Interplay Between Chiral Dynamics and Repulsive Interactions

Total Page:16

File Type:pdf, Size:1020Kb

Interplay Between Chiral Dynamics and Repulsive Interactions Interplay between chiral dynamics and repulsive interactions Michal Marczenko,∗ Krzysztof Redlich, and Chihiro Sasaki Institute of Theoretical Physics, University of Wroc law, plac Maksa Borna 9, PL-50204 Wroc law, Poland (Dated: January 1, 2021) We investigate fluctuations of the net-baryon number density in hot hadronic matter. We discuss the interplay between chiral dynamics and repulsive interactions and their influence on the properties of these fluctuations near the chiral crossover. The chiral dynamics is modeled by the parity doublet Lagrangian that incorporates the attractive and repulsive interactions mediated via the exchange of scalar and vector mesons, respectively. The mean-field approximation is employed to account for chiral criticality. We focus on the properties and systematics of the cumulants of the net- baryon number density up to the sixth order. It is shown that the higher-order cumulants exhibit a substantial suppression in the vicinity of the chiral phase transition due to the presence of repulsive interactions. We find, however, that the characteristic properties of cumulants near the chiral crossover observed in lattice QCD results are entirely linked to the critical chiral dynamics and, in general, cannot be reproduced in phenomenological models, which account only for effective repulsive interactions via excluded-volume corrections or van-der-Waals type interactions. Consequently, a description of the higher-order cumulants of the net-baryon density in the chiral crossover requires a self-consistent treatment of the chiral in-medium effects and repulsive interactions. I. INTRODUCTION of QCD is well-described by the hadron resonance gas (HRG) model [40, 41]. Since the fundamental quarks Establishing the thermodynamic properties of strongly and gluons are confined, it is to be expected that at interacting matter, described by quantum chromody- low temperatures the QCD partition function is domi- namics (QCD), is one of the key directions in modern nated by the contribution of hadrons. The HRG model high-energy physics. At vanishing density, the first- describes well the LQCD data below the crossover tran- principles calculations of lattice QCD (LQCD) provide sition to a quark-gluon plasma, as well as the hadron a reliable description of the equation of state (EoS) and yields in heavy-ion collisions [41]. Different extensions fluctuations of conserved charges [1{4]. There, the EoS of the HRG model have been proposed to quantify the exhibits a smooth crossover from confined hadronic mat- LQCD EoS and various fluctuation observable up to near ter to a deconfined quark-gluon plasma, which is linked chiral-crossover. They account for consistent implemen- to the color deconfinement and the restoration of chiral tation of hadronic interactions within the S-matrix ap- symmetry [5, 6]. However, the nature of the EoS at finite proach [42{46], a more complete implementation or a density is still not resolved by LQCD, owing to the sign continuously growing exponential mass spectrum and/or problem, and remains an open question. possible repulsive interactions among constituents [47{ The LQCD results [7{9] exhibit a clear manifestation 53]. Recently, an interesting suggestion was made that of the parity doubling structure for the low-lying baryons deviations of the LQCD data on higher-order fluctuations around the chiral crossover. The masses of the positive- of net-baryon number density from the HRG baseline in parity ground states are found to be rather temperature- the near vicinity of the chiral transition can be attributed independent, while the masses of negative-parity states to repulsive interactions among constituent hadrons [54]. drop substantially when approaching the chiral crossover Fluctuations of conserved charges are known to be aus- temperature Tc. The parity doublet states become al- picious observable for the search of the chiral-critical be- most degenerate with a finite mass in the vicinity of the havior at the QCD phase boundary [55{57], and chem- arXiv:2012.15535v1 [hep-ph] 31 Dec 2020 chiral crossover. Even though these LQCD results are ical freeze-out of produced hadrons in heavy-ion colli- still not obtained in the physical limit, the observed be- sions [58{63]. In particular, fluctuations have been pro- havior of parity partners is likely an imprint of the chi- posed to probe the QCD critical point in the beam energy ral symmetry restoration in the baryonic sector of QCD. scan (BES) programs at the Relativistic Heavy Ion Col- Such properties of the chiral partners can be described in lider (RHIC) at BNL and the Super Proton Synchrotron the framework of the parity doublet model [10{12]. The (SPS) at CERN, as well as the remnants of the O(4) crit- model has been applied to hot and dense hadronic mat- icality at vanishing and finite baryon densities [63{66]. ter, neutron stars, as well as the vacuum phenomenology of QCD [13{39]. In this work, we analyze the properties and systematics It is already confirmed, that at small net-baryon num- of the fluctuations of conserved charges in the context of ber density, the thermodynamics of the confined phase the parity doublet model, which incorporates the chiral symmetry restoration and repulsive interactions via the exchange of the scalar and vector mesons, respectively. To account for critical behavior, the mean-field approxi- ∗ [email protected] mation is employed, which contains basic features of the 2 O(4) criticality, albeit with different critical exponents. the vector field, and the potentials read We study the behavior of the second- and higher-order cumulants of the net-baryon number density up to the λ2 λ4 2 λ6 3 Vσ = − Σ + Σ − Σ − σ, (4a) sixth order, as well as the bulk equation of state. It 2 4 6 is systematically examined to what extent the thermal m2 V = − ! ! !µ. (4b) behaviors are dominated by the chiral criticality and re- ! 2 µ pulsive interactions. 2 2 2 4 2 This paper is organized as follows. In Sec. II, we in- where Σ = σ + π , λ2 = λ4fπ − λ6fπ − mπ, and 2 troduce the parity doublet model. In Sec. III, we discuss = mπfπ. mπ and m! are the π and ! meson masses, the structure of the higher-order cumulants of the net- respectively, and fπ is the pion decay constant. Note baryon number density. In Sec. IV, we present results on that the chiral symmetry is explicitly broken by the lin- the equation of state and the higher-order cumulants of ear term in σ in Eq. (4a). the net-baryon number density. Finally, Sec. V is devoted The full Lagrangian of the parity doublet model is then to summary and conclusions. L = LN + LM . (5) In the diagonal basis, the masses of the chiral partners, II. PARITY DOUBLET MODEL N±, are given by q 1 2 2 2 In the conventional Gell-Mann{Levy model of mesons m± = (g1 + g2) σ + 4m0 ∓ (g1 − g2) σ . (6) and nucleons [67], the nucleon mass is entirely generated 2 by the non-vanishing expectation value of the sigma field. From Eq. (6), it is clear that, in contrast to the naive Thus, the nucleon inevitably becomes massless when the assignment under chiral symmetry, the chiral symmetry chiral symmetry gets restored. This is led by the partic- breaking generates only the splitting between the two ular chirality-assignment to the nucleon parity doublers, masses. When the symmetry is restored, the masses be- where the nucleons are assumed to be transformed in the come degenerate, m±(σ = 0) = m0. same way as the quarks are under chiral rotations. To investigate the properties of strongly-interacting More general allocation of the left- and right-handed matter, we adopt a mean-field approximation [68]. Ro- chiralities to the nucleons, the mirror assignment, was tational invariance requires that the spatial component proposed in [10]. This allows an explicit mass-term for #1 of the !µ field vanishes, namely h!i = 0 . Parity the nucleons, and consequently, the nucleons stay mas- conservation on the other hand dictates hπi = 0. The sive at the chiral restoration point. For more details, see mean-field thermodynamic potential of the parity dou- Refs. [10{12]. blet model reads In the mirror assignment, under SU(2) × SU(2) ro- L R X tation, two chiral fields 1 and 2 are transformed as Ω = Ωx + Vσ + V!, (7) follows: x=± 1L ! L 1L; 1R ! R 1R, with (1) 2L ! R 2L; 2R ! L 2R, Z d3p Ω = γ T ln (1 − f ) + ln 1 − f¯ , (8) x x (2π)3 x x where i = iL + iR, L 2 SU(2)L and R 2 SU(2)R. The nucleon part of the Lagrangian in the mirror model where γ± = 2 × 2 denotes the spin-isospin degeneracy ¯ reads factor for both parity partners, and fx (fx) is the particle (antiparticle) Fermi-Dirac distribution function, ¯ ¯ ¯ ¯ LN = i 1@/ 1 + i 2@/ 2 + m0 1γ5 2 − 2γ5 1 ¯ ¯ 1 + g1 1 (σ + iγ5τ · π) 1 + g2 2 (σ − iγ5τ · π) 2 fx = ∗ , β(Ex−µ ) ¯ ¯ 1 + e − g! 1!/ 1 − g! 2!/ 2, (9) ¯ 1 (2) fx = ∗ , 1 + eβ(Ex+µ ) where g1, g2, and g! are the baryon-to-meson coupling with β being the inverse temperature, the dispersion rela- p 2 2 constants and m0 is a mass parameter. tion Ex = p + mx and the effective chemical potential ∗ The mesonic part of the Lagrangian reads µ = µB − g!!. 1 1 1 L = (@ σ)2 + (@ π)2 − (! )2 − V − V , (3) M 2 µ 2 µ 4 µν σ ! #1 Since !0 is the only non-zero component in the mean-field ap- proximation, we simply denote it by ! ≡ !. where !µν = @µ!ν − @ν !µ is the field-strength tensor of 0 3 2 m0 [MeV] m+ [MeV] m− [MeV] mπ [MeV] fπ [MeV] m! [MeV] mρ [MeV] λ4 λ6fπ g! g1 g2 850 939 1500 140 93 783 775 13.15 4.67 4.64 12.42 6.39 TABLE I.
Recommended publications
  • Chiral Matrix Model of the Semi-Quark Gluon Plasma in QCD
    BNL-113249-2016-JA Chiral matrix model of the semi-Quark Gluon Plasma in QCD Robert D. Pisarski, Vladimir V. Skokov Accepted for publication in Physical Review D August 2016 Physics Department/Nuclear Theory Group/Office of Science Brookhaven National Laboratory U.S. Department of Energy USDOE Office Of Science USDOE Office of Under Secretary for Science Notice: This manuscript has been authored by employees of Brookhaven Science Associates, LLC under Contract No. DE-SC0012704 with the U.S. Department of Energy. The publisher by accepting the manuscript for publication acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or any third party’s use or the results of such use of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof or its contractors or subcontractors. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof.
    [Show full text]
  • Chiral Magnetism: a Geometric Perspective
    SciPost Phys. 10, 078 (2021) Chiral magnetism: a geometric perspective Daniel Hill1, Valeriy Slastikov2 and Oleg Tchernyshyov1? 1 Department of Physics and Astronomy and Institute for Quantum Matter, Johns Hopkins University, Baltimore, MD 21218, USA 2 School of Mathematics, University of Bristol, Bristol BS8 1TW, UK ? [email protected] Abstract We discuss a geometric perspective on chiral ferromagnetism. Much like gravity be- comes the effect of spacetime curvature in theory of relativity, the Dzyaloshinski-Moriya interaction arises in a Heisenberg model with nontrivial spin parallel transport. The Dzyaloshinskii-Moriya vectors serve as a background SO(3) gauge field. In 2 spatial di- mensions, the model is partly solvable when an applied magnetic field matches the gauge curvature. At this special point, solutions to the Bogomolny equation are exact excited states of the model. We construct a variational ground state in the form of a skyrmion crystal and confirm its viability by Monte Carlo simulations. The geometric perspective offers insights into important problems in magnetism, e.g., conservation of spin current in the presence of chiral interactions. Copyright D. Hill et al. Received 15-01-2021 This work is licensed under the Creative Commons Accepted 25-03-2021 Check for Attribution 4.0 International License. Published 29-03-2021 updates Published by the SciPost Foundation. doi:10.21468/SciPostPhys.10.3.078 Contents 1 Introduction2 1.1 The specific problem: the skyrmion crystal2 1.2 The broader impact: geometrization of chiral magnetism3 2 Chiral magnetism: a geometric perspective4 2.1 Spin vectors4 2.2 Local rotations and the SO(3) gauge field5 2.3 Spin parallel transport and curvature5 2.4 Gauged Heisenberg model6 2.5 Spin conservation7 2.5.1 Pure Heisenberg model7 2.5.2 Gauged Heisenberg model8 2.6 Historical note9 3 Skyrmion crystal in a two-dimensional chiral ferromagnet9 3.1 Bogomolny states in the pure Heisenberg model 10 3.2 Bogomolny states in the gauged Heisenberg model 11 3.2.1 False vacuum 12 1 SciPost Phys.
    [Show full text]
  • Quantum Mechanics Quantum Chromodynamics (QCD)
    Quantum Mechanics_quantum chromodynamics (QCD) In theoretical physics, quantum chromodynamics (QCD) is a theory ofstrong interactions, a fundamental forcedescribing the interactions between quarksand gluons which make up hadrons such as the proton, neutron and pion. QCD is a type of Quantum field theory called a non- abelian gauge theory with symmetry group SU(3). The QCD analog of electric charge is a property called 'color'. Gluons are the force carrier of the theory, like photons are for the electromagnetic force in quantum electrodynamics. The theory is an important part of the Standard Model of Particle physics. A huge body of experimental evidence for QCD has been gathered over the years. QCD enjoys two peculiar properties: Confinement, which means that the force between quarks does not diminish as they are separated. Because of this, when you do split the quark the energy is enough to create another quark thus creating another quark pair; they are forever bound into hadrons such as theproton and the neutron or the pion and kaon. Although analytically unproven, confinement is widely believed to be true because it explains the consistent failure of free quark searches, and it is easy to demonstrate in lattice QCD. Asymptotic freedom, which means that in very high-energy reactions, quarks and gluons interact very weakly creating a quark–gluon plasma. This prediction of QCD was first discovered in the early 1970s by David Politzer and by Frank Wilczek and David Gross. For this work they were awarded the 2004 Nobel Prize in Physics. There is no known phase-transition line separating these two properties; confinement is dominant in low-energy scales but, as energy increases, asymptotic freedom becomes dominant.
    [Show full text]
  • Generalised Velocity-Dependent One-Scale Model for Current-Carrying Strings
    Generalised velocity-dependent one-scale model for current-carrying strings C. J. A. P. Martins,1, 2, ∗ Patrick Peter,3, 4, y I. Yu. Rybak,1, 2, z and E. P. S. Shellard4, x 1Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal 2Instituto de Astrofísica e Ciências do Espaço, CAUP, Rua das Estrelas, 4150-762 Porto, Portugal 3 GR"CO – Institut d’Astrophysique de Paris, CNRS & Sorbonne Université, UMR 7095 98 bis boulevard Arago, 75014 Paris, France 4Centre for Theoretical Cosmology, Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, United Kingdom (Dated: November 20, 2020) We develop an analytic model to quantitatively describe the evolution of superconducting cosmic string networks. Specifically, we extend the velocity-dependent one-scale (VOS) model to incorpo- rate arbitrary currents and charges on cosmic string worldsheets under two main assumptions, the validity of which we also discuss. We derive equations that describe the string network evolution in terms of four macroscopic parameters: the mean string separation (or alternatively the string correlation length) and the root mean square (RMS) velocity which are the cornerstones of the VOS model, together with parameters describing the averaged timelike and spacelike current contribu- tions. We show that our extended description reproduces the particular cases of wiggly and chiral cosmic strings, previously studied in the literature. This VOS model enables investigation of the evolution and possible observational signatures of superconducting cosmic string networks for more general equations of state, and these opportunities will be exploited in a companion paper.
    [Show full text]
  • 6 STANDARD MODEL: One-Loop Structure
    6 STANDARD MODEL: One-Loop Structure Although the fundamental laws of Nature obey quantum mechanics, mi- croscopically challenged physicists build and use quantum field theories by starting from a classical Lagrangian. The classical approximation, which de- scribes macroscopic objects from physics professors to dinosaurs, has in itself a physical reality, but since it emerges only at later times of cosmological evolution, it is not fundamental. We should therefore not be too surprised if unforeseen special problems and opportunities emerge in the analysis of quantum perturbations away from the classical Lagrangian. The classical Lagrangian is used as input to the path integral, whose eval- uation produces another Lagrangian, the effective Lagrangian, Leff , which encodes all the consequences of the quantum field theory. It contains an infinite series of polynomials in the fields associated with its degrees of free- dom, and their derivatives. The classical Lagrangian is reproduced by this expansion in the lowest power of ~ and of momentum. With the notable exceptions of scale invariance, and of some (anomalous) chiral symmetries, we think that the symmetries of the classical Lagrangian survive the quanti- zation process. Consequently, not all possible polynomials in the fields and their derivatives appear in Leff , only those which respect the symmetries. The terms which are of higher order in ~ yield the quantum corrections to the theory. They are calculated according to a specific, but perilous path, which uses the classical Lagrangian as input. This procedure gener- ates infinities, due to quantum effects at short distances. Fortunately, most fundamental interactions are described by theories where these infinities can be absorbed in a redefinition of the input parameters and fields, i.e.
    [Show full text]
  • On the Massless Tree-Level S-Matrix in 2D Sigma Models
    Imperial-TP-AT-2018-05 On the massless tree-level S-matrix in 2d sigma models Ben Hoarea;1, Nat Levineb;2 and Arkady A. Tseytlinb;3 aETH Institut für Theoretische Physik, ETH Zürich, Wolfgang-Pauli-Strasse 27, 8093 Zürich, Switzerland. bBlackett Laboratory, Imperial College, London SW7 2AZ, U.K. Abstract Motivated by the search for new integrable string models, we study the properties of massless tree-level S-matrices for 2d σ-models expanded near the trivial vacuum. We find that, in contrast to the standard massive case, there is no apparent link between massless S-matrices and integrability: in well-known integrable models the tree-level massless S-matrix fails to factorize and exhibits particle production. Such tree-level particle production is found in several classically integrable models: the principal chiral model, its classically equivalent “pseudo-dual” model, its non-abelian dual model and also the SO(N +1)=SO(N) coset model. The connection to integrability may, in principle, be restored if one expands near a non- trivial vacuum with massive excitations. We discuss IR ambiguities in 2d massless tree-level amplitudes and their resolution using either a small mass parameter or the i-regularization. In general, these ambiguities can lead to anomalies in the equivalence of the S-matrix under field redefinitions, and may be linked to the observed particle production in integrable models. We also comment on the transformation of massless S-matrices under σ-model T-duality, comparing the standard and the “doubled” formulations (with T-duality covariance built into the latter). arXiv:1812.02549v4 [hep-th] 15 May 2019 [email protected] [email protected] 3Also at Lebedev Institute and ITMP, Moscow State University.
    [Show full text]
  • Chiral Soliton Models and Nucleon Structure Functions
    S S symmetry Review Chiral Soliton Models and Nucleon Structure Functions Herbert Weigel 1,* and Ishmael Takyi 2 1 Institute of Theoretical Physics, Physics Department, Stellenbosch University, Matieland 7602, South Africa 2 Department of Mathematics, Kwame Nkrumah University of Science and Technology, Private Mail Bag, Kumasi, Ghana; [email protected] * Correspondence: [email protected] Abstract: We outline and review the computations of polarized and unpolarized nucleon structure functions within the bosonized Nambu-Jona-Lasinio chiral soliton model. We focus on a consistent regularization prescription for the Dirac sea contribution and present numerical results from that formulation. We also reflect on previous calculations on quark distributions in chiral quark soliton models and attempt to put them into perspective. Keywords: chiral quark model; regularization; chiral soliton; hadron tensor; structure functions 1. Introduction In this mini-review we reflect on nucleon structure function calculations in chiral soliton models. This is an interesting topic not only because structure functions are of high empirical relevance but maybe even more so conceptually as of how much information about the nucleon structure can be retrieved from soliton models. In this spirit, this paper to quite an extent is a proof of concept review. Solitons emerge in most nonlinear field theories as classical solutions to the field equations. These solutions have localized energy densities and can be attributed particle like properties. In the context of strong interactions, that govern the structure of hadrons, solitons of meson field configurations are considered as baryons [1]. Nucleon structure functions play an important role in deep inelastic scattering (DIS) Citation: Weigel, H.; Takyi, I.
    [Show full text]
  • The Φ - Meson Physics in the Chiral Model
    The φ - Meson Physics in the Chiral Model K.R. Nasriddinov, N.Z. Rajabov and N.E. Iskandarov Tashkent State Pedagogical University named after Nizami, Yusuf Khos Khojib str.-103, 700100, Tashkent, Uzbekistan + − 0 0 0 0 The φ → K K , K L K S , K K decays are studied using the method of phenomenological chiral Lagrangians. Calculated values for partial widths for these decay channels are compared with available experimental data. At present investigations of the φ(1020) - meson decays in experiments [1] and in the framework of theoretical models [2] are intensively carried out. It should be noted, that such decay channels of the φ - meson are not considered in chiral models and there are a few attempts [3] to calculate only some radiative decay channels of this meson. Studies of decay channels of this meson in chiral models are of interest because of the following reasons: First, the φ - meson mass is comparable to the chiral symmetry breaking scale of 1 GeV, the proposed decays into a rather heavy meson (the ρ or ω of about 800 MeV) and a light meson (the π or K ) might be manageable along the lines of heavy- mass chiral perturbation theory (similarly to the heavy-baryon chiral perturbation theory of the pion-nucleon sector); Second, this meson (also another particles) are produced in colliders, for example, at the cooler synchrotron ring (COSY) at the Institut fuer Kernphysic at the Forschungzentrum Juelich in proton-proton collisions. And in this case the environment has a temperature not equal zero. Therefore, we need to take into account the influence of temperature factors of the environment to the decay probabilities.
    [Show full text]
  • Lectures on Algebraic Quantum Field Theory and Operator Algebras
    ISSN 0029-3865- meiiiiffiiB BR01G1424 CBPF - CENTRO BRASILE1RO DE PESQUISAS FISICAS Rio de Janeiro Notas de Ffsica CBPF-NF-019/01 April 2001 Lectures on Algebraic Quantum Field Theory and Operator Algebras Bert Schroer MCT - Ministerio da Ciencia © Tecnologia BRASIL Lectures on Algebraic Quantum Field Theory and Operator Algebras BERT SCHROER INSTITUT FUR THEORETISCHE PHYSIK FU-BERLIN, ARNIMALLEE 14, 14195 BERLIN, GERMANY PRESENTLY: CBPF, RUA DR. XAVIER SIGAUD, 22290-180 Rio DE JANEIRO, BRAZIL EMAIL [email protected] based on lectures presented at the 2001 Summer School in Florianopolis and at the IMPA in Rio de Janeiro, April 2001 ABSTRACT. In this series of lectures directed towards a mainly mathematically oriented audience I try to motivate the use of operator algebra methods in quantum field theory. Therefore a title as "why mathematicians are/should be interested in algebraic quantum field theory" would be equally fitting. Besides a presentation of the framework and the main results of local quantum physics these notes may serve as a guide to frontier research problems in mathematical physics with applications in particle and condensed matter physics for whose solution operator algebraic methods seem indispensable. The ultraviolet problems of the standard approach and the recent holographic aspects belong to this kind of problems. CONTENTS 1 Quantum Theoretical and Mathematical Background 1 2 Superselections and Locality in Quantum Physics 21 3 Conformally invariant Local Quantum Physics 45 4 Constructive use of Modular Theory 57 CBPF-NF-019/01 1 1. QUANTUM THEORETICAL AND MATHEMATICAL BACKGROUND The fact that quantum field theory came into being almost at the same time as quantum mechanics often lead people to believe that it is "just a relativistic version of quantum mechanics".
    [Show full text]
  • Modified Instanton Sum in QCD and Higher-Groups
    Prepared for submission to JHEP Modified instanton sum in QCD and higher-groups Yuya Tanizaki, Mithat Ünsal North Carlina State University, Raleigh, NC, 27607, USA E-mail: [email protected], [email protected] Abstract: We consider the SU(N) Yang-Mills theory, whose topological sectors are restricted to the instanton number with integer multiples of p. We can formulate such a quantum field theory maintaining locality and unitarity, and the model contains both 2π- periodic scalar and 3-form gauge fields. This can be interpreted as coupling a topological theory to Yang-Mills theory, so the local dynamics becomes identical with that of pure Yang- Mills theory. The theory has not only ZN 1-form symmetry but also Zp 3-form symmetry, and we study the global nature of this theory from the recent ’t Hooft anomaly matching. The computation of ’t Hooft anomaly incorporates an intriguing higher-group structure. We also carefully examine that how such kinematical constraint is realized in the dynamics 3 1 by using the large-N and also the reliable semiclassics on R S , and we find that the × topological susceptibility plays a role of the order parameter for the Zp 3-form symmetry. Introducing a fermion in the fundamental or adjoint representation, we find that the chiral symmetry becomes larger than the usual case by Zp, and it leads to the extra p vacua by discrete chiral symmetry breaking. No dynamical domain wall can interpolate those extra vacua since such objects must be charged under the 3-form symmetry in order to match the ’t Hooft anomaly.
    [Show full text]
  • Arxiv:2011.07973V2 [Hep-Th]
    November, 2020 Higher Derivative Supersymmetric Nonlinear Sigma Models on Hermitian Symmetric Spaces, and BPS States Therein a b Muneto Nitta† and Shin Sasaki‡ † Department of Physics, and Research and Education Center for Natural Sciences, Keio University, Hiyoshi 4-1-1, Yokohama, Kanagawa 223-8521, Japan ‡ Department of Physics, Kitasato University Sagamihara 252-0373, Japan Abstract We formulate four-dimensional = 1 supersymmetric nonlinear sigma models on N Hermitian symmetric spaces with higher derivative terms, free from the auxiliary field problem and the Ostrogradski’s ghosts, as gauged linear sigma models. We then study Bogomol’nyi-Prasad-Sommerfield equations preserving 1/2 or 1/4 supersymmetries. We find that there are distinct branches, that we call canonical (F = 0) and non-canonical (F = 0) branches, associated with solutions to auxiliary fields F in chiral multiplets. 6 For the CP N model, we obtain a supersymmetric CP N Skyrme-Faddeev model in the canonical branch while in the non-canonical branch the Lagrangian consists of solely the C N arXiv:2011.07973v2 [hep-th] 5 Jan 2021 P Skyrme-Faddeev term without a canonical kinetic term. These structures can be extended to the Grassmann manifold GM,N = SU(M)/[SU(M N) SU(N) U(1)]. For − × × other Hermitian symmetric spaces such as the quadric surface QN−2 = SO(N)/[SO(N − 2) U(1)]), we impose F-term (holomorphic) constraints for embedding them into CP N−1 × or Grassmann manifold. We find that these constraints are consistent in the canonical branch but yield additional constraints on the dynamical fields thus reducing the target spaces in the non-canonical branch.
    [Show full text]
  • Quantum Field Theory
    V. Parameswaran Nair Quantum Field Theory A Modern Perspective November 10, 2004 Springer Berlin Heidelberg NewYork Hong Kong London Milan Paris Tokyo To the memory of my parents Velayudhan and Gowrikutty Nair Preface Quantum field theory, which started with Dirac’s work shortly after the dis- covery of quantum mechanics, has produced an impressive and important array of results. Quantum electrodynamics, with its extremely accurate and well-tested predictions, and the standard model of electroweak and chromo- dynamic (nuclear) forces are examples of successful theories. Field theory has also been applied to a variety of phenomena in condensed matter physics, in- cluding superconductivity, superfluidity and the quantum Hall effect. The concept of the renormalization group has given us a new perspective on field theory in general and on critical phenomena in particular. At this stage, a strong case can be made that quantum field theory is the mathematical and intellectual framework for describing and understanding all physical phenom- ena, except possibly for quantum gravity. This also means that quantum field theory has by now evolved into such a vast subject, with many subtopics and many ramifications, that it is im- possible for any book to capture much of it within a reasonable length. While there is a common core set of topics, every book on field theory is ultimately illustrating facets of the subject which the author finds interesting and fas- cinating. This book is no exception; it presents my view of certain topics in field theory loosely knit together and it grew out of courses on field theory and particle physics which I have taught at Columbia University and the City College of the CUNY.
    [Show full text]