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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 -
Fundamentals of Particle Physics
Fundamentals of Par0cle Physics Particle Physics Masterclass Emmanuel Olaiya 1 The Universe u The universe is 15 billion years old u Around 150 billion galaxies (150,000,000,000) u Each galaxy has around 300 billion stars (300,000,000,000) u 150 billion x 300 billion stars (that is a lot of stars!) u That is a huge amount of material u That is an unimaginable amount of particles u How do we even begin to understand all of matter? 2 How many elementary particles does it take to describe the matter around us? 3 We can describe the material around us using just 3 particles . 3 Matter Particles +2/3 U Point like elementary particles that protons and neutrons are made from. Quarks Hence we can construct all nuclei using these two particles -1/3 d -1 Electrons orbit the nuclei and are help to e form molecules. These are also point like elementary particles Leptons We can build the world around us with these 3 particles. But how do they interact. To understand their interactions we have to introduce forces! Force carriers g1 g2 g3 g4 g5 g6 g7 g8 The gluon, of which there are 8 is the force carrier for nuclear forces Consider 2 forces: nuclear forces, and electromagnetism The photon, ie light is the force carrier when experiencing forces such and electricity and magnetism γ SOME FAMILAR THE ATOM PARTICLES ≈10-10m electron (-) 0.511 MeV A Fundamental (“pointlike”) Particle THE NUCLEUS proton (+) 938.3 MeV neutron (0) 939.6 MeV E=mc2. Einstein’s equation tells us mass and energy are equivalent Wave/Particle Duality (Quantum Mechanics) Einstein E -
Exploring the Spectrum of QCD Using a Space-Time Lattice
ExploringExploring thethe spectrumspectrum ofof QCDQCD usingusing aa spacespace--timetime latticelattice Colin Morningstar (Carnegie Mellon University) New Theoretical Tools for Nucleon Resonance Analysis Argonne National Laboratory August 31, 2005 August 31, 2005 Exploring spectrum (C. Morningstar) 1 OutlineOutline z spectroscopy is a powerful tool for distilling key degrees of freedom z calculating spectrum of QCD Æ introduction of space-time lattice spectrum determination requires extraction of excited-state energies discuss how to extract excited-state energies from Monte Carlo estimates of correlation functions in Euclidean lattice field theory z applications: Yang-Mills glueballs heavy-quark hybrid mesons baryon and meson spectrum (work in progress) August 31, 2005 Exploring spectrum (C. Morningstar) 2 MonteMonte CarloCarlo methodmethod withwith spacespace--timetime latticelattice z introduction of space-time lattice allows Monte Carlo evaluation of path integrals needed to extract spectrum from QCD Lagrangian LQCD Lagrangian of hadron spectrum, QCD structure, transitions z tool to search for better ways of calculating in gauge theories what dominates the path integrals? (instantons, center vortices,…) construction of effective field theory of glue? (strings,…) August 31, 2005 Exploring spectrum (C. Morningstar) 3 EnergiesEnergies fromfrom correlationcorrelation functionsfunctions z stationary state energies can be extracted from asymptotic decay rate of temporal correlations of the fields (in the imaginary time formalism) Ht −Ht z evolution in Heisenberg picture φ ( t ) = e φ ( 0 ) e ( H = Hamiltonian) z spectral representation of a simple correlation function assume transfer matrix, ignore temporal boundary conditions focus only on one time ordering insert complete set of 0 φφ(te) (0) 0 = ∑ 0 Htφ(0) e−Ht nnφ(0) 0 energy eigenstates n (discrete and continuous) 2 −−()EEnn00t −−()EEt ==∑∑neφ(0) 0 Ane nn z extract A 1 and E 1 − E 0 as t → ∞ (assuming 0 φ ( 0 ) 0 = 0 and 1 φ ( 0 ) 0 ≠ 0) August 31, 2005 Exploring spectrum (C. -
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. -
Theoretical and Experimental Aspects of the Higgs Mechanism in the Standard Model and Beyond Alessandra Edda Baas University of Massachusetts Amherst
University of Massachusetts Amherst ScholarWorks@UMass Amherst Masters Theses 1911 - February 2014 2010 Theoretical and Experimental Aspects of the Higgs Mechanism in the Standard Model and Beyond Alessandra Edda Baas University of Massachusetts Amherst Follow this and additional works at: https://scholarworks.umass.edu/theses Part of the Physics Commons Baas, Alessandra Edda, "Theoretical and Experimental Aspects of the Higgs Mechanism in the Standard Model and Beyond" (2010). Masters Theses 1911 - February 2014. 503. Retrieved from https://scholarworks.umass.edu/theses/503 This thesis is brought to you for free and open access by ScholarWorks@UMass Amherst. It has been accepted for inclusion in Masters Theses 1911 - February 2014 by an authorized administrator of ScholarWorks@UMass Amherst. For more information, please contact [email protected]. THEORETICAL AND EXPERIMENTAL ASPECTS OF THE HIGGS MECHANISM IN THE STANDARD MODEL AND BEYOND A Thesis Presented by ALESSANDRA EDDA BAAS Submitted to the Graduate School of the University of Massachusetts Amherst in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE September 2010 Department of Physics © Copyright by Alessandra Edda Baas 2010 All Rights Reserved THEORETICAL AND EXPERIMENTAL ASPECTS OF THE HIGGS MECHANISM IN THE STANDARD MODEL AND BEYOND A Thesis Presented by ALESSANDRA EDDA BAAS Approved as to style and content by: Eugene Golowich, Chair Benjamin Brau, Member Donald Candela, Department Chair Department of Physics To my loving parents. ACKNOWLEDGMENTS Writing a Thesis is never possible without the help of many people. The greatest gratitude goes to my supervisor, Prof. Eugene Golowich who gave my the opportunity of working with him this year. -
New Insights to Old Problems
New Insights to Old Problems∗ T. D. Lee Pupin Physics Laboratory, Columbia University, New York, NY, USA and China Center of Advanced Science and Technology (CCAST), Beijing, China Abstract From the history of the θ-τ puzzle and the discovery of parity non-conservation in 1956, we review the current status of discrete symmetry violations in the weak interaction. Possible origin of these symmetry violations are discussed. PACS: 11.30.Er, 12.15.Ff, 14.60.Pq Key words: history of discovery of parity violation, mixing angles, origin of symmetry violation, scalar field and properties of vacuum arXiv:hep-ph/0605017v1 1 May 2006 ∗Based on an invited talk given at the 2006 APS Meeting as the first presentation in the Session on 50 Years Since the Discovery of Parity Nonconservation in the Weak Interaction I, April 22, 2006 (Appendix A) 1 1. Symmetry Violations: The Discovery Almost exactly 50 years ago, I had an important conversation with my dear friend and colleague C. S. Wu. This conversation was critical for setting in mo- tion the events that led to the experimental discovery of parity nonconservation in β-decay by Wu, et al.[1]. In the words of C. S. Wu[2]: ”· · · One day in the early Spring of 1956, Professor T. D. Lee came up to my little office on the thirteenth floor of Pupin Physical Laboratories. He explained to me, first, the τ-θ puzzle. If the answer to the τ-θ puzzle is violation of parity–he went on–then the violation should also be observed in the space distribution of the beta-decay of polarized nuclei: one must measure the pseudo-scalar quantity <σ · p > where p is the electron momentum and σ the spin of the nucleus. -
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. -
The Standard Model Part II: Charged Current Weak Interactions I
Prepared for submission to JHEP The Standard Model Part II: Charged Current weak interactions I Keith Hamiltona aDepartment of Physics and Astronomy, University College London, London, WC1E 6BT, UK E-mail: [email protected] Abstract: Rough notes on ... Introduction • Relation between G and g • F W Leptonic CC processes, ⌫e− scattering • Estimated time: 3 hours ⇠ Contents 1 Charged current weak interactions 1 1.1 Introduction 1 1.2 Leptonic charge current process 9 1 Charged current weak interactions 1.1 Introduction Back in the early 1930’s we physicists were puzzled by nuclear decay. • – In particular, the nucleus was observed to decay into a nucleus with the same mass number (A A) and one atomic number higher (Z Z + 1), and an emitted electron. ! ! – In such a two-body decay the energy of the electron in the decay rest frame is constrained by energy-momentum conservation alone to have a unique value. – However, it was observed to have a continuous range of values. In 1930 Pauli first introduced the neutrino as a way to explain the observed continuous energy • spectrum of the electron emitted in nuclear beta decay – Pauli was proposing that the decay was not two-body but three-body and that one of the three decay products was simply able to evade detection. To satisfy the history police • – We point out that when Pauli first proposed this mechanism the neutron had not yet been discovered and so Pauli had in fact named the third mystery particle a ‘neutron’. – The neutron was discovered two years later by Chadwick (for which he was awarded the Nobel Prize shortly afterwards in 1935). -
The Algebra of Grand Unified Theories
The Algebra of Grand Unified Theories John Baez and John Huerta Department of Mathematics University of California Riverside, CA 92521 USA May 4, 2010 Abstract The Standard Model is the best tested and most widely accepted theory of elementary particles we have today. It may seem complicated and arbitrary, but it has hidden patterns that are revealed by the relationship between three ‘grand unified theories’: theories that unify forces and particles by extend- ing the Standard Model symmetry group U(1) × SU(2) × SU(3) to a larger group. These three are Georgi and Glashow’s SU(5) theory, Georgi’s theory based on the group Spin(10), and the Pati–Salam model based on the group SU(2)×SU(2)×SU(4). In this expository account for mathematicians, we ex- plain only the portion of these theories that involves finite-dimensional group representations. This allows us to reduce the prerequisites to a bare minimum while still giving a taste of the profound puzzles that physicists are struggling to solve. 1 Introduction The Standard Model of particle physics is one of the greatest triumphs of physics. This theory is our best attempt to describe all the particles and all the forces of nature... except gravity. It does a great job of fitting experiments we can do in the lab. But physicists are dissatisfied with it. There are three main reasons. First, it leaves out gravity: that force is described by Einstein’s theory of general relativity, arXiv:0904.1556v2 [hep-th] 1 May 2010 which has not yet been reconciled with the Standard Model. -
XIII Probing the Weak Interaction
XIII Probing the weak interaction 1) Phenomenology of weak decays 2) Parity violation and neutrino helicity (Wu experiment and Goldhaber experiment) 3) V- A theory 4) Structure of neutral currents Parity → eigenvalues of parity are +1 (even parity), -1 (odd parity) Parity is conserved in strong and electromagnetic interactions Parity and momentum operator do not commute! Therefore intrinsic partiy is (strictly speaken) defined only for particles AT REST If a system of two particles has a relative angular momentum L, total parity is given by: (*) where are the intrinsic parity of particles Parity is a multiplicative quantum number Parity of spin + ½ fermions (quarks, leptons) per definition P = +1 Parity of spin - ½ anti-fermions (anti-quarks, anti-leptons) P = -1 Parity of W, Z, photon, gluons (and their antiparticles) P =-1 (result of gauge theory) (strictly speaken parity of photon and gluons are not defined, use definition of field) For all other composed and excited particles e.g. kaon, proton, pion, use rule (*) and/or parity conserving IA to determine intrinsic parity Reminder: Parity operator: Intrinsic parity of spin ½ fermions AT REST: +1; of antiparticles: -1 Wu-Experiment Idea: Measurement of the angular distribution of the emitted electron in the decay of polarized 60Co nulcei Angular momentum is an axial vector P J=5 J=4 If P is conserved, the angular distribution must be symmetric (to the dashed line) Identical rates for and . Experiment: Invert 60Co polarization and compare the rates under the same angle . photons are preferably emitted in direction of spin of Ni → test polarization of 60Co (elm. -
– 1– LEPTOQUARK QUANTUM NUMBERS Revised September
{1{ LEPTOQUARK QUANTUM NUMBERS Revised September 2005 by M. Tanabashi (Tohoku University). Leptoquarks are particles carrying both baryon number (B) and lepton number (L). They are expected to exist in various extensions of the Standard Model (SM). The possible quantum numbers of leptoquark states can be restricted by assuming that their direct interactions with the ordinary SM fermions are dimensionless and invariant under the SM gauge group. Table 1 shows the list of all possible quantum numbers with this assumption [1]. The columns of SU(3)C,SU(2)W,andU(1)Y in Table 1 indicate the QCD representation, the weak isospin representation, and the weak hypercharge, respectively. The spin of a leptoquark state is taken to be 1 (vector leptoquark) or 0 (scalar leptoquark). Table 1: Possible leptoquarks and their quan- tum numbers. Spin 3B + L SU(3)c SU(2)W U(1)Y Allowed coupling c c 0 −2 311¯ /3¯qL`Loru ¯ReR c 0 −2 314¯ /3 d¯ReR c 0−2331¯ /3¯qL`L cµ c µ 1−2325¯ /6¯qLγeRor d¯Rγ `L cµ 1 −2 32¯ −1/6¯uRγ`L 00327/6¯qLeRoru ¯R`L 00321/6 d¯R`L µ µ 10312/3¯qLγ`Lor d¯Rγ eR µ 10315/3¯uRγeR µ 10332/3¯qLγ`L If we do not require leptoquark states to couple directly with SM fermions, different assignments of quantum numbers become possible [2,3]. The Pati-Salam model [4] is an example predicting the existence of a leptoquark state. In this model a vector lepto- quark appears at the scale where the Pati-Salam SU(4) “color” gauge group breaks into the familiar QCD SU(3)C group (or CITATION: S. -
Weak Interaction Processes: Which Quantum Information Is Revealed?
Weak Interaction Processes: Which Quantum Information is revealed? B. C. Hiesmayr1 1University of Vienna, Faculty of Physics, Boltzmanngasse 5, 1090 Vienna, Austria We analyze the achievable limits of the quantum information processing of the weak interaction revealed by hyperons with spin. We find that the weak decay process corresponds to an interferometric device with a fixed visibility and fixed phase difference for each hyperon. Nature chooses rather low visibilities expressing a preference to parity conserving or violating processes (except for the decay Σ+ pπ0). The decay process can be considered as an open quantum channel that carries the information of the−→ hyperon spin to the angular distribution of the momentum of the daughter particles. We find a simple geometrical information theoretic 1 α interpretation of this process: two quantization axes are chosen spontaneously with probabilities ±2 where α is proportional to the visibility times the real part of the phase shift. Differently stated the weak interaction process corresponds to spin measurements with an imperfect Stern-Gerlach apparatus. Equipped with this information theoretic insight we show how entanglement can be measured in these systems and why Bell’s nonlocality (in contradiction to common misconception in literature) cannot be revealed in hyperon decays. We study also under which circumstances contextuality can be revealed. PACS numbers: 03.67.-a, 14.20.Jn, 03.65.Ud Weak interactions are one out of the four fundamental in- systems. teractions that we think that rules our universe. The weak in- Information theoretic content of an interfering and de- teraction is the only interaction that breaks the parity symme- caying system: Let us start by assuming that the initial state try and the combined charge-conjugation–parity( P) symme- of a decaying hyperon is in a separable state between momen- C try.