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lecture 5. strong interactions. Q C D. quantum chromodynamics. -. quarks: triplets of SU(3). -. proton: ( u u d ) neutron: ( d d u ). -. problems of the quark model. s. s. s. Omega Minus: symmetric wave function. -. three s – quarks in the ground state:
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lecture 5 strong interactions QCD quantum chromodynamics
- quarks: triplets of SU(3)
- proton: ( u u d ) neutron: ( d d u )
- problems of the quark model
s s s Omega Minus: symmetric wave function
- • three s – quarks in the • ground state: • - spins aligned - • space wave function symmetric - problem: Pauli statistics
- 1964 O. Greenberg quarks ==> parastatistics of rank 3
- 1965 Han and Nambu quarks ==> integral charges
- broken
- 1971 color Fritzsch Gell-Mann q=> q q q SU(3,c)
- broken exact
baryons: (antisymmetric in color index) Hadrons: color singlets “white states”
- - Hadrons - white states
b r g
no problem with Pauli statistics antisymmetric in color
forces between the quarks: 1972: F., Gell-Mann 1973: F., Gell-Mann, Leutwyler gauge theory in color space ==> QCD
Lagrange function : ==> QED
- QED: photon - QCD: gluons
Q E D photon e e
gluon g g
QED photon electron
QCD gluon quark
gluon field strength self-interaction
g new quark 3-gluon interactions
2 g 4-gluon interactions
Quantum Field Theory: Finestructure constant becomes function of energy or scale due to quantum fluctuations of electron-positron pairs => partial screening of bare charge of the electron at distances less than the compton wavelength of the electron M. Gell-Mann, F. Low 1955
partial screening + - + + - - - -
- renormalization group M. Gell-Mann, F. Low - 1954
ALEPH L3 OPAL DELPHI LEP
- LEP: ~ 1/127
QCD: asymptotically free coupling at high energies ==> 0 Khriplovich t Hooft Gross, Wilczek Politzer
QED - QCD negativ!!!
as in QED const. = +5 const. = -16 -
QCD as
3 Quarks: u,d,s coupling ==>0
- infrared slavery
infrared slavery ==> Confinement
* * small distances: Coulomb potential