\|\|\/|\\// ((o)) ((o)) U July 21, 2009 Lecture 3 of 4 @ ORICL Philosophical Phil hi l S Society i t Yuri Kamyshkov University of Tennessee kamyshkov@utk.edu Previous lectures are posted at http://web.utk.edu/~kamyshko/ORICL/ matter tt and d anti-matter ti tt particles ti l have h spin i ½ X; X use the same forces for interactions How quarks make protons, neutrons, and other particles Baryons Mesons Nucleons uc eo s hadrons π− = d u K 0 = d s (strangeness +1) π+ =u d K 0 = s d (strangeness − 1) ( ) Cπ = du = du = π − uu − dd π = 2 Cπ 0 = π 0 0 + CK 0 = K 0 p = uud ; p = uud Cp p = p; Cpp = p Cn = n ; Cn = n (qq ) Mesons [using u, d , s, c] (qqq ) Baryons [using u , d , s, c] Constituents of atomic nuclei = nucleons anti-nuclei = anti-nucleons proton quarks neutron baryons anti-proton, antineutron → anti-baryons Summary of terminology Leptons: electron, positron, neutrino, anti-neutrino (3 families) Quarks: do not exist as free objects, only inside hadrons Hadrons: made of quarks - Baryons and Mesons Baryons: objects made of 3 quarks ( qqq ) or ( qqq ) Mesons: objects made of quark and anti-quarks ( qq ) Pentaquarks: recently ? ( qqqqq ) ... not confirmed Can anti-matter be stored? Can not be stored like that The Low Energy Antiproton Ring (LEAR) at CERN (Geneva, Switzerland) The Antiproton Accumulator (AA) which has been transformed into the Antiproton Decelerator (AD) in 1999 Anti--hydrogen storage at CERN (Antiproton Decelerator) Anti Three experiments: p ASACUSA " Atomic Spectroscopy and Collisions using Slow Antiprotons"; ATHENA "Antihydrogen Production and Precision Experiments" and ATRAP "Cold Antihydrogen for Precise Laser Spectroscopy". Penning Trap Electron--Positron Annihilation Electron annihilation at rest − + e + e → γ + γ + (γ ) + − e e scattering e+ e+ γ e− e− As more energy is available the annihilation of electron and positron can lead to creation of many new particles, some more massive than electron or positron (e.g. at Large Electron – Positron collider at CERN) View of annihilation ☯ How will nucleon and antianti-nucleon annihilate ? Nucleon + antianti-nucleon annihilate mostly into pions. i Average A number b of pions = 5 Pions and muons eventually decay into stable particles: electrons positrons, electrons, positrons photons and neutrinos (~ 60% of energy ultimately is curried awayy byy neutrinos). ) π + → μ + +ν Antiproton annihilation in hydrogen bubble chamber H How neutrino-antineutrino i i i can annihilate? ihil ? If e+e− and pp― annihilate annihilate,, why e− and p+ do not ? i.e. why hydrogen atom is stable and there is no 1H (e−p+) → 2 γ ? or why doesn’t proton decay p → e+ γ ? Nucleons (p (p, n) and other heavy 3-quark particles are called Baryons e, ν, and other particles with similar properties are called Leptons Stability St bilit off the th matter tt (at ( t the th level l l observed b d so far) f ) can be b explained as a conservation of the global quantum numbers called “baryon charge” and “lepton charge”. Why baryon charge is conserved conserved?? H. Weyl (1929) H (1929), E. E Stueckelberg (1938) (1938), E. E Wigner (1949) independently tried to postulate the conservation of nucleon (baryon) charge by analogy with conservation of electric charge. Test results confirm strict conservation of electric charge How do we know whether “baryonic photons” exist? ((Lee ee & Yang, ang, Pati ati & Salam, Okun, Sakharov) Sakha ov) There are no reasons to believe that baryonic y charge g can be conserved for the same reason as electric charge , i.e. there is no good explanation of baryon and lepton number conservation. Sacred and Approximate Conservation Laws Sacred: conservation of energy-momentum, angular momentum, electric charge; casuality, casuality Lorentz invariance, invariance unitarity unitarity, CPT symmetry Approximate: Left-Right symmetry Particle-Antiparticle symmetry CP-symmetry y y T-symmetry Lepton family number (Lμ ,Le) Lepton number (L) Baryon number (B) (P-parity, fallen in 1956) (C-parity, fallen in 1956) ((fallen in 1964)) (fallen in 1999) (fallen in 1998) hold (to be tested in 2β0ν expts) hold (needs to be tested) The Universe Th U i provides id us an evidence id that net baryon number is not conserved