Proceedings of the International School of Physics "Enrico Fermi.", Volume 11N. Zanichelli, 1960 - Nuclear physics |
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Page 29
Decay problems . Weak interactions can , because of their weakness , practically
only be studied in decay processes . S matrix theory is not directly applicable on
decay processes since only states of stable particles can occur as initial or final ...
Decay problems . Weak interactions can , because of their weakness , practically
only be studied in decay processes . S matrix theory is not directly applicable on
decay processes since only states of stable particles can occur as initial or final ...
Page 332
B In summary , we repeat that the success of the ( 1 - 1 ) weak - interaction
current hypothesis for B - decay , p - decay and i - - capture has led to the
suggestion that it should be extended to strange particle decay processes . We
have seen that ...
B In summary , we repeat that the success of the ( 1 - 1 ) weak - interaction
current hypothesis for B - decay , p - decay and i - - capture has led to the
suggestion that it should be extended to strange particle decay processes . We
have seen that ...
Page 339
If S were coupled , then by coupling it with Si + 1 ) one would have weak
interactions with AS = £2 , which seem to be excluded experimentally Now what
about neutral current ? One can define a neutral lepton current pro countaining (
vv ) , ( e ...
If S were coupled , then by coupling it with Si + 1 ) one would have weak
interactions with AS = £2 , which seem to be excluded experimentally Now what
about neutral current ? One can define a neutral lepton current pro countaining (
vv ) , ( e ...
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Contents
GENERALITĄ | 1 |
PARTE PRIMA Problemi teorici | 9 |
PARTE SECONDA Correlazioni angolari polarizzazioni e decadimenti beta | 197 |
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allowed angle angular assumed calculated charge classical combination completely component connection conservation consider constant contribute correlation corresponding coupling curvature decay defined density dependence derived described determination direction discussed effects electric electromagnetic field electron element elementary emission energy equations example existence experiment experimental expression factor Fermi field final finds formula function geometrodynamics geometry give given gravitational histories initial interaction invariance known leads limit magnetic mass matrix means measured metric modes momentum neutrino neutron nuclei nucleons observed obtained operators pairs parity particle phase Phys physics polarization possible present principle problem properties purely quantity quantum quantum mechanics question radiation ratio reason reference relation relativity requires respect result scattering shown shows solution space spin symmetry Table theory transformation transitions universe vector wave weak zero