Proceedings of the International School of Physics "Enrico Fermi.", Volume 11N. Zanichelli, 1960 - Nuclear physics |
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Page 30
If the strong interactions are irrelevant for the process under consideration phasiz
orde ( III . 17 ) < a | 8 , 16 ) = ( a 16 ) er der one finds the particularly simple result
( * ) I low 0 ( I11 . 18 ) ( a [ MK , = { Ta | M | Tk * . white , immed 18 dec of oth ...
If the strong interactions are irrelevant for the process under consideration phasiz
orde ( III . 17 ) < a | 8 , 16 ) = ( a 16 ) er der one finds the particularly simple result
( * ) I low 0 ( I11 . 18 ) ( a [ MK , = { Ta | M | Tk * . white , immed 18 dec of oth ...
Page 337
The B - decay hamiltonian must therefore have the form ( 6 ) where the coupling
constant has been called V & G to respect old traditions . This is the A – ”
coupling . If n and p are antifermions one finds instead V & G ( 9 . 7 , āy ) ( , 797 . )
, which ...
The B - decay hamiltonian must therefore have the form ( 6 ) where the coupling
constant has been called V & G to respect old traditions . This is the A – ”
coupling . If n and p are antifermions one finds instead V & G ( 9 . 7 , āy ) ( , 797 . )
, which ...
Page 358
Integrating over dx one finds that Z must be a one pion state . But for such a state
in the 10 - ja ) ( 019 ( x ) = ) = 0 , ( 3 . 18 ) which shows that this contribution is
zero . Now the last two terms . They contain 8 ( t ) and 8 ( t ) . By partial integration
...
Integrating over dx one finds that Z must be a one pion state . But for such a state
in the 10 - ja ) ( 019 ( x ) = ) = 0 , ( 3 . 18 ) which shows that this contribution is
zero . Now the last two terms . They contain 8 ( t ) and 8 ( t ) . By partial integration
...
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Contents
GENERALITÀ | 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