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ParticleZoo Nucleons Are Not Elementary Particles! eep hadron jet Scatter high-energy electrons off protons. If there is no internal structure of e- or p, then welldefined “elastic” e- energy for each angle. See structure!! scatter probability excited states of the proton elastic x1/8.5 Each line in the energy spectrum of scattered electrons ground state of the proton Bartel etal. PL28B, 148 (1968) energy of scattered electron corresponds to a different energy state of the proton. The Quark Model The quark model represents a relatively simple picture of the internal structure of subatomic particles and makes predictions of their production and decay. It uses a minimum of adjusted quark parameters and has great predictive power, e.g., for the composite-particle masses, magnetic moments, and lifetimes. There are no contradictions to this model known so far, (but many questions remain). Internal Nucleonic Structure e- e- The proton has internal structure, so-called quarks (u,u,d). Quarks combine to nucleon states of different excitations. Proton is the (u,u,d) ground state p 1200 MeV 938 MeV 135 MeV S=3/2 N S=½ e (1232) e p e (1450) e (1688) N: one doublet with a splitting of only m = 1.3 MeV : one quadruplet with a splitting of only m = 8 MeV p S=0 Mesons The Quark-Lepton Model of Matter Explains the consistency of the known particles in all of their states. 3 families of quarks (3 “colors” each) and associated leptons. All are spin-1/2 particles, quarks have non-integer charges Nucleons (q,q,q) Mesons (q, q-bar) q-bar:anti-quark Leptons Hadrons Baryons Particle Spectrum Mesons Simplified scheme of stable or unstable subatomic particles. Y'’ 4 Mass (GeV/c2) Y' Families have different interactions, Leptons: weak+elm, Hadrons: weak+elm+strong J/Y 3 “strange” 2 t W X* Y* X 8 S L N 1 10 K* w r h K 0 m n, e Spin ½ 8 p ½ 3/2 0 1 Each particle also has an anti-particle, with inverse quantum numbers. e e p p nn K K , etc. Quark Quantum Numbers All: spin=1/2, baryon number B=1/3 Flavor Q/e M/GeVc-2 T T3 S C B* Top u +2/3 0.005 ½ ½ 0 0 0 0 d -1/3 0.009 ½ -½ 0 0 0 0 s -1/3 0.175 0 0 -1 0 0 0 c +2/3 1.5 0 0 0 1 0 0 b -1/3 4.9 0 0 0 0 -1 0 t +2/3 162 0 0 0 0 0 1 T,T3: isospin; S: strangeness; C: charm; B*: bottom qu.#, Top: top qu.# Structure of Composite Particles There are only 3-quark (q,q,q) Baryons and quark-antiquark ( q, q ) configurations. No free quarks or higher quark multiplicities. _ _ _ u d s quarks antiquarks u s d s= 1/2 s= 0 0 T3 d d n u Sd d s S u u d p s d X- s S0 u d s L0 K0 S+ u u s s u s 0 X p_u d _ s d _ s u K+ p0 _ _ u u d d _ h h’ s s _ s u K- _ u s p_+ d u _ K0 s = 3/2 0 T3 0 d d d d d u S* d s d d u u S*0 d s u d X* s s S u S* s u u s s W s s s u u u X*0 Meson Wave Functions Examples to interpret the graphic shorthand in these figures: Mesons p ud p 0 p ud 1 uu dd 2 simple qq structure mixed qq state Meson spins are integer, vector sum of halfinteger quark and anti-quark spins, and their integer orbital angular momentum l. In ground state, mostly l =0. Baryon Wave Functions Examples to interpret the graphic shorthand: s 1/ 2 Baryons p u u d n d d u qqq structure s 3 / 2 Baryons 0 u d d u u d aligned qqq state These Baryon and Meson wave functions are schematic, do not have proper (anti-)symmetry property required by Pauli Principle: The total particle wave function (all coordinates) ( space) ( flavor ) ( spin) must be antisymmetric under quark exchange (quarks are fermions) Pauli Principle and Color Coordinate Quarks are Fermions no two same quarks can be in the same state d d d have both 3 identical fermions (same quarks) with same spins (S=3/2) and isospin (T3=+3/2) states u u u s3,T 3 s3,T 3 Violates Pauli Principle !? Conclusion: There must be an additional quantum number (degree of freedom), “color”. Need 3 colors and their anti-colors Red Green Blue Red Cyan, Green Magenta, Blue Yellow Color and complementary color (anti-color) add up to color-less (white) _ _ _ d d d d quarks anti-d quarks d d d Color Wave Function d d d d quarks anti-d quarks _ d _ d _ d ++ : Flavor and spin configurations symmetric, spatial configuration symmetric (no orbital angular momentum, l =0) color configuration must be antisymmetric. All colors are present with equal weights. All physical particles are “white.” Mesons rr p mix of ur d r , ub db , u g d g Baryons p mix of ur ub d g , ubur d g , ur u g db ,... Necessity of color rules out combinations such as (q),(q, q, q),..... There are no free quarks Confinement Gluons Bound quark systems (physical particles) by q-q interactions. Field quanta: 8 Gluons (not actually pions!) Spin and parity 1- like a photon. Gluons carry color and the corresponding anticolor. Color can be transferred but particle remains colorless. _ q qc’ qc gluon emission changes color q q-qbar creation self coupling of the color charges Usual conservation laws apply to reactions between quarks. time Gluon Exchange b _ b g _ g b _ b g b _ r _ d b g r u p g r u b Gluons are exchanged back and forth between q-q, g changing q colors and momenta dynamically r, g, and b are visited with equal probability r u p d Baryon Production with Strong Interactions Typically: Energetic projectile hits nucleon/nucleus, new particles are produced. Rules for strong interactions: •Energy, momentum, s, charge, baryon numbers, etc., conserved •q existing in system are rearranged, no flavor is changed •q-q-bar pairs can be produced p p u u d _ d u time annihilation d, d-bar u u s _ s u creation s, s-bar S Example p p S K K time Baryon Resonances p p+ _ d u u u d Typically: Energetic projectile hits nucleon/nucleus, intermediate particle is produced and decays into other particles. Example p p p p u u u ++ ++ produced as short-lived intermediate state, t = 0.5·10-23s corresp. width of state: G = ħ/t = 120 MeV u u d p _ d u p+ This happens with high probability when a nucleon of 300 MeV/c, or a relative energy of 1232 MeV penetrates into the medium of a nucleus. Resonance Confinement and Strings Why are there no free quarks? Earlier: symmetry arguments. Property of gluon interaction between color charges (“stringlike character). Q: Can one dissociate a qq pair? field lines: color strings energy in strings proportional to length 0.9GeV/fm successive q/q-bar creation, always in pairs! Leptons Leptons have their own quantum number, L, which is conserved. It seems likely, but is not yet known, whether electronic, muonic and tau lepton numbers are independently conserved in reactions and decays. Conservation Laws Quantum numbers are additive. Anti-quarks have all signs of quark quantum numbers reversed, except spin and isospin. Derived quantities: Charge Q e T3 (1 2) B S C B * Top Hypercharge Y B S In a reaction/transmutation, decay, the following quantities are conserved (before=after): •The total energy, momentum, angular momentum (spin), •The total charge, baryon number, lepton number Conservation Laws in Decays Decay A B + C possible, if mAc2 ≥ mBc2 + mCc2 Otherwise, balance must be supplied as kinetic energy. Relativistic energy of particle with rest mass m, momentum p : E pc 2 mc 2 2 Ekin mc 2 Example: Conservation of charge, baryon number, lepton number in neutron decay. n p e n e n decay p m n n m m capture B 1 1 0 0 1 Le 0 0 1 1 0 1 0 1 0 Lm 0 1 0 1 Q 0 e e 0 0 e e 00 Weak Interactions 10-5 weaker than strong interaction, small probabilities for reaction/decays. Mediated by heavy (mass ~100GeV) intermediate bosons W± ,Z0. Weak bosons can change quark flavor d u W+ u up-down conversion carries +e u Z0 W- s strange-non-strange conversion carries –e u no flavor change carries no charge Decays of W± and Z0 Bosons Hadronic decays to quark pair are dominant (>90%), leptonic decays are weak. All possible couplings: l , n e , n , m , n , t ,n t leptonic decays e m W q, q d , u , s, c , b, t hadronic decays l ,n e ,n e , m ,n m , t ,n t W q , q ' d , u , s , c , b , t l , l e , e , n e ,n e , m , m ), (n m ,n m , 0 Z t , t ), (n t ,n t q, q (d , d ), (u, u ), s, s ), (c, c , (b, b ), (t , t ) Examples of Weak Decays Can you predict, which (if any) weak boson effects the change? _ p ne p n e m ne ? ? time ? n n-decay? p n neutrino scattering off protons? nm e- neutrino-induced reaction off e-? Examples of Weak Decays Answer: Yes, all processes are possible. These are the bosons, p e- _ p ne n ne m W+ Z0 time W- n n-decay p n nm e- neutrino scattering neutrino-induced off protons reaction off e- Method: •Balance conserved quantities at the vortex, where boson originates. Remember W± carries away charge ±|e|. •Balance conserved quantities at lepton vortex. Particle Production probability In electron-positron collisions, particle-anti-particle pairs can be created out of collision energy, either via electromagnetic or weak interaction. collision energy (GeV) m+ m- e+ electromagnetic e- Z0 e+ weak m+ m- Z0 g e- antifermion fermion e- e+ example The Standard Model The body of currently accepted views of structure and interactions of subatomic particles. Interactions Interaction Coupling Charge Field Boson Mass/ GeVc-2 Jp strong color gluons (8) 0 1- elmgn electric (e) photon (g) 0 1- weak weak W+, W-, Z0 100 1 Weak interactions violate certain symmetries (parity, helicity) see later Particles Fermions Family Q/e Color Spin Weak Isospin Quarks u c t d s b +2/3 -1/3 r, b, g ½ ½ Leptons ne nm nt e m t 0 -1 none ½ ½ The Standard Model ct’d Combine weak and elm interactions “electro-weak” Type of isospin-symmetry: same particles carry weak and elm charge. Vqq Force range Electromagnetic: ∞ 0 1 fm 2mqc2 r Weak: 10-3fm Strong qq force increases with distance There are no free quarks. All free physical particles are colorless. The End