Introduction to Chiral Symmetry in QCD
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QCD Theory 6Em2pt Formation of Quark-Gluon Plasma In
QCD theory Formation of quark-gluon plasma in QCD T. Lappi University of Jyvaskyl¨ a,¨ Finland Particle physics day, Helsinki, October 2017 1/16 Outline I Heavy ion collision: big picture I Initial state: small-x gluons I Production of particles in weak coupling: gluon saturation I 2 ways of understanding glue I Counting particles I Measuring gluon field I For practical phenomenology: add geometry 2/16 A heavy ion event at the LHC How does one understand what happened here? 3/16 Concentrate here on the earliest stage Heavy ion collision in spacetime The purpose in heavy ion collisions: to create QCD matter, i.e. system that is large and lives long compared to the microscopic scale 1 1 t L T > 200MeV T T t freezefreezeout out hadronshadron in eq. gas gluonsquark-gluon & quarks in eq. plasma gluonsnonequilibrium & quarks out of eq. quarks, gluons colorstrong fields fields z (beam axis) 4/16 Heavy ion collision in spacetime The purpose in heavy ion collisions: to create QCD matter, i.e. system that is large and lives long compared to the microscopic scale 1 1 t L T > 200MeV T T t freezefreezeout out hadronshadron in eq. gas gluonsquark-gluon & quarks in eq. plasma gluonsnonequilibrium & quarks out of eq. quarks, gluons colorstrong fields fields z (beam axis) Concentrate here on the earliest stage 4/16 Color charge I Charge has cloud of gluons I But now: gluons are source of new gluons: cascade dN !−1−O(αs) d! ∼ Cascade of gluons Electric charge I At rest: Coulomb electric field I Moving at high velocity: Coulomb field is cloud of photons -
3. Models of EWSB
The Higgs Boson and Electroweak Symmetry Breaking 3. Models of EWSB M. E. Peskin Chiemsee School September 2014 In this last lecture, I will take up a different topic in the physics of the Higgs field. In the first lecture, I emphasized that most of the parameters of the Standard Model are associated with the couplings of the Higgs field. These parameters determine the Higgs potential, the spectrum of quark and lepton masses, and the structure of flavor and CP violation in the weak interactions. These parameters are not computable within the SM. They are inputs. If we want to compute these parameters, we need to build a deeper and more predictive theory. In particular, a basic question about the SM is: Why is the SU(2)xU(1) gauge symmetry spontaneously broken ? The SM cannot answer this question. I will discuss: In what kind of models can we answer this question ? For orientation, I will present the explanation for spontaneous symmetry breaking in the SM. We have a single Higgs doublet field ' . It has some potential V ( ' ) . The potential is unknown, except that it is invariant under SU(2)xU(1). However, if the theory is renormalizable, the potential must be of the form V (')=µ2 ' 2 + λ ' 4 | | | | Now everything depends on the sign of µ 2 . If µ2 > 0 the minimum of the potential is at ' =0 and there is no symmetry breaking. If µ 2 < 0 , the potential has the form: and there is a minimum away from 0. That’s it. Don’t ask any more questions. -
The Positons of the Three Quarks Composing the Proton Are Illustrated
The posi1ons of the three quarks composing the proton are illustrated by the colored spheres. The surface plot illustrates the reduc1on of the vacuum ac1on density in a plane passing through the centers of the quarks. The vector field illustrates the gradient of this reduc1on. The posi1ons in space where the vacuum ac1on is maximally expelled from the interior of the proton are also illustrated by the tube-like structures, exposing the presence of flux tubes. a key point of interest is the distance at which the flux-tube formaon occurs. The animaon indicates that the transi1on to flux-tube formaon occurs when the distance of the quarks from the center of the triangle is greater than 0.5 fm. again, the diameter of the flux tubes remains approximately constant as the quarks move to large separaons. • Three quarks indicated by red, green and blue spheres (lower leb) are localized by the gluon field. • a quark-an1quark pair created from the gluon field is illustrated by the green-an1green (magenta) quark pair on the right. These quark pairs give rise to a meson cloud around the proton. hEp://www.physics.adelaide.edu.au/theory/staff/leinweber/VisualQCD/Nobel/index.html Nucl. Phys. A750, 84 (2005) 1000000 QCD mass 100000 Higgs mass 10000 1000 100 Mass (MeV) 10 1 u d s c b t GeV HOW does the rest of the proton mass arise? HOW does the rest of the proton spin (magnetic moment,…), arise? Mass from nothing Dyson-Schwinger and Lattice QCD It is known that the dynamical chiral symmetry breaking; namely, the generation of mass from nothing, does take place in QCD. -
Symmetries of the Strong Interaction
Symmetries of the strong interaction H. Leutwyler University of Bern DFG-Graduiertenkolleg ”Quanten- und Gravitationsfelder” Jena, 19. Mai 2009 H. Leutwyler – Bern Symmetries of the strong interaction – p. 1/33 QCD with 3 massless quarks As far as the strong interaction goes, the only difference between the quark flavours u,d,...,t is the mass mu, md, ms happen to be small For massless fermions, the right- and left-handed components lead a life of their own Fictitious world with mu =md =ms =0: QCD acquires an exact chiral symmetry No distinction between uL,dL,sL, nor between uR,dR,sR Hamiltonian is invariant under SU(3) SU(3) ⇒ L× R H. Leutwyler – Bern Symmetries of the strong interaction – p. 2/33 Chiral symmetry of QCD is hidden Chiral symmetry is spontaneously broken: Ground state is not symmetric under SU(3) SU(3) L× R symmetric only under the subgroup SU(3)V = SU(3)L+R Mesons and baryons form degenerate SU(3)V multiplets ⇒ and the lowest multiplet is massless: Mπ± =Mπ0 =MK± =MK0 =MK¯ 0 =Mη =0 Goldstone bosons of the hidden symmetry H. Leutwyler – Bern Symmetries of the strong interaction – p. 3/33 Spontane Magnetisierung Heisenbergmodell eines Ferromagneten Gitter von Teilchen, Wechselwirkung zwischen Spins Hamiltonoperator ist drehinvariant Im Zustand mit der tiefsten Energie zeigen alle Spins in dieselbe Richtung: Spontane Magnetisierung Grundzustand nicht drehinvariant ⇒ Symmetrie gegenüber Drehungen gar nicht sichtbar Symmetrie ist versteckt, spontan gebrochen Goldstonebosonen in diesem Fall: "Magnonen", "Spinwellen" Haben keine Energielücke: ω 0 für λ → → ∞ Nambu realisierte, dass auch in der Teilchenphysik Symmetrien spontan zusammenbrechen können H. -
Goldstone Theorem, Higgs Mechanism
Introduction to the Standard Model Lecture 12 Classical Goldstone Theorem and Higgs Mechanism The Classical Goldstone Theorem: To each broken generator corresponds a massless field (Goldstone boson). Proof: 2 ∂ V Mij = ∂φi∂φj φ~= φ~ h i V (φ~)=V (φ~ + iεaT aφ~) ∂V =V (φ~)+ iεaT aφ~ + ( ε 2) ∂φj O | | ∂ ∂V a Tjlφl =0 ⇒∂φk ∂φj 2 ∂ ∂V a ∂ V a ∂V a Til φl = Tjlφl + Tik ∂φk ∂φi ∂φi∂φj ∂φi φ~= φ~ h i 0= M T a φ +0 ki il h li =~0i | 6 {z } If T a is a broken generator one has T a φ~ = ~0 h i 6 ⇒ Mik has a null eigenvector null eigenvalues massless particle since the eigenvalues of the mass matrix are the particle⇒ masses. ⇒ We now combine the concept of a spontaneously broken symmetry to a gauge theory. The Higgs Mechanism for U(1) gauge theory Consider µ 2 2 1 µν = D φ∗ D φ µ φ∗φ λ φ∗φ F F L µ − − − 4 µν µν µ ν ν µ with Dµ = ∂µ + iQAµ and F = ∂ A ∂ A . Gauge symmetry here means invariance under Aµ Aµ ∂µΛ. − → − 2 2 2 case a) unbroken case, µ > 0 : V (φ)= µ φ∗φ + λ φ∗φ with a minimum at φ = 0. The ground state or vaccuum is U(1) symmetric. The corresponding theory is known as Scalar Electrodynamics of a massive spin-0 boson with mass µ and charge Q. 1 case b) nontrivial vaccuum case 2 µ 2 v iα V (φ) has a minimum for 2 φ∗φ = − = v which gives φ = e . -
2.4 Spontaneous Chiral Symmetry Breaking
70 Hadrons 2.4 Spontaneous chiral symmetry breaking We have earlier seen that renormalization introduces a scale. Without a scale in the theory all hadrons would be massless (at least for vanishing quark masses), so the anomalous breaking of scale invariance is a necessary ingredient to understand their nature. The second ingredient is spontaneous chiral symmetry breaking. We will see that this mechanism plays a quite important role in the light hadron spectrum: it is not only responsible for the Goldstone nature of the pions, but also the origin of the 'constituent quarks' which produce the typical hadronic mass scales of 1 GeV. ∼ Spontaneous symmetry breaking. Let's start with some general considerations. Suppose 'i are a set of (potentially composite) fields which transform nontrivially under some continuous global symmetry group G. For an infinitesimal transformation we have δ'i = i"a(ta)ij 'j, where "a are the group parameters and ta the generators of the Lie algebra of G in the representation to which the 'i belong. Let's call the representation matrices Dij(") = exp(i"ata)ij. The quantum-field theoretical version of this relation is ei"aQa ' e−i"aQa = D−1(") ' [Q ;' ] = (t ) ' ; (2.128) i ij j , a i − a ij j where the charge operators Qa form a representation of the algebra on the Hilbert space. (An example of this is Eq. (2.47).) If the symmetry group leaves the vacuum invariant, ei"aQa 0 = 0 , then all generators Q must annihilate the vacuum: Q 0 = 0. Hence, j i j i a aj i when we take the vacuum expectation value (VEV) of this equation we get 0 ' 0 = D−1(") 0 ' 0 : (2.129) h j ij i ij h j jj i If the 'i had been invariant under G to begin with, this relation would be trivially −1 satisfied. -
Doi:10.5281/Zenodo.2566644
Higgs, dark sector and the vacuum: From Nambu-Goldstone bosons to massive particles via the hydrodynamics of a doped vacuum. Marco Fedi * v2, February 16, 2019 Abstract is the energy density of the vacuum, whose units corre- spond to pressure (J=m3 = Pa), hence justifying the re- Here the physical vacuum is treated as a superfluid, fun- pulsive action of dark energy. One can describe the damental quantum scalar field, coinciding with dark en- virtual pairs forming and annihilating in quantum vac- ergy and doped with particle dark matter, able to pro- uum – considered as a fundamental, scalar, quantum duce massive particles and interactions via a hydrody- field – as vortex-antivortex pairs of vacuum’s quanta, namic reinterpretation of the Higgs mechanism. Here via a mechanism analogous to the Higgs mechanism, the Nambu-Goldstone bosons are circularly polarized where phonons in the superfluid vacuum are the Nambu- phonons around the edge of the Brillouin zone of vac- Goldstone bosons, which here trigger quantized vortices uum’s quasi-lattice and they give mass to particles by trig- and the mass-acquisition process, due to the interaction gering quantized vortices, whose dynamics reproduces with diffused particle dark matter [2], which acts as a any possible spin. Doped vortices also exert hydrody- dopant of the superfluid vacuum and that could be the rea- namic forces which may correspond to fundamental in- son for vacuum dilatancy, described and proven in [22]. teractions. Hence, is the Higgs field really something different or along with the dark sector and quantum vacuum we are Keywords— quantum vacuum; dilatant vacuum; dark en- using different names to refer to the same thing? Dilatant ergy; dark matter; Higgs mechanism; spin; fundamental vacuum [22] could refer to the possible apparent viscosity interactions. -
Exotic Goldstone Particles: Pseudo-Goldstone Boson and Goldstone Fermion
Exotic Goldstone Particles: Pseudo-Goldstone Boson and Goldstone Fermion Guang Bian December 11, 2007 Abstract This essay describes two exotic Goldstone particles. One is the pseudo- Goldstone boson which is related to spontaneous breaking of an approximate symmetry. The other is the Goldstone fermion which is a natural result of spontaneously broken global supersymmetry. Their realization and implication in high energy physics are examined. 1 1 Introduction In modern physics, the idea of spontaneous symmetry breaking plays a crucial role in understanding various phenomena such as ferromagnetism, superconductivity, low- energy interactions of pions, and electroweak unification of the Standard Model. Nowadays, broken symmetry and order parameters emerged as unifying theoretical concepts are so universal that they have become the framework for constructing new theoretical models in nearly all branches of physics. For example, in particle physics there exist a number of new physics models based on supersymmetry. In order to explain the absence of superparticle in current high energy physics experiment, most of these models assume the supersymmetry is broken spontaneously by some underlying subtle mechanism. Application of spontaneous broken symmetry is also a common case in condensed matter physics [1]. Some recent research on high Tc superconductor [2] proposed an approximate SO(5) symmetry at least over part of the theory’s parameter space and the detection of goldstone bosons resulting from spontaneous symmetry breaking would be a ’smoking gun’ for the existence of this SO(5) symmetry. From the Goldstone’s Theorem [3], we know that there are two explicit common features among Goldstone’s particles: (1) they are massless; (2) they obey Bose-Einstein statistics i.e. -
The Symmetries of QCD (And Consequences)
Introduction QCD Lattice Physics Challenges The symmetries of QCD (and consequences) Sinéad M. Ryan Trinity College Dublin antum Universe Symposium, Groningen, March 2018 Understand nature in terms of fundamental building blocks Introduction QCD Lattice Physics Challenges The Rumsfeld Classification “As we know, there are known knowns. There are things we know we know. We also know, there are known unknowns. That is to say we know there are some things we do not know. But there are also unknown unknowns, the ones we don’t know we don’t know.” – Donald Rumsfeld, U.S. Secretary of Defense, Feb. 12, 2002 Introduction QCD Lattice Physics Challenges Some known knowns antum ChromoDynamics - the theory of quarks and gluons Embarassingly successful Precision tests of SM can reveal new physics - more important than ever! Why focus on the 4.6%? QCD is the only experimentally studied strongly-interacting quantum field theory - highlights many subtleties. A paradigm for other strongly-interacting theories in BSM physics. There are still puzzles and surprises in this well-studied arena. Introduction QCD Lattice Physics Challenges What is QCD? A gauge theory for SU(3) colour interactions of quarks and gluons: Color motivated by experimental measurements; not a “measureable” quantum number. Lagrangian invariant under colour transformations. Elementary fields: arks Gluons 8 colour a = 1,..., 3 < colour a = 1,..., 8 (q )a spin 1/2 Dirac fermions Aa α f μ spin 1bosons : avour f = u, d, s, c, b, t 1 L = ¯q i muD m q Ga Ga f γ μ f f μν μν − − 4 with Ga = Aa Aa + gf abcAb Ac μν ∂μ ν ∂ν μ μ ν and − i μD q = μ i + gAa ta q γ μ γ ∂μ μ Generates gluon self-interactions - might expect consequences! Introduction QCD Lattice Physics Challenges Elucidating the effect of the self-interactions: QED vs QCD In QED: coupling runs and bare e is − screened at large distances - reducing Same but dierent for QCD with anti-screening from gluon interactions dominates! Asymptotic freedom Coupling small at high energies - energetic quarks are (almost) free. -
Goldstone Bosons in a Crystalline Chiral Phase
Goldstone Bosons in a Crystalline Chiral Phase Goldstone Bosonen in einer Kristallinen Chiralen Phase Zur Erlangung des Grades eines Doktors der Naturwissenschaften (Dr. rer. nat.) genehmigte Dissertation von M.Sc. Marco Schramm, Tag der Einreichung: 29.06.2017, Tag der Prüfung: 24.07.2017 Darmstadt 2017 — D 17 1. Gutachten: PD Dr. Michael Buballa 2. Gutachten: Prof. Dr. Jens Braun Fachbereich Physik Institut für Kernphysik NHQ Goldstone Bosons in a Crystalline Chiral Phase Goldstone Bosonen in einer Kristallinen Chiralen Phase Genehmigte Dissertation von M.Sc. Marco Schramm, 1. Gutachten: PD Dr. Michael Buballa 2. Gutachten: Prof. Dr. Jens Braun Tag der Einreichung: 29.06.2017 Tag der Prüfung: 24.07.2017 Darmstadt 2017 — D 17 Bitte zitieren Sie dieses Dokument als: URN: urn:nbn:de:tuda-tuprints-66977 URL: http://tuprints.ulb.tu-darmstadt.de/6697 Dieses Dokument wird bereitgestellt von tuprints, E-Publishing-Service der TU Darmstadt http://tuprints.ulb.tu-darmstadt.de [email protected] Die Veröffentlichung steht unter folgender Creative Commons Lizenz: Namensnennung – Keine kommerzielle Nutzung – Keine Bearbeitung 4.0 International https://creativecommons.org/licenses/by-nc-nd/4.0/ Abstract The phase diagram of strong interaction matter is expected to exhibit a rich structure. Different models have shown, that crystalline phases with a spatially varying chiral condensate can occur in the regime of low temperatures and moderate densities, where they replace the first-order phase transition found for spatially constant order parameters. We investigate this inhomogeneous phase, where in addition to the chiral symmetry, transla- tional and rotational symmetry are broken as well, in a two flavor Nambu–Jona-Lasinio model. -
Ft». 421* Clffis-Lh'- Fjf.F.Ol
ClffiS-lH'- fjf.f.Ol THE ABELIAN HIGGS KIEBLE MODEL. UNITARITY OF THE S- OPERATOR. C. BECCHI* by A. ROUET '•"• R. STORA Centre de Physique Théorique CNRS Marseille. : Results concerning the renormali nation of the abelian Higgs Kibble model in the 't Hooft gauges are presented. A direct combinatorial proof of the unitarity of the physical S -operator is described. ft». 421* x On leave of absence from the University of Genova xx. Boursier de thèse CEA Postal Address i Centre de Physique Théorique 31. chemin J. Aiguier 13274 MARSEILLE CEDEX 2 The Higgs-Kibble model [IJ provides the best known exception to the Goldstone theorem I 2 j concerning the phenomenon of spontaneous symmetry breaking in local field theory. If zero mass vector particles are present in the unbroken theory the degrees of freedom corresponding to the Goldstone boson may be lost, the vector particles becoming massive. In order to discuss this phenomenon in the framework of renormalized quantum field theory [3,4,5j it is necessary to introduce a certain number of non physical degrees of freedom, some of which are associated with negative norm one-particle states. The number of non physical fields and their properties depend on the choice of the gauge [3,4,5,6] , It is however convenient to exclude gauges such as the Stueckelberg gauge which lead [sj to massless particles, in order to avoid unnecessary infrared problems. A choice of gauge satisfying this requirement has been proposed by G. t'Hoofc 14 . In this gauge, according to the Faddeev-Popov fTJ prescription, a system of anticommuting scalar ghost fields must be introduced, which are coupled to the remaining fields. -
CHIRAL DYNAMICS 1 Introduction the Low Energy Properties of the Strong Interactions Are Governed by a Chi- Ral Symmetry. For
CORE Metadata, citation and similar papers at core.ac.uk Provided by CERN Document Server CHIRAL DYNAMICS H. LEUTWYLER Institute for Theoretical Physics, University of Bern, Sidlerstr. 5, CH-3012 Bern, Switzerland The effective field theory relevant for the analysis of QCD at low energies is re- viewed. The foundations of the method are discussed in some detail and a few illustrative examples are described. 1 Introduction The low energy properties of the strong interactions are governed by a chi- ral symmetry. For this reason, the physics of the degrees of freedom that are relevant in this domain is referred to as chiral dynamics and the corre- sponding effective field theory is called chiral perturbation theory. Effective field theories play an increasingly important role in physics, not only in the context of the strong interactions, but also in other areas: heavy quarks, elec- troweak symmetry breaking, spin models, magnetism, etc. In fact, one of the remarkable features of effective Lagrangians is their universality. A compound like La2CuO4 which develops two-dimensional antiferromagnetic layers and ex- hibits superconductivity up to rather high temperatures can be described by an effective field theory that closely resembles the one relevant for the strong interactions! The reason is that the effective theory only exploits the symme- try properties of the underlying theory and does not invoke the dynamics of the fields occurring therein. In fact, the development of chiral perturbation theory started in the 1960’s, at a time when it was rather unclear whether the strong interactions could at all be described in terms of local fields.