialists wishing to gain insight into the deeper implications and fascinating questions involved. Taken as a whole, the series reflects the need for a fundamental and interdisciplinary approach to modern science and research. Furthermore, it is intended to encourage active academics in all fields to ponder over important and perhaps controversial issues beyond their own speciality. Extending from quantum physics and relativity to entropy, conscious- ness, language and complex systems—the Frontiers Collection will inspire readers to push back the frontiers of their own knowledge. More information about this series at http://www.springer.com/series/5342 For a full list of published titles, please see back of book or springer.com/series/5342 James B. -
Towards a Construction of a Quantum Field Theory in Four Dimensions
Towards a construction of a quantum field theory in four dimensions Harald Grosse1 and Raimar Wulkenhaar2 1 Fakult¨atf¨urPhysik, Universit¨atWien Boltzmanngasse 5, A-1090 Wien, Austria 2 Mathematisches Institut der Westf¨alischenWilhelms-Universit¨at Einsteinstraße 62, D-48149 M¨unster,Germany Abstract 4 We summarise our recent construction of the λφ4-model on four- dimensional Moyal space. In the limit of infinite noncommutativity, this model is exactly solvable in terms of the solution of a non-linear integral equation. Surprisingly, this limit describes Schwinger functions of a Euclidean quantum field theory on standard R4 which satisfy the easy Osterwalder-Schrader axioms boundedness, invariance and sym- metry. We prove that the decisive reflection positivity axiom is, for the 2-point function, equivalent to the question whether or not the solution of the integral equation is a Stieltjes function. A numerical investigation leaves no doubt that this is true for coupling constants λc < λ ≤ 0 with λc ≈ −0:39. 1 Introduction 1.1 Rigorous quantum field theories Perturbatively renormalised quantum field theory is an enormous phenomeno- logical success, a success which lacks a mathematical understanding. The per- turbation series is at best an asymptotic expansion which cannot converge at physical coupling constants. Some physical effects such as confinement are out of reach for perturbation theory. In two, and partly three dimensions, meth- ods of constructive physics [GJ87, Riv91], often combined with the Euclidean approach [Sch59, OS73, OS75], were used to rigorously establish existence and certain properties of quantum field theory models. In four dimensions there has been little success so far. -
DENSITY, TEMPERATURE and CONTINUUM STRONG QCD Craig D. Roberts A
ANL-PHY-9530-TH-2000 CORE Metadata, citationnucl-th/0005064 and similar papers at core.ac.uk Provided by CERN Document Server DYSON-SCHWINGER EQUATIONS: DENSITY, TEMPERATURE AND CONTINUUM STRONG QCD Craig D. Roberts and Sebastian M. Schmidt Physics Division, Building 203, Argonne National Laboratory, Argonne, IL 60439-4843, USA e-mail: [email protected] [email protected] ABSTRACT Continuum strong QCD is the application of models and continuum quantum field theory to the study of phenomena in hadronic physics, which includes; e.g., the spectrum of QCD bound states and their in- teractions; and the transition to, and properties of, a quark gluon plasma. We provide a contemporary perspective, couched primarily in terms of the Dyson-Schwinger equations but also making compar- isons with other approaches and models. Our discourse provides a practitioners’ guide to features of the Dyson-Schwinger equations [such as confinement and dynamical chiral symmetry breaking] and canvasses phenomenological applications to light meson and baryon properties in cold, sparse QCD. These provide the foundation for an extension to hot, dense QCD, which is probed via the introduc- tion of the intensive thermodynamic variables: chemical potential and temperature. We describe order parameters whose evolution signals deconfinement and chiral symmetry restoration, and chronicle their use in demarcating the quark gluon plasma phase boundary and characterising the plasma’s properties. Hadron traits change in an equilibrated plasma. We exemplify this and discuss putative signals of the effects. Finally, since plasma formation is not an equilibrium process, we discuss recent developments in kinetic theory and its application to describing the evolution from a relativistic heavy ion collision to an equilibrated quark gluon plasma.