Notes on Elementary Particle Physics
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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. -
Followed by a Stretcher That Fits Into the Same
as the booster; the main synchro what cheaper because some ex tunnel (this would require comple tron taking the beam to the final penditure on buildings and general mentary funding beyond the normal energy; followed by a stretcher infrastructure would be saved. CERN budget); and at the Swiss that fits into the same tunnel as In his concluding remarks, SIN Laboratory. Finally he pointed the main ring of circumference 960 F. Scheck of Mainz, chairman of out that it was really one large m (any resemblance to existing the EHF Study Group, pointed out community of future users, not presently empty tunnels is not that the physics case for EHF was three, who were pushing for a unintentional). Bradamante pointed well demonstrated, that there was 'kaon factory'. Whoever would be out that earlier criticisms are no a strong and competent European first to obtain approval, the others longer valid. The price seems un physics community pushing for it, would beat a path to his door. der control, the total investment and that there were good reasons National decisions on the project for a 'green pasture' version for building it in Europe. He also will be taken this year. amounting to about 870 million described three site options: a Deutschmarks. A version using 'green pasture' version in Italy; at By Florian Scheck existing facilities would be some- CERN using the now defunct ISR A ZEUS group meeting, with spokesman Gunter Wolf one step in front of the pack. (Photo DESY) The HERA electron-proton collider now being built at the German DESY Laboratory in Hamburg will be a unique physics tool. -
Qcd in Heavy Quark Production and Decay
QCD IN HEAVY QUARK PRODUCTION AND DECAY Jim Wiss* University of Illinois Urbana, IL 61801 ABSTRACT I discuss how QCD is used to understand the physics of heavy quark production and decay dynamics. My discussion of production dynam- ics primarily concentrates on charm photoproduction data which is compared to perturbative QCD calculations which incorporate frag- mentation effects. We begin our discussion of heavy quark decay by reviewing data on charm and beauty lifetimes. Present data on fully leptonic and semileptonic charm decay is then reviewed. Mea- surements of the hadronic weak current form factors are compared to the nonperturbative QCD-based predictions of Lattice Gauge The- ories. We next discuss polarization phenomena present in charmed baryon decay. Heavy Quark Effective Theory predicts that the daugh- ter baryon will recoil from the charmed parent with nearly 100% left- handed polarization, which is in excellent agreement with present data. We conclude by discussing nonleptonic charm decay which are tradi- tionally analyzed in a factorization framework applicable to two-body and quasi-two-body nonleptonic decays. This discussion emphasizes the important role of final state interactions in influencing both the observed decay width of various two-body final states as well as mod- ifying the interference between Interfering resonance channels which contribute to specific multibody decays. "Supported by DOE Contract DE-FG0201ER40677. © 1996 by Jim Wiss. -251- 1 Introduction the direction of fixed-target experiments. Perhaps they serve as a sort of swan song since the future of fixed-target charm experiments in the United States is A vast amount of important data on heavy quark production and decay exists for very short. -
Effects of Scalar Mesons in a Skyrme Model with Hidden Local Symmetry
Effects of scalar mesons in a Skyrme model with hidden local symmetry 1, 2, 1, Bing-Ran He, ∗ Yong-Liang Ma, † and Masayasu Harada ‡ 1Department of Physics, Nagoya University, Nagoya, 464-8602, Japan 2Center of Theoretical Physics and College of Physics, Jilin University, Changchun, 130012, China (Dated: March 5, 2018) We study the effects of light scalar mesons on the skyrmion properties by constructing and ex- amining a mesonic model including pion, rho meson, and omega meson fields as well as two-quark and four-quark scalar meson fields. In our model, the physical scalar mesons are defined as mixing states of the two- and four-quark fields. We first omit the four-quark scalar meson field from the model and find that when there is no direct coupling between the two-quark scalar meson and the vector mesons, the soliton mass is smaller and the soliton size is larger for lighter scalar mesons; when direct coupling is switched on, as the coupling strength increases, the soliton becomes heavy, and the radius of the baryon number density becomes large, as the repulsive force arising from the ω meson becomes strong. We then include the four-quark scalar meson field in the model and find that mixing between the two-quark and four-quark components of the scalar meson fields also affects the properties of the soliton. When the two-quark component of the lighter scalar meson is increased, the soliton mass decreases and the soliton size increases. PACS numbers: 11.30.Rd, 12.39.Dc, 12.39.Fe, 14.40.Be I. -
Electron-Nucleon Scattering at LDMX for DUNE
Snowmass Letter of Intent: Snowmass Topical Groups: NF6, RF6, TF11 Electron-Nucleon Scattering at LDMX for DUNE Torsten Akesson1, Artur Ankowski2, Nikita Blinov3, Lene Kristian Bryngemark4, Pierfrancesco Butti2, Caterina Doglioni1, Craig Dukes5, Valentina Dutta6, Bertrand Echenard7, Thomas Eichlersmith8, Ralf Ehrlich5, Andrew Furmanski∗8, Niramay Gogate9, Mathew Graham2, Craig Group5, Alexander Friedland2, David Hitlin7, Vinay Hegde9, Christian Herwig3, Joseph Incandela6, Wesley Ketchumy3, Gordan Krnjaic3, Amina Li6, Shirley Liz2,3, Dexu Lin7, Jeremiah Mans8, Cristina Mantilla Suarez3, Phillip Masterson6, Martin Meier8, Sophie Middleton7, Omar Moreno2, Geoffrey Mullier1, Tim Nelson2, James Oyang7, Gianluca Petrillo2, Ruth Pottgen1, Stefan Prestel1, Luis Sarmiento1, Philip Schuster2, Hirohisa Tanaka2, Lauren Tompkins4, Natalia Toro2, Nhan Tran§3, and Andrew Whitbeck9 1Lund University 2Stanford Linear Accelerator Laboratory 3Fermi National Accelerator Laboratory 4Stanford University 5University of Virginia 6University of California Santa Barbara 7California Institute of Technology 8University of Minnesota 9Texas Tech University ABSTRACT We point out that the LDMX (Light Dark Matter eXperiment) detector design, conceived to search for sub-GeV dark matter, will also have very advantageous characteristics to pursue electron-nucleus scattering measurements of direct relevance to the neutrino program at DUNE and elsewhere. These characteristics include a 4-GeV electron beam, a precision tracker, electromagnetic and hadronic calorimeters with near 2p azimuthal acceptance from the forward beam axis out to 40◦ angle, and low reconstruction energy threshold. LDMX thus could provide (semi)exclusive cross section measurements, with∼ detailed information about final-state electrons, pions, protons, and neutrons. We compare the predictions of two widely used neutrino generators (GENIE, GiBUU) in the LDMX region of acceptance to illustrate the large modeling discrepancies in electron-nucleus interactions at DUNE-like kinematics. -
Accelerator Search of the Magnetic Monopo
Accelerator Based Magnetic Monopole Search Experiments (Overview) Vasily Dzhordzhadze, Praveen Chaudhari∗, Peter Cameron, Nicholas D’Imperio, Veljko Radeka, Pavel Rehak, Margareta Rehak, Sergio Rescia, Yannis Semertzidis, John Sondericker, and Peter Thieberger. Brookhaven National Laboratory ABSTRACT We present an overview of accelerator-based searches for magnetic monopoles and we show why such searches are important for modern particle physics. Possible properties of monopoles are reviewed as well as experimental methods used in the search for them at accelerators. Two types of experimental methods, direct and indirect are discussed. Finally, we describe proposed magnetic monopole search experiments at RHIC and LHC. Content 1. Magnetic Monopole characteristics 2. Experimental techniques 3. Monopole Search experiments 4. Magnetic Monopoles in virtual processes 5. Future experiments 6. Summary 1. Magnetic Monopole characteristics The magnetic monopole puzzle remains one of the fundamental and unsolved problems in physics. This problem has a along history. The military engineer Pierre de Maricourt [1] in1269 was breaking magnets, trying to separate their poles. P. Curie assumed the existence of single magnetic poles [2]. A real breakthrough happened after P. Dirac’s approach to the solution of the electron charge quantization problem [3]. Before Dirac, J. Maxwell postulated his fundamental laws of electrodynamics [4], which represent a complete description of all known classical electromagnetic phenomena. Together with the Lorenz force law and the Newton equations of motion, they describe all the classical dynamics of interacting charged particles and electromagnetic fields. In analogy to electrostatics one can add a magnetic charge, by introducing a magnetic charge density, thus magnetic fields are no longer due solely to the motion of an electric charge and in Maxwell equation a magnetic current will appear in analogy to the electric current. -
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. -
Selfconsistent Description of Vector-Mesons in Matter 1
Selfconsistent description of vector-mesons in matter 1 Felix Riek 2 and J¨orn Knoll 3 Gesellschaft f¨ur Schwerionenforschung Planckstr. 1 64291 Darmstadt Abstract We study the influence of the virtual pion cloud in nuclear matter at finite den- sities and temperatures on the structure of the ρ- and ω-mesons. The in-matter spectral function of the pion is obtained within a selfconsistent scheme of coupled Dyson equations where the coupling to the nucleon and the ∆(1232)-isobar reso- nance is taken into account. The selfenergies are determined using a two-particle irreducible (2PI) truncation scheme (Φ-derivable approximation) supplemented by Migdal’s short range correlations for the particle-hole excitations. The so obtained spectral function of the pion is then used to calculate the in-medium changes of the vector-meson spectral functions. With increasing density and temperature a strong interplay of both vector-meson modes is observed. The four-transversality of the polarisation tensors of the vector-mesons is achieved by a projector technique. The resulting spectral functions of both vector-mesons and, through vector domi- nance, the implications of our results on the dilepton spectra are studied in their dependence on density and temperature. Key words: rho–meson, omega–meson, medium modifications, dilepton production, self-consistent approximation schemes. PACS: 14.40.-n 1 Supported in part by the Helmholz Association under Grant No. VH-VI-041 2 e-mail:[email protected] 3 e-mail:[email protected] Preprint submitted to Elsevier Preprint Feb. 2004 1 Introduction It is an interesting question how the behaviour of hadrons changes in a dense hadronic medium. -
From Quark and Nucleon Correlations to Discrete Symmetry and Clustering
From quark and nucleon correlations to discrete symmetry and clustering in nuclei G. Musulmanbekov JINR, Dubna, RU-141980, Russia E-mail: [email protected] Abstract Starting with a quark model of nucleon structure in which the valence quarks are strongly correlated within a nucleon, the light nu- clei are constructed by assuming similar correlations of the quarks of neighboring nucleons. Applying the model to larger collections of nucleons reveals the emergence of the face-centered cubic (FCC) sym- metry at the nuclear level. Nuclei with closed shells possess octahedral symmetry. Binding of nucleons are provided by quark loops formed by three and four nucleon correlations. Quark loops are responsible for formation of exotic (borromean) nuclei, as well. The model unifies independent particle (shell) model, liquid-drop and cluster models. 1 Introduction arXiv:1708.04437v2 [nucl-th] 19 Sep 2017 Historically there are three well known conventional nuclear models based on different assumption about the phase state of the nucleus: the liquid-drop, shell (independent particle), and cluster models. The liquid-drop model re- quires a dense liquid nuclear interior (short mean-free-path, local nucleon interactions and space-occupying nucleons) in order to predict nuclear bind- ing energies, radii, collective oscillations, etc. In contrast, in the shell model each point nucleon moves in mean-field potential created by other nucleons; the model predicts the existence of nucleon orbitals and shell-like orbital- filling. The cluster models require the assumption of strong local-clustering 1 of particularly the 4-nucleon alpha-particle within a liquid or gaseous nuclear interior in order to make predictions about the ground and excited states of cluster configurations. -
An Analysis on Single and Central Diffractive Heavy Flavour Production at Hadron Colliders
416 Brazilian Journal of Physics, vol. 38, no. 3B, September, 2008 An Analysis on Single and Central Diffractive Heavy Flavour Production at Hadron Colliders M. V. T. Machado Universidade Federal do Pampa, Centro de Cienciasˆ Exatas e Tecnologicas´ Campus de Bage,´ Rua Carlos Barbosa, CEP 96400-970, Bage,´ RS, Brazil (Received on 20 March, 2008) In this contribution results from a phenomenological analysis for the diffractive hadroproduction of heavy flavors at high energies are reported. Diffractive production of charm, bottom and top are calculated using the Regge factorization, taking into account recent experimental determination of the diffractive parton density functions in Pomeron by the H1 Collaboration at DESY-HERA. In addition, multiple-Pomeron corrections are considered through the rapidity gap survival probability factor. We give numerical predictions for single diffrac- tive as well as double Pomeron exchange (DPE) cross sections, which agree with the available data for diffractive production of charm and beauty. We make estimates which could be compared to future measurements at the LHC. Keywords: Heavy flavour production; Pomeron physics; Single diffraction; Quantum Chromodynamics 1. INTRODUCTION the diffractive quarkonium production, which is now sensitive to the gluon content of the Pomeron at small-x and may be For a long time, diffractive processes in hadron collisions particularly useful in studying the different mechanisms for have been described by Regge theory in terms of the exchange quarkonium production. of a Pomeron with vacuum quantum numbers [1]. However, the nature of the Pomeron and its reaction mechanisms are In order to do so, we will use the hard diffractive factoriza- not completely known. -
Introduction to Elementary Particle Physics
Introduction to Elementary Particle Physics Joachim Meyer DESY Lectures DESY Summer Student Program 2009 Preface ● This lecture is not a powerpoint show ● This lecture does not substitute an university course ● I know that your knowledge about the topic varies a lot ● So we have to make compromises in simplicity and depth ● Still I hope that all of you may profit somehow ● The viewgraphs shown are only for illustrations ● We will develop things together in discussion and at blackboard ● I hope there are lots of questions. I shall ask you a lot 2 Structures at different sizes Elementary Particle Physics 3 3 Fermion Generations Interactions through Gauge Boson Exchange This lecture is going to tell you something about HOW we arrived at this picture 4 Content of this lectures . Its only a sketch : Depending on your preknowledge we will go more or less in detail in the different subjects 5 6 WHY High Energies ? 7 The very basic minimum you have to know about Relativistic Kinematics 8 Which CM-energy do we reach at HERA ? 9 HEP 100 Years ago : Radioactive Decay Energy region : MeV =He−nucleus....=electron...= photon 10 Today : Some more particles : 11 The Particle Zoo I can't spare you this chapter. Quarks are nice to EXPLAIN observed phenomena. But, what we OBSERVE are particles like protons, muons, pions,.......... 12 'Artificial' Production of New Particles (Resonances): − p scattering 13 Particle classification Hadrons : strongly interacting Leptons : not Strongly interacting 14 All these particles are listed in the Particle Data Booklet