Quarks and Hadrons. Properties of hadrons Pions and nucleons Strange particles Charm and beauty Breit-Wigner distribution Exotics

Similar documents
M. Cobal, PIF 2006/7. Quarks

Interactions and Fields

Some fundamental questions

M. Cobal, PIF 2006/7. Quarks

Discovery of Pions and Kaons in Cosmic Rays in 1947

Quark Model. Mass and Charge Patterns in Hadrons. Spin-1/2 baryons: Nucleons: n: MeV; p: MeV

Overview. The quest of Particle Physics research is to understand the fundamental particles of nature and their interactions.

Quarks and hadrons. Chapter Quark flavor and color

January 31, PHY357 Lecture 8. Quark composition of hadrons. Hadron magnetic moments. Hadron masses

Quark model. Jan 30, 2006 Lecture 8 1

Most of Modern Physics today is concerned with the extremes of matter:

Dr Victoria Martin, Prof Steve Playfer Spring Semester 2013

Gian Gopal Particle Attributes Quantum Numbers 1

The Quark Parton Model

Most of Modern Physics today is concerned with the extremes of matter:

Lecture 9. Isospin The quark model

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes.

Part II Particle and Nuclear Physics Examples Sheet 1

Forefront Issues in Meson Spectroscopy

8. Quark Model of Hadrons

Quantum Field Theory. Ling-Fong Li. (Institute) Quark Model 1 / 14

PhysicsAndMathsTutor.com 1

Lecture 8. CPT theorem and CP violation

Hadronic Resonances in a Hadronic Picture. Daisuke Jido (Nuclear physics group)

Quantum Numbers. F. Di Lodovico 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F. Di Lodovico. Quantum Numbers.

PHYS 420: Astrophysics & Cosmology

Lecture 9 Valence Quark Model of Hadrons

Lecture 02. The Standard Model of Particle Physics. Part I The Particles

PhysicsAndMathsTutor.com

Electron-positron pairs can be produced from a photon of energy > twice the rest energy of the electron.

Particle Physics. Lecture 12: Hadron Decays.!Resonances!Heavy Meson and Baryons!Decays and Quantum numbers!ckm matrix

DEEP INELASTIC SCATTERING

Nuclear and Particle Physics 3: Particle Physics. Lecture 1: Introduction to Particle Physics February 5th 2007

The Standard Model. 1 st 2 nd 3 rd Describes 3 of the 4 known fundamental forces. Separates particle into categories

Production cross sections of strange and charmed baryons at Belle

Particle Physics. Lecture 11: Mesons and Baryons

Particle Physics: Problem Sheet 5

Visit for more fantastic resources. AQA. A Level. A Level Physics. Particles (Answers) Name: Total Marks: /30

Chapter 32 Lecture Notes

Charmed Baryon spectroscopy at Belle 1. Y. Kato KMI topics. Mainly based on the paper recently accepted by PRD ( arxiv: )

Exotic Hadrons. O Villalobos Baillie MPAGS PP5 November 2015

The SU(3) Group SU(3) and Mesons Contents Quarks and Anti-quarks SU(3) and Baryons Masses and Symmetry Breaking Gell-Mann Okubo Mass Formulae Quark-Mo

Name : Physics 490. Practice Final (closed book; calculator, one notecard OK)

Part 7: Hadrons: quarks and color

Chapter 46 Solutions

.! " # e " + $ e. have the same spin as electron neutrinos, and is ½ integer (fermions).

Quantum Numbers. Elementary Particles Properties. F. Di Lodovico c 1 EPP, SPA6306. Queen Mary University of London. Quantum Numbers. F.

1. Introduction. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 1. Introduction 1

Physics Quarknet/Service Learning

Overview of Elementary Particle Physics

Current knowledge tells us that matter is made of fundamental particle called fermions,

The Strong Interaction

Particle Discovery at the LHC. Sally Seidel University of New Mexico 20 October 2017 APS Four Corners Meeting

Particle Physics. All science is either physics or stamp collecting and this from a 1908 Nobel laureate in Chemistry

PHYS 3446 Lecture #17

Heavy Quark Baryons and Exotica

The Standard Model (part I)

cgrahamphysics.com Particles that mediate force Book pg Exchange particles

The Development of Particle Physics. Dr. Vitaly Kudryavtsev E45, Tel.:

Kai Zhu on behalf of BESIII collaboration Institute of High Energy Physics, Beijing March, Moriond QCD 2015

PG lectures- Particle Physics Introduction. C.Lazzeroni

Modern physics 1 Chapter 13

SECOND PUBLIC EXAMINATION. Honour School of Physics Part C: 4 Year Course. Honour School of Physics and Philosophy Part C C4: PARTICLE PHYSICS

Discrete Transformations: Parity

FXA Candidates should be able to :

Clebsch-Gordan Coefficients

L. David Roper

TETRAQUARKS AND PENTAQUARK(S)

Introduction to Elementary Particle Physics. Note 22 Page 1 of 8. Charm Quark Bottom Quark Top Quark Are there more lepton-quark generations?

Introduction. Read: Ch 1 of M&S

Physics 129. Nuclear and Particle Astrophysics Winter Lecture 2 - January 8 Cross Sections and Decay Rates

Discovery of c, b and t quarks and quarkonia Marco Schramm

This means that n or p form a doublet under isospin transformation. Isospin invariance simply means that. [T i, H s ] = 0

Option 212: UNIT 2 Elementary Particles

Weak interactions. Chapter 7

Heavy Quark Spectroscopy at LHCb

Hand of Anna Röntgen. From Life magazine,6 April 1896

Lecture 12 Weak Decays of Hadrons

The experimental discovery of charm quarks

Meson Spectroscopy Methods, Measurements & Machines

The Uncertainty Principle and the Quarks

ψ(t) = U(t) ψ(0). (6.1.1)

Physics 4213/5213 Lecture 1

6. QED. Particle and Nuclear Physics. Dr. Tina Potter. Dr. Tina Potter 6. QED 1

Heavy quark production in e + e - & pp collisions

NATIONAL OPEN UNIVERSITY OF NIGERIA

Essential Physics II. Lecture 14:

Do you know what is special about quarks?

Overview of Light-Hadron Spectroscopy and Exotics

Recent Result on Pentaquark Searches from

Lecture 23. November 16, Developing the SM s electroweak theory. Fermion mass generation using a Higgs weak doublet

INTRODUCTION TO THE STANDARD MODEL OF PARTICLE PHYSICS

Lecture PowerPoint. Chapter 32 Physics: Principles with Applications, 6 th edition Giancoli

Quark Model. Ling-Fong Li. (Institute) Note 8 1 / 26

Quarks and hadrons. Chapter 7

Problem Set # 1 SOLUTIONS

Hadron Spectroscopy at COMPASS

Part 6: Hadrons: quantum numbers and excited states

Lattice Methods for Hadron Spectroscopy: new problems and challenges

Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuanquanlu, Shijingshan district, Beijing, , China

Transcription:

Quarks and Hadrons Properties of hadrons Pions and nucleons Strange particles Charm and beauty Breit-Wigner distribution Exotics J. Brau Physics 661, Quarks and Hadrons 1

Quark Flavors 3 pairs Called generations Fractional charge J. Brau Physics 661, Introduction 2

Quark Flavor Interactions Strong EM Weak Gravity u d c s t b J. Brau Physics 661, Introduction 3

Quark Flavors Quantum Number Rest Mass, GeV up, down I = 1/2 m u m d 0.3 strange S = -1 m s 0.50 charm C = +1 m c 1.50 bottom B = -1 m b 4.5 top T = +1 m t 173 Particles comprised of these quarks will have masses determined roughly by the rest masses of the quarks (internal interactions alter the mass some) The strong interaction conserves each of the flavor quantum numbers J. Brau Physics 661, Introduction 4

Mass Spectrum of Standard Model Particles J. Brau Physics 661, Introduction 5

Quark Flavor Conservation Strange production and decay is a good example of how the quark flavor conservation law works Strange particles are always produced in pairs in strong interactions: π - p Λ Κ 0 S(Λ) = -1, contains strange quark S(K) = +1, contains antistrange quark this is a strong interaction and therefore has a large cross section In the decays of strange particles, the strangeness may vanish: Λ p π - ( {S = -1} {S = 0} ) this process is not allowed by the strong interaction, therefore must involve the weak interaction, and is therefore slow. J. Brau Physics 661, Introduction 6

Baryons and Mesons Quarks have never been observed in isolation in nature, in bounds states of three quarks or a quark and an antiquark baryon = QQQ {three quark state} meson = QQ {quark antiquark pair} Baryons and mesons are collectively referred to as hadrons and comprise all of the strongly interaction particles Baryons have half-integer spin (1/2, 3/2, 5/2, ) and mesons integer spin (0, 1, 2, ) Note exotics = QQQQ or QQQQQ J. Brau Physics 661, Introduction 7

Baryon Number Baryon number of quark is 1/3, and baryon number of anti-quark is -1/3 so B 1/3 [N(q) N(q)] Baryons have baryon number 1, anti-baryons have baryon number -1, and mesons have baryon number 0 J. Brau Physics 661, Quarks and Hadrons 8

Baryons and antibaryons J. Brau Physics 661, Introduction 9

Quark Mass There are two ways of describing the quark mass: constituent quark mass (used in Perkins) m(u) 0.31 GeV m(d) 0.31 GeV current quark mass m(u) 0.003 GeV m(d) 0.006 GeV Consider the mass of the two light mesons, the pion and the rho, both composed of ud m(pi) = 0.14 GeV m(rho) = 0.77 GeV constituent quark picture requires large spinorbit interaction energy to explain difference J. Brau Physics 661, Introduction 10

Pions Lightest mesons are π ± (140), π 0 (135), where the mass in MeV is indicated π ± decays to µ ± ν with τ = 2.6 x 10-8 sec, π 0 decays to γγ with τ = 0.8 x 10-16 sec J. Brau Physics 661, Quarks and Hadrons 11

Strange Particles The same year in which pions were discovered (1947), particles which were produced through the strong interaction, but decayed via the weak interaction were found in cosmic rays these were deemed strange particles because of this behavior. Associated production Strange particles are produced copiously on a time scale of 10-23 sec., but decay slowly on a time scale of 10-10 sec. This suggests (Pais) the production mechanism is entirely different from the decay mechanism Produced in pairs with property(strangeness) that is conserved by strong interactions, but not conserved by weak interaction eg. π - + p K + + Σ - or π - + p K 0 + Λ J. Brau Physics 661, Quarks and Hadrons 12

Strange Particles Kaons K 0 (498) = ds K + (494) = us K 0 (498) = sd K - (494) = su Lambda Λ(1116) = sud Sigma Σ + (1189) = suu Σ 0 (1193) = sud Σ - (1197) = sdd J. Brau Physics 661, Quarks and Hadrons 13

Strong Interactions & Strange Decays Decay of the Σ baryons Baryon Composition Q-value, MeV Decay Mode Lifetime, s Σ 0 (1192) uds 77 Λγ 10-19 Σ + (1189) uus 116 pπ 0 10-10 Σ 0 (1385) uds 135 Λπ 0 10-23 J. Brau Physics 661, Interactions/Weak Force/ Leptons 14

Strong Interactions & Strange Decays Decay of the Σ baryons Baryon Composition Q-value, MeV Decay Mode Lifetime, s Σ 0 (1192) uds 74 Λγ 10-19 Σ + (1189) uus 189 pπ 0 10-10 Σ 0 (1385) uds 208 Λπ 0 10-23 These are the Q-values given in Perkins Table 2.1, which are wrong. Correct values are 77, 116, and 135 J. Brau Physics 661, Interactions/Weak Force/ Leptons 15

Strong Interactions & Strange Decays Decay of the Σ baryons Baryon Composition Q-value, MeV Decay Mode Lifetime, s Σ 0 (1192) uds 77 Λγ 10-19 Σ + (1189) uus 116 pπ 0 10-10 Σ 0 (1385) uds 135 Λπ 0 10-23 why is the Σ 0 (1192) 3 MeV heavier than the Σ + (1189)? why does the Σ + (1189) live a billion times longer than the Σ 0 (1192)? J. Brau Physics 661, Interactions/Weak Force/ Leptons 16

Strong Interactions & Strange Decays Decay of the Σ baryon 1385 - Σ 0 (1385) M Λ = 1115 MeV/c 2 M p = 938 MeV/c 2 M π = 140 MeV/c 2 1255 - Λπ 0 1190 - Σ 0 (1192) Σ + (1189) 1115-1078 - Λγ pπ 0 Q = 0 Q = +1 J. Brau Physics 661, Interactions/Weak Force/ Leptons 17

Strong Interactions & Strange Decays Decay of the Σ baryon 1385 - Σ 0 (1385) 1250 - Λπ 0 strong (pion) M Λ = 1115 MeV/c 2 M p = 938 MeV/c 2 M π = 135 MeV/c 2 1190-1115 - 1073 - Σ 0 (1192) Λγ EM (photon) Σ + (1189) pπ 0 Weak (why not strong?) Q = 0 Q = +1 J. Brau Physics 661, Interactions/Weak Force/ Leptons 18

Strong Interactions & Strange Decays Decay of the Σ baryons Baryon Composition Q-value, MeV Decay Mode Lifetime, s Σ 0 (1192) uds 77 Λγ (EM) 10-19 Σ + (1189) uus 116 pπ 0 (weak) 10-10 Σ 0 (1385) uds 135 Λπ 0 (strong) 10-23 strong EM Σ 0 (1192) cannot decay strongly because M Λ + M π = 1250 MeV/c 2 Σ + (1189) cannot decay strongly (same reason) Σ + (1189) cannot decay Emly because there is no lighter charged, strange baryon (Σ + (1189) is lightest charged, strange baryon) J. Brau Physics 661, Interactions/Weak Force/ Leptons 19

Strong Interactions & Strange Decays The ratios of the decay rates give an approximate indication of the relative strengths of the interactions: {τ[σ 0 (1192) ] / τ[σ 0 (1385) ] } 1/2 100 α s / α Since α = 1/137, α s 1 J. Brau Physics 661, Interactions/Weak Force/ Leptons 20

Charm and Beauty In 1970, three quarks explained all known hadrons. During the 1970 s, two more quarks were discovered charm, 1974 bottom, 1977 In 1995, the top quark was finally observed Flavor I I 3 S C B * T Q/e u 1/2 1/2 0 0 0 0 +2/3 d 1/2-1/2 0 0 0 0-1/3 s 0 0-1 0 0 0-1/3 c 0 0 0 1 0 0 +2/3 b 0 0 0 0-1 0-1/3 t 0 0 0 0 0 1 +2/3 J. Brau Physics 661, Quarks and Hadrons 21

Discovery of Charm 1974 two complementary experiments SLAC: e + e - ψ hadrons e + e -, µ + µ - BNL: p + Be J/ψ + anything e + e - J. Brau Physics 661, Quarks and Hadrons 22

Discovery of Charm 1974 SLAC: e + e - ψ hadrons hadrons e + e -, µ + µ - width dominated by experimental resolution µ + µ - Also observed second peak at 3.7 GeV (ψʹ ) e + e - J. Brau Physics 661, Quarks and Hadrons 23

Discovery of Charm 1974 BNL: p + Be J/ψ + anything e + e - J. Brau Physics 661, Quarks and Hadrons 24

Breit-Wigner Distribution When two particles collide, they can form an unstable, broad state, known as a resonance. The cross section which measures the probability of forming the resonant state follows the Breit- Wigner distribution: J. Brau Physics 661, Interactions/Weak Force/ Leptons 25

Breit-Wigner Distribution J. Brau Physics 661, Interactions/Weak Force/ Leptons 26

Breit-Wigner Distribution ψ(t) = ψ 0 e -Γ/2t e -ieo t Fourier Transform: ψ(e) = ψ(t) e iet dt = ψ 0 e -Γ/2t e -ieo t e iet dt = ψ 0 e i[(e - Eo) + iγ/2]t dt ψ(e) ~ 1/[E-E 0 +iγ/2] ψ(e) 2 ~ 1/[(E-E 0 ) 2 +Γ 2 /4] J. Brau Physics 661, Interactions/Weak Force/ Leptons 27

Breit-Wigner Distribution When spin and angular momentum are taken into consideration where λ is the wavelength of the scattered and scattering particle in their common CMS λ = h/p J. Brau Physics 661, Interactions/Weak Force/ Leptons 28

Breit-Wigner Distribution Elastic scattering el General scattering (i j) i j J. Brau Physics 661, Interactions/Weak Force/ Leptons 29

Discovery of Charm Total width from integral of the cross section: i j σ(e) de e + e - J. Brau Physics 661, Quarks and Hadrons 30

Discovery of Charm Total width from integral of the cross section: i j σ(e) de Γ i = Γ j = Γ ee Let x = 2(E-E R )/Γ, dx = 2dE/Γ, de=(γ/2) dx 2J+1=3 and 2s a +1=2s b +1=2 σ(e) de = 3π/2 λ 2 (Γ ee /Γ) 2 Γ dx (1+x 2 ) J. Brau Physics 661, Quarks and Hadrons 31 π

Discovery of Charm Total width from integral of the cross section: i j σ(e) de = 3π 2 /2 λ 2 (Γ ee /Γ) 2 Γ = 800 nb MeV Γ ee /Γ = 0.06 λ = hc/pc = 197 MeV-fm/1550 MeV Γ = 0.093 MeV (very narrow) Ref: Particle Data Group J. Brau Physics 661, Quarks and Hadrons 32

Vector mesons: Discovery of Charm Γ. ρ(776 MeV) 150 MeV ω(784 MeV) 8.4 MeV J/ψ(3100 MeV) 0.093 MeV Γ ee ρ(776 MeV) 6.8 kev φ(1020 MeV) 1.4 kev ω(784 MeV) 0.6 kev J/ψ(3100 MeV) 5 kev J. Brau Physics 661, Quarks and Hadrons 33

Discovery of Charm Shape of the resonance was consistent with J p = 1 - interference of the direct and virtual photon channels ratio of decay modes (such as ρ 0 π 0 and ρ - π + ) shows J/ψ is I=0 state J. Brau Physics 661, Quarks and Hadrons 34

Discovery of Charm ψ(3700) ψ(3100) π + π - J. Brau Physics 661, Quarks and Hadrons 35

Discovery of Charm Ref: Particle Data Group R = σ (e + e - hadrons) / σ PT (e + e - µ + µ - ) consider e + e - hadrons as e + e - QQ, summed over all quarks σ PT (e + e - µ + µ - ) = 4πα 2 / 3s = 87nb / s(gev 2 ) (point cross section) J. Brau Physics 661, Quarks and Hadrons 36

Discovery of Charm Narrowness of ψ(3100) and ψ(3700) explained by QCD, 3G exchange required Colorless, and C parity odd J. Brau Physics 661, Quarks and Hadrons 37

Discovery of Charm For heavier charmionium states, open charm decay modes open up -> broader resonances J. Brau Physics 661, Quarks and Hadrons 38

ψ(3100) ψ(3700) ψ(3770) ψ(4040) ψ(4160) ψ(4415) Discovery of Charm Γ = 0.093 MeV Γ = 0.30 MeV Γ = 27 ± 1 MeV Γ = 80 ± 10 MeV Γ = 103 ± 8 MeV Γ = 62 ± 20 MeV Open charm threshold Ref: Particle Data Group J. Brau Physics 661, Quarks and Hadrons 39

Open Charm D + (1869) = cd C=+1 D 0 (1865) = cu C=+1 D - (1869) = dc C=-1 D 0 (1865) = uc C=-1 D s+ (1969) = cs C=+1, S=+1 D s- (1969) = sc C=-1, S=-1 Λ c+ (2285) = cdu C=+1 τ(charm) ~ 10-13 sec J. Brau Physics 661, Quarks and Hadrons 40

1977 history repeats itself Discovery of Beauty another narrow resonance this time at Fermilab p+be -> µ + µ - + anything p+cu -> µ + µ - + anything p+pt -> µ + µ - + anything 400 GeV protons J. Brau Physics 661, Quarks and Hadrons 41

Discovery of Beauty Electron-positron colliders refine measurements: DORIS at DESY, CLEO at Cornell J. Brau Physics 661, Quarks and Hadrons 42

Discovery of Beauty Ref: Particle Data Group J. Brau Physics 661, Quarks and Hadrons 43

Discovery of Beauty Mass Γ ee (kev) Γ (MeV) (MeV) ϒ(1S) 9460 1.34 0.054 ϒ(2S) 10023 0.61 0.032 ϒ(3S) 10355 0.020 ϒ(4S) 10579 0.27 20.5 ± 2.5 Ref: Particle Data Group J. Brau Physics 661, Quarks and Hadrons 44

Naked Bottom B + (5278) = ub B=+1 B 0 (5279) = db B=+1 B - (5278) = bu B=-1 B 0 (5279) = bd B=-1 Λ b0 (5624) = udb Ξ b0 (5792) = usb Ξ b- (5792) = dsb B=-1 B=-1, S=-1 B=-1, S=-1 τ(beauty) ~ 10-12 sec J. Brau Physics 661, Quarks and Hadrons 45

Exotics The allowed combinations of S and Q for q q q baryons and q q mesons BARYONS MESONS S Q S Q 0 2, 1, 0, -1 1 1, 0-1 1, 0, -1 0 1, 0, -1-2 0, -1-1 0, -1-3 -1 Exotic QNs can be formed by q q q q q or q q q q or only gluons (glueballs) J. Brau Physics 661, Quarks and Hadrons 46