Chiral Magnetism: a Geometric Perspective
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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. -
Skyrmions in Composite Higgs Models in QCD
The skyrmion Skyrmions in Composite Higgs Models in QCD Topology of composite Higgs models Marc Gillioz An example: the littlest Higgs model Relic density August 29, 2011 based on arXiv:1012.5288 and arXiv:1103.5990, in collaboration with Andreas von Manteuffel, Pedro Schwaller and Daniel Wyler 1/18 Marc Gillioz, Zurich PhD seminar 2011 Introduction SM ATLAS Preliminary CLs Limits σ / SM CMS Preliminary, s = 7 TeV The skyrmion σ Observed Observed σ -1 / Combined, L = 1.1-1.7 fb Expected ± 1σ int in QCD Expected σ ∫ Ldt = 1.0-2.3 fb-1 10 Expected ± 2σ 10 ± 1 σ LEP excluded Topology of ± 2 σ s = 7 TeV Tevatron excluded composite Higgs models 95% CL Limit on on Limit CL 95% 1 1 An example: limit on 95% CL the littlest Higgs model -1 Relic density 10 200 300 400 500 600 100 200 300 400 500 600 mH [GeV] Higgs boson mass (GeV/c2) Atlas collaboration (Lepton-Photon 2011) CMS collaboration (Lepton-Photon 2011) LHC data (and indirect evidence from previous experiments) points towards a light Higgs in the mass range 100–150 GeV. 2/18 Marc Gillioz, Zurich PhD seminar 2011 Introduction Any new physics above this scale contributes to The skyrmion in QCD the Higgs mass through radiative corrections. Topology of composite Higgs models need for a symmetry to protect it: An example: ⇒ the littlest Higgs model 1 SUSY: requires the introduction of a superpartner for each Relic density SM field. 2 Composite Higgs: the Higgs is a bound state of fermions from some strongly interacting sector, and it is light since it arises as a pseudo-Goldstone boson technicolor, little Higgs, holographic models, .. -
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. -
A Simple Mass-Splitting Mechanism in the Skyrme Model
A simple mass-splitting mechanism in the Skyrme model J.M. Speight∗ School of Mathematics, University of Leeds Leeds LS2 9JT, England April 2, 2018 Abstract It is shown that the addition of a single chiral symmetry breaking term to the standard !-meson variant of the nuclear Skyrme model can reproduce the proton-neutron mass difference. 1 Introduction The Skyrme model [9] is a nonlinear sigma model whose perturbative quanta are interpreted as pions and whose topological solitons are interpreted as nucleons. At the classical level, there is no difference between protons and neutrons in this model; the distinction only emerges after quantization of the internal rotational degrees of freedom enjoyed by the static soliton, and is determined, roughly speaking, by the sense (clockwise or anticlockwise) of internal rotation. It is clear, therefore, that in order to account for the slight mass difference between the neutron and the proton (mn = 939:56563 MeV, mp = 938:27231 MeV), the model's action must contain a small term which breaks time reversal symmetry, so that \clockwise" and \anticlockwise" internal rotation are dynamically inequivalent. Devising such a term, while maintaining Lorentz and parity invariance, does not seem to be possible in any version of the model containing only pion fields. It should be noted that adding electromagnetic effects to arXiv:1803.11216v1 [hep-th] 29 Mar 2018 the usual Skyrme model has precisely the opposite effect to the one desired: unsurprisingly, Coulomb repulsion renders the proton heavier than the neutron [3]. As has been long known, the proton-neutron mass splitting can be accommodated if one extends the model to include coupled vector mesons [5]. -
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. -
Recent Progress on Dense Nuclear Matter in Skyrmion Approaches Yong-Liang Ma, Mannque Rho
Recent progress on dense nuclear matter in skyrmion approaches Yong-Liang Ma, Mannque Rho To cite this version: Yong-Liang Ma, Mannque Rho. Recent progress on dense nuclear matter in skyrmion approaches. SCIENCE CHINA Physics, Mechanics & Astronomy, 2017, 60, pp.032001. 10.1007/s11433-016-0497- 2. cea-01491871 HAL Id: cea-01491871 https://hal-cea.archives-ouvertes.fr/cea-01491871 Submitted on 17 Mar 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. SCIENCE CHINA Physics, Mechanics & Astronomy . Invited Review . Month 2016 Vol. *** No. ***: ****** doi: ******** Recent progress on dense nuclear matter in skyrmion approaches Yong-Liang Ma1 & Mannque Rho2 1Center of Theoretical Physics and College of Physics, Jilin University, Changchun, 130012, China; Email:[email protected] 2Institut de Physique Th´eorique, CEA Saclay, 91191 Gif-sur-Yvette c´edex, France; Email:[email protected] The Skyrme model provides a novel unified approach to nuclear physics. In this approach, single baryon, baryonic matter and medium-modified hadron properties are treated on the same footing. Intrinsic density dependence (IDD) reflecting the change of vacuum by compressed baryonic matter figures naturally in the approach. In this article, we review the recent progress on accessing dense nuclear matter by putting baryons treated as solitons, namely, skyrmions, on crystal lattice with accents on the implications in compact stars. -
Skyrmion Flow Near Room Temperature in an Ultralow Current Density
ARTICLE Received 16 Apr 2012 | Accepted 5 Jul 2012 | Published 7 Aug 2012 DOI: 10.1038/ncomms1990 Skyrmion flow near room temperature in an ultralow current density X.Z. Yu1, N. Kanazawa2, W.Z. Zhang3, T. Nagai3, T. Hara3, K. Kimoto3, Y. Matsui3, Y. Onose2,4 & Y. Tokura1,2,4 The manipulation of spin textures with electric currents is an important challenge in the field of spintronics. Many attempts have been made to electrically drive magnetic domain walls in ferromagnets, yet the necessary current density remains quite high (~107 A cm − 2). A recent neutron study combining Hall effect measurements has shown that an ultralow current density of J~102 A cm − 2 can trigger the rotational and translational motion of the skyrmion lattice in MnSi, a helimagnet, within a narrow temperature range. Raising the temperature range in which skyrmions are stable and reducing the current required to drive them are therefore desirable objectives. Here we demonstrate near-room-temperature motion of skyrmions driven by electrical currents in a microdevice composed of the helimagnet FeGe, by using in-situ Lorentz transmission electron microscopy. The rotational and translational motions of skyrmion crystal begin under critical current densities far below 100 A cm − 2. 1 Correlated Electron Research Group (CERG) and Cross-Correlated Materials Research Group (CMRG), RIKEN-ASI, Wako 351-0198, Japan. 2 Department of Applied Physics and Quantum-Phase Electronics Center (QPEC), University of Tokyo, Tokyo 113-8656, Japan. 3 National Institute for Materials Science, Tsukuba 305-0044, Japan. 4 Multiferroics Project, Exploratory Research for Advanced Technology (ERATO), Japan Science and Technology Agency, Tokyo 113-8656, Japan. -
Mesons, Baryons and Waves in the Baby Skyrmion Model 1. Introduction
DTP-96/17 November 28, 1996 Mesons, Baryons and Waves in the Baby Skyrmion Mo del 1 A. Kudryavtsev B. Piette, and W.J. Zakrzewski Department of Mathematical Sciences University of Durham, Durham DH1 3LE, England 1 also at ITEP, Moscow, Russia E-Mail: [email protected] [email protected] [email protected] ABSTRACT We study various classical solutions of the baby-Skyrmion mo del in (2 + 1) dimen- sions. We p oint out the existence of higher energy states interpret them as resonances of Skyrmions and anti-Skyrmions and study their decays. Most of the discussion in- volves a highly exited Skyrmion-like state with winding numb er one which decays into an ordinary Skyrmion and a Skyrmion-anti-Skyrmion pair. We also study wave-like solutions of the mo del and show that some of such solutions can b e constructed from the solutions of the sine-Gordon equation. We also show that the baby-Skyrmion has non-top ological stationary solutions. We study their interactions with Skyrmions. 1. Intro duction. In previous pap ers bytwo of us (BP and WJZ) [1-3] some hedgehog-like solutions of the so called baby-Skyrmion mo del were studied. It was shown there that the mo del has soliton-like top ologically stable static solutions (called baby-Skyrmions) and that these solitons can form b ound states. The interaction b etween the solitons was studied in detail and it was shown that the long distance force between 2 baby-Skyrmions dep ends on their relative orientation. -
Skyrmion Deformation in Finite Nuclei
Section I. Particles and Nuclei optimization of the basis) results in more high precision at essentially less dimensions of the basis in comparison with the known calculations [1] in traditional approach In addition to the energies and r.m.s radii, the density distributions, formfactors, pair correlation functions and momentum distributions are analyzed for three and four nucleons with a number of commonly used interaction potentials (Minnesota, Afnan-Tang. F.ikemeier-Haekenbroich etc.) as well as with our version of potential K2 [2] with small repulsion at short distances. Comparison of the results is carried out, and the convergence with the basis dimension increase is analyzed in the cases of spinless approximation [2,3] for the nuclear interaction potential, isospin representation with spin-dependent potentials, and the approach without use of the isospin quantum number. We find the hierarchy of configurations for symmetric and asymmetric (with respect to permutation o\" identical particles) wave function components with the increase of the basis dimension, and it is shown for the optimal choice of the basis functions that each of the involved asymmetric Gaussian component needs a few (about 3) symmetric ones to be involved into consideration because of their dominant role Due to the essential deer ase of the number of equations in comparison with that in traditional approaches, precise study of nuclei containing up to six nucleons with central exchange NN-potentials becoues possible. The minimum number of equations in our approach as well as the optimization schemes for constructing the optimal basis gives a possibility to present the results of precise calculations in the form of a short list of parameters of the explicit wave function (in Gaussian representation) which can be directly used by other researches for studying the processes with the nuclei *H, 'He and ''He involved References 1. -
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. -
A New Large Nc Relation As a Probe of Skyrmions and Their Holographic
Tests of Universality of Baryon Form Factors In Holographic QCD A. Cherman, T.D. Cohen, M. Nielsen, PRL103(09) Univ. of Maryland and Univ. of Sao Paulo Low x Meeting, September 2009 QCD: strong-coupled theory AdS/QCD models: successful at reproducing low energy hadronic observables • two classes of AdS/QCD models Top-down models: Botton-up models: arise from sting theory QCD large Nc dual to a classical 5D theory D4/D8 system gauge theory confining as QCD field content 5D matched AdS/CFT requires large Nc to low energy chiral and ´t Hooft coupling symmetry of QCD Both cases: large Nc is required QCD is a weakly-interacting theory of long -lived mesons in the • ‘t Hooft, 1973 large Nc limit. • In the large Nc limit, baryons are ‘soliton -like’ configurations of meson fields. Witten, 1979 1 • Baryon masses scale as Nc (composed of Nc quarks), 1/2 interactions with mesons scale as Nc . • Unlike mesons, baryons are not narrow at large Nc. • Nucleons, deltas, become degenerate. Mass splitting -1 scales as Nc . • In contrast to the pure meson sector, meson loops make leading order contributions to baryon properties at large Nc. • Variety of baryon models (Skyrme models) use large Nc properties of baryons for inspiration. Skyrme, 1961 • Baryons modeled as quantum states of slowly rotating Adkins, Nappi, hedgehog Skyrmions of meson fields. Witten, 1983 Dashen, Manohar, Jenkins,1993-95 Model-independent relations for baryons valid at large Nc • Goldberger-Treiman relation: • Relation is model-indepedent, and follows from chiral symmetry. • Nucleon and delta couplings with pions are related by • • This relation follows just from the large Nc limit • New model-independent relation: • Ratio of nucleon form factors in position space, evaluated at large distances: • Relation depends on both the large Nc and chiral limits. -
Nucleon-Antinucleon Interaction from the Skyrme Model: II
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server Nucleon-Antinucleon Interaction from the Skyrme Model: II Yang Lu, Pavlos Protopapas and R. D. Amado Department of Physics and Astronomy University of Pennsylvania, Philadelphia, Pennsylvania 19104 September 13, 1997 Abstract We calculate the full static interaction of a Skyrmion and an anti-Skyrmion as a function of separation and relative grooming. From this, using projection methods and Born-Oppenheimer mixing, we obtain the nucleon antinucleon interaction. We find agreement with the major features of the empirical interaction including the strong central attraction and the sharp onset of annihilation at about 1 fm. 1 Introduction Making a theory of low energy nucleon-antinucleon annihilation from the entrance channel through to the annihilation products presents a daunting challenge. An exact QCD based calculation of the process is beyond our present analytical understanding and our computational resources. We are left then with either abandoning the problem or using some approximate or effective theory. Such a theory must include an account of the nature of the nucleon and the antinucleon, in order to describe annihilation, as well as containing a description of their interaction. The theory should also have its roots in QCD. The only such effective theory of annihilation that contains the requisite ingredients and gives hope of being tractable is based on the Skyrme model [1]. This models QCD in the classical or large number of colors (NC ) limit and at long distances or low momentum [2, 3]. Sommermann et al.