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The Role of Strangeness in Ultrarelativistic Nuclear
HUTFT THE ROLE OF STRANGENESS IN a ULTRARELATIVISTIC NUCLEAR COLLISIONS Josef Sollfrank Research Institute for Theoretical Physics PO Box FIN University of Helsinki Finland and Ulrich Heinz Institut f ur Theoretische Physik Universitat Regensburg D Regensburg Germany ABSTRACT We review the progress in understanding the strange particle yields in nuclear colli sions and their role in signalling quarkgluon plasma formation We rep ort on new insights into the formation mechanisms of strange particles during ultrarelativistic heavyion collisions and discuss interesting new details of the strangeness phase di agram In the main part of the review we show how the measured multistrange particle abundances can b e used as a testing ground for chemical equilibration in nuclear collisions and how the results of such an analysis lead to imp ortant con straints on the collision dynamics and spacetime evolution of high energy heavyion reactions a To b e published in QuarkGluon Plasma RC Hwa Eds World Scientic Contents Introduction Strangeness Pro duction Mechanisms QuarkGluon Pro duction Mechanisms Hadronic Pro duction Mechanisms Thermal Mo dels Thermal Parameters Relative and Absolute Chemical Equilibrium The Partition Function The Phase Diagram of Strange Matter The Strange Matter Iglo o Isentropic Expansion Trajectories The T ! Limit of the Phase Diagram -
The Five Common Particles
The Five Common Particles The world around you consists of only three particles: protons, neutrons, and electrons. Protons and neutrons form the nuclei of atoms, and electrons glue everything together and create chemicals and materials. Along with the photon and the neutrino, these particles are essentially the only ones that exist in our solar system, because all the other subatomic particles have half-lives of typically 10-9 second or less, and vanish almost the instant they are created by nuclear reactions in the Sun, etc. Particles interact via the four fundamental forces of nature. Some basic properties of these forces are summarized below. (Other aspects of the fundamental forces are also discussed in the Summary of Particle Physics document on this web site.) Force Range Common Particles It Affects Conserved Quantity gravity infinite neutron, proton, electron, neutrino, photon mass-energy electromagnetic infinite proton, electron, photon charge -14 strong nuclear force ≈ 10 m neutron, proton baryon number -15 weak nuclear force ≈ 10 m neutron, proton, electron, neutrino lepton number Every particle in nature has specific values of all four of the conserved quantities associated with each force. The values for the five common particles are: Particle Rest Mass1 Charge2 Baryon # Lepton # proton 938.3 MeV/c2 +1 e +1 0 neutron 939.6 MeV/c2 0 +1 0 electron 0.511 MeV/c2 -1 e 0 +1 neutrino ≈ 1 eV/c2 0 0 +1 photon 0 eV/c2 0 0 0 1) MeV = mega-electron-volt = 106 eV. It is customary in particle physics to measure the mass of a particle in terms of how much energy it would represent if it were converted via E = mc2. -
Penguin Decays of B Mesons
COLO–HEP–395 SLAC-PUB-7796 HEPSY 98-1 April 23, 1998 PENGUIN DECAYS OF B MESONS Karen Lingel 1 Stanford Linear Accelerator Center Stanford University, Stanford, CA 94309 and Tomasz Skwarnicki 2 Department of Physics, Syracuse University Syracuse, NY 13244 and James G. Smith 3 Department of Physics, University of Colorado arXiv:hep-ex/9804015v1 27 Apr 1998 Boulder, CO 80309 Submitted to Annual Reviews of Nuclear and Particle Science 1Work supported by Department of Energy contract DE-AC03-76SF00515 2Work supported by National Science Foundation contract PHY 9807034 3Work supported by Department of Energy contract DE-FG03-95ER40894 2 LINGEL & SKWARNICKI & SMITH PENGUIN DECAYS OF B MESONS Karen Lingel Stanford Linear Accelerator Center Tomasz Skwarnicki Department of Physics, Syracuse University James G. Smith Department of Physics, University of Colorado KEYWORDS: loop CP-violation charmless ABSTRACT: Penguin, or loop, decays of B mesons induce effective flavor-changing neutral currents, which are forbidden at tree level in the Standard Model. These decays give special insight into the CKM matrix and are sensitive to non-standard model effects. In this review, we give a historical and theoretical introduction to penguins and a description of the various types of penguin processes: electromagnetic, electroweak, and gluonic. We review the experimental searches for penguin decays, including the measurements of the electromagnetic penguins b → sγ ∗ ′ and B → K γ and gluonic penguins B → Kπ, B+ → ωK+ and B → η K, and their implications for the Standard Model and New Physics. We conclude by exploring the future prospects for penguin physics. CONTENTS INTRODUCTION .................................... 3 History of Penguins .................................... -
Quantum Field Theory*
Quantum Field Theory y Frank Wilczek Institute for Advanced Study, School of Natural Science, Olden Lane, Princeton, NJ 08540 I discuss the general principles underlying quantum eld theory, and attempt to identify its most profound consequences. The deep est of these consequences result from the in nite number of degrees of freedom invoked to implement lo cality.Imention a few of its most striking successes, b oth achieved and prosp ective. Possible limitation s of quantum eld theory are viewed in the light of its history. I. SURVEY Quantum eld theory is the framework in which the regnant theories of the electroweak and strong interactions, which together form the Standard Mo del, are formulated. Quantum electro dynamics (QED), b esides providing a com- plete foundation for atomic physics and chemistry, has supp orted calculations of physical quantities with unparalleled precision. The exp erimentally measured value of the magnetic dip ole moment of the muon, 11 (g 2) = 233 184 600 (1680) 10 ; (1) exp: for example, should b e compared with the theoretical prediction 11 (g 2) = 233 183 478 (308) 10 : (2) theor: In quantum chromo dynamics (QCD) we cannot, for the forseeable future, aspire to to comparable accuracy.Yet QCD provides di erent, and at least equally impressive, evidence for the validity of the basic principles of quantum eld theory. Indeed, b ecause in QCD the interactions are stronger, QCD manifests a wider variety of phenomena characteristic of quantum eld theory. These include esp ecially running of the e ective coupling with distance or energy scale and the phenomenon of con nement. -
A Slice of Ads 5 As the Large N Limit of Seiberg Duality
IPPP/10/86 ; DCPT/10/172 CERN-PH-TH/2010-234 A slice of AdS5 as the large N limit of Seiberg duality Steven Abela,b,1 and Tony Gherghettac,2 aInstitute for Particle Physics Phenomenology Durham University, DH1 3LE, UK bTheory Division, CERN, CH-1211 Geneva 23, Switzerland cSchool of Physics, University of Melbourne Victoria 3010, Australia Abstract A slice of AdS5 is used to provide a 5D gravitational description of 4D strongly-coupled Seiberg dual gauge theories. An (electric) SU(N) gauge theory in the conformal window at large N is described by the 5D bulk, while its weakly coupled (magnetic) dual is confined to the IR brane. This framework can be used to construct an = 1 N MSSM on the IR brane, reminiscent of the original Randall-Sundrum model. In addition, we use our framework to study strongly-coupled scenarios of supersymmetry breaking mediated by gauge forces. This leads to a unified scenario that connects the arXiv:1010.5655v2 [hep-th] 28 Oct 2010 extra-ordinary gauge mediation limit to the gaugino mediation limit in warped space. [email protected] [email protected] 1 Introduction Seiberg duality [1, 2] is a powerful tool for studying strong dynamics, enabling calcu- lable approaches to otherwise intractable questions, as for example in the discovery of metastable minima in the free magnetic phase of supersymmetric quantum chromodynam- ics (SQCD) [3] (ISS). Despite such successes, the phenomenological applications of Seiberg duality are somewhat limited, simply by the relatively small number of known examples. An arguably more flexible tool for thinking about strong coupling is the gauge/gravity correspondence, namely the existence of gravitational duals for strongly-coupled gauge theories [4–6]. -
Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 12: Hadron Decays
Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 12: Hadron Decays !Resonances !Heavy Meson and Baryons !Decays and Quantum numbers !CKM matrix 1 Announcements •No lecture on Friday. •Remaining lectures: •Tuesday 13 March •Friday 16 March •Tuesday 20 March •Friday 23 March •Tuesday 27 March •Friday 30 March •Tuesday 3 April •Remaining Tutorials: •Monday 26 March •Monday 2 April 2 From Friday: Mesons and Baryons Summary • Quarks are confined to colourless bound states, collectively known as hadrons: " mesons: quark and anti-quark. Bosons (s=0, 1) with a symmetric colour wavefunction. " baryons: three quarks. Fermions (s=1/2, 3/2) with antisymmetric colour wavefunction. " anti-baryons: three anti-quarks. • Lightest mesons & baryons described by isospin (I, I3), strangeness (S) and hypercharge Y " isospin I=! for u and d quarks; (isospin combined as for spin) " I3=+! (isospin up) for up quarks; I3="! (isospin down) for down quarks " S=+1 for strange quarks (additive quantum number) " hypercharge Y = S + B • Hadrons display SU(3) flavour symmetry between u d and s quarks. Used to predict the allowed meson and baryon states. • As baryons are fermions, the overall wavefunction must be anti-symmetric. The wavefunction is product of colour, flavour, spin and spatial parts: ! = "c "f "S "L an odd number of these must be anti-symmetric. • consequences: no uuu, ddd or sss baryons with total spin J=# (S=#, L=0) • Residual strong force interactions between colourless hadrons propagated by mesons. 3 Resonances • Hadrons which decay due to the strong force have very short lifetime # ~ 10"24 s • Evidence for the existence of these states are resonances in the experimental data Γ2/4 σ = σ • Shape is Breit-Wigner distribution: max (E M)2 + Γ2/4 14 41. -
Thermal Evolution of the Axial Anomaly
Thermal evolution of the axial anomaly Gergely Fej}os Research Center for Nuclear Physics Osaka University The 10th APCTP-BLTP/JINR-RCNP-RIKEN Joint Workshop on Nuclear and Hadronic Physics 18th August, 2016 G. Fejos & A. Hosaka, arXiv: 1604.05982 Gergely Fej}os Thermal evolution of the axial anomaly Outline aaa Motivation Functional renormalization group Chiral (linear) sigma model and axial anomaly Extension with nucleons Summary Gergely Fej}os Thermal evolution of the axial anomaly Motivation Gergely Fej}os Thermal evolution of the axial anomaly Chiral symmetry is spontaneuously broken in the ground state: < ¯ > = < ¯R L > + < ¯L R > 6= 0 SSB pattern: SUL(Nf ) × SUR (Nf ) −! SUV (Nf ) Anomaly: UA(1) is broken by instantons Details of chiral symmetry restoration? Critical temperature? Axial anomaly? Is it recovered at the critical point? Motivation QCD Lagrangian with quarks and gluons: 1 L = − G a G µνa + ¯ (iγ Dµ − m) 4 µν i µ ij j Approximate chiral symmetry for Nf = 2; 3 flavors: iT aθa iT aθa L ! e L L; R ! e R R [vector: θL + θR , axialvector: θL − θR ] Gergely Fej}os Thermal evolution of the axial anomaly Details of chiral symmetry restoration? Critical temperature? Axial anomaly? Is it recovered at the critical point? Motivation QCD Lagrangian with quarks and gluons: 1 L = − G a G µνa + ¯ (iγ Dµ − m) 4 µν i µ ij j Approximate chiral symmetry for Nf = 2; 3 flavors: iT aθa iT aθa L ! e L L; R ! e R R [vector: θL + θR , axialvector: θL − θR ] Chiral symmetry is spontaneuously broken in the ground state: < ¯ > = < ¯R L > + < ¯L R -
7. Gamma and X-Ray Interactions in Matter
Photon interactions in matter Gamma- and X-Ray • Compton effect • Photoelectric effect Interactions in Matter • Pair production • Rayleigh (coherent) scattering Chapter 7 • Photonuclear interactions F.A. Attix, Introduction to Radiological Kinematics Physics and Radiation Dosimetry Interaction cross sections Energy-transfer cross sections Mass attenuation coefficients 1 2 Compton interaction A.H. Compton • Inelastic photon scattering by an electron • Arthur Holly Compton (September 10, 1892 – March 15, 1962) • Main assumption: the electron struck by the • Received Nobel prize in physics 1927 for incoming photon is unbound and stationary his discovery of the Compton effect – The largest contribution from binding is under • Was a key figure in the Manhattan Project, condition of high Z, low energy and creation of first nuclear reactor, which went critical in December 1942 – Under these conditions photoelectric effect is dominant Born and buried in • Consider two aspects: kinematics and cross Wooster, OH http://en.wikipedia.org/wiki/Arthur_Compton sections http://www.findagrave.com/cgi-bin/fg.cgi?page=gr&GRid=22551 3 4 Compton interaction: Kinematics Compton interaction: Kinematics • An earlier theory of -ray scattering by Thomson, based on observations only at low energies, predicted that the scattered photon should always have the same energy as the incident one, regardless of h or • The failure of the Thomson theory to describe high-energy photon scattering necessitated the • Inelastic collision • After the collision the electron departs -
Chirality-Assisted Lateral Momentum Transfer for Bidirectional
Shi et al. Light: Science & Applications (2020) 9:62 Official journal of the CIOMP 2047-7538 https://doi.org/10.1038/s41377-020-0293-0 www.nature.com/lsa ARTICLE Open Access Chirality-assisted lateral momentum transfer for bidirectional enantioselective separation Yuzhi Shi 1,2, Tongtong Zhu3,4,5, Tianhang Zhang3, Alfredo Mazzulla 6, Din Ping Tsai 7,WeiqiangDing 5, Ai Qun Liu 2, Gabriella Cipparrone6,8, Juan José Sáenz9 and Cheng-Wei Qiu 3 Abstract Lateral optical forces induced by linearly polarized laser beams have been predicted to deflect dipolar particles with opposite chiralities toward opposite transversal directions. These “chirality-dependent” forces can offer new possibilities for passive all-optical enantioselective sorting of chiral particles, which is essential to the nanoscience and drug industries. However, previous chiral sorting experiments focused on large particles with diameters in the geometrical-optics regime. Here, we demonstrate, for the first time, the robust sorting of Mie (size ~ wavelength) chiral particles with different handedness at an air–water interface using optical lateral forces induced by a single linearly polarized laser beam. The nontrivial physical interactions underlying these chirality-dependent forces distinctly differ from those predicted for dipolar or geometrical-optics particles. The lateral forces emerge from a complex interplay between the light polarization, lateral momentum enhancement, and out-of-plane light refraction at the particle-water interface. The sign of the lateral force could be reversed by changing the particle size, incident angle, and polarization of the obliquely incident light. 1234567890():,; 1234567890():,; 1234567890():,; 1234567890():,; Introduction interface15,16. The displacements of particles controlled by Enantiomer sorting has attracted tremendous attention thespinofthelightcanbeperpendiculartothedirectionof – owing to its significant applications in both material science the light beam17 19. -
Chiral Anomaly Without Relativity Arxiv:1511.03621V1 [Physics.Pop-Ph]
Chiral anomaly without relativity A.A. Burkov Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada, and ITMO University, Saint Petersburg 197101, Russia Perspective on J. Xiong et al., Science 350, 413 (2015). The Dirac equation, which describes relativistic fermions, has a mathematically inevitable, but puzzling feature: negative energy solutions. The physical reality of these solutions is unques- tionable, as one of their direct consequences, the existence of antimatter, is confirmed by ex- periment. It is their interpretation that has always been somewhat controversial. Dirac’s own idea was to view the vacuum as a state in which all the negative energy levels are physically filled by fermions, which is now known as the Dirac sea. This idea seems to directly contradict a common-sense view of the vacuum as a state in which matter is absent and is thus generally disliked among high-energy physicists, who prefer to regard the Dirac sea as not much more than a useful metaphor. On the other hand, the Dirac sea is a very natural concept from the point of view of a condensed matter physicist, since there is a direct and simple analogy: filled valence bands of an insulating crystal. There exists, however, a phenomenon within the con- arXiv:1511.03621v1 [physics.pop-ph] 26 Oct 2015 text of the relativistic quantum field theory itself, whose satisfactory understanding seems to be hard to achieve without assigning physical reality to the Dirac sea. This phenomenon is the chiral anomaly, a quantum-mechanical violation of chiral symmetry, which was first observed experimentally in the particle physics setting as a decay of a neutral pion into two photons. -
Chiral Symmetry and Quantum Hadro-Dynamics
Chiral symmetry and quantum hadro-dynamics G. Chanfray1, M. Ericson1;2, P.A.M. Guichon3 1IPNLyon, IN2P3-CNRS et UCB Lyon I, F69622 Villeurbanne Cedex 2Theory division, CERN, CH12111 Geneva 3SPhN/DAPNIA, CEA-Saclay, F91191 Gif sur Yvette Cedex Using the linear sigma model, we study the evolutions of the quark condensate and of the nucleon mass in the nuclear medium. Our formulation of the model allows the inclusion of both pion and scalar-isoscalar degrees of freedom. It guarantees that the low energy theorems and the constrains of chiral perturbation theory are respected. We show how this formalism incorporates quantum hadro-dynamics improved by the pion loops effects. PACS numbers: 24.85.+p 11.30.Rd 12.40.Yx 13.75.Cs 21.30.-x I. INTRODUCTION The influence of the nuclear medium on the spontaneous breaking of chiral symmetry remains an open problem. The amount of symmetry breaking is measured by the quark condensate, which is the expectation value of the quark operator qq. The vacuum value qq(0) satisfies the Gell-mann, Oakes and Renner relation: h i 2m qq(0) = m2 f 2, (1) q h i − π π where mq is the current quark mass, q the quark field, fπ =93MeV the pion decay constant and mπ its mass. In the nuclear medium the quark condensate decreases in magnitude. Indeed the total amount of restoration is governed by a known quantity, the nucleon sigma commutator ΣN which, for any hadron h is defined as: Σ = i h [Q , Q˙ ] h =2m d~x [ h qq(~x) h qq(0) ] , (2) h − h | 5 5 | i q h | | i−h i Z ˙ where Q5 is the axial charge and Q5 its time derivative. -
Full-Heavy Tetraquarks in Constituent Quark Models
Eur. Phys. J. C (2020) 80:1083 https://doi.org/10.1140/epjc/s10052-020-08650-z Regular Article - Theoretical Physics Full-heavy tetraquarks in constituent quark models Xin Jina, Yaoyao Xueb, Hongxia Huangc, Jialun Pingd Department of Physics and Jiangsu Key Laboratory for Numerical Simulation of Large Scale Complex Systems, Nanjing Normal University, Nanjing 210023, People’s Republic of China Received: 4 July 2020 / Accepted: 10 November 2020 / Published online: 23 November 2020 © The Author(s) 2020 Abstract The full-heavy tetraquarks bbb¯b¯ and ccc¯c¯ are [5]. Since then, more and more exotic states were observed systematically investigated within the chiral quark model and proposed, such as Y (4260), Zc(3900), X(5568), and so and the quark delocalization color screening model. Two on. The study of exotic states can help us to understand the structures, meson–meson and diquark–antidiquark, are con- hadron structures and the hadron–hadron interactions better. sidered. For the full-beauty bbb¯b¯ systems, there is no any The full-heavy tetraquark states (QQQ¯ Q¯ , Q = c, b) bound state or resonance state in two structures in the chiral attracted extensive attention for the last few years, since such quark model, while the wide resonances with masses around states with very large energy can be accessed experimentally 19.1 − 19.4 GeV and the quantum numbers J P = 0+,1+, and easily distinguished from other states. In the experiments, and 2+ are possible in the quark delocalization color screen- the CMS collaboration measured pair production of ϒ(1S) ing model. For the full-charm ccc¯c¯ systems, the results are [6].