930 likes | 1.09k Views
weak interactions. weak decays beta decay of neutron. n. p. problem energy and momentum not conserved. e. W. Pauli: 1930 Neutrino mass ~ m(e). weak decays beta decay of neutron. n. p. e. electron. p. n. antineutrino.
E N D
weak interactions
weakdecays betadecay of neutron
n p problem energy and momentum not conserved e
W. Pauli: 1930 Neutrino mass ~ m(e)
weakdecays betadecay of neutron
n p e
electron p n antineutrino direct interaction of four fermions Enrico Fermi, ~1936
Enrico Fermi
weak interactions current-current interaction weak currents ~ lefthanded:
lefthanded fermion S= - 1/2 righthanded antifermion S = + 1/2
maximal breaking of parity
weak interaction of the quarks beta – decay d u
weak decays of strange particles ( u d s ) ( u u d ) s u
Cabibbo angle: flavor mixing
1957 weak bosons W J. Schwinger
- 1964 => 1968 gauge theory of the electroweak interactions ( Glashow, Salam, Weinberg )
Glashow Salam Weinberg 1964-1968
weak and electromagnetic interactions => electroweak interactions partial unification
gaugegroup SU(2)xU(1)
S U (2) xU (1) weak interaction electromagnetic interaction
4 gauge bosons W(+) W(-) Z photon
SU(2)xU(1) weak Interactions W(+) – W(-) photon neutral current - Z
photon: superposition SU(2) U(1)
Why photon massless? Why W–boson massive?
mass generation by spontaneous symmetry breaking
spontaneous symmetry breaking in classical mechanics rotation symmetry
direction singled out rotation symmetry broken
spontaneous symmetrrybreaking in fieldtheory
example 1: real scalar field V potential
spontaneous mass generation in gauge theories: U(1)