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and<br />

(5 .6 .26) might still be absent from the total Hamiltonian . Thus there<br />

exist two separate possibilities : first, the Hamiltonian contains onl y<br />

charged-current terms, and its Al<br />

= 3/2 is suppressed by the strong<br />

<strong>interaction</strong> ; and second, the Hamiltonian does, in fact, involve neutral<br />

lepton currents with a strength comparable to that of the charged lepto n<br />

currents . We now examine the predictions of these two models . Both indicat e<br />

<strong>weak</strong> .AY = 0 hadron <strong>interaction</strong>s . Assuming the Cabibbo form of universality<br />

(5 .6 .5), (5 .6 .9) become s<br />

HI (QY = 0) = -( G/ .!2") (cos2 e(Jr(l,l) J0(1,—1))<br />

-<br />

whereas (5.6.22) yields<br />

HI (AY = 0)<br />

+ sin2 6 (Jr(+, ) 5 .(+,—) ) ) , (5 .6.27 )<br />

-(G/4Q) (cos20 (Jr(l,l )<br />

a'Dr(l,-.1) - ( J0 ,0 ( 1 ,0 ) J<br />

0r,0(1,0)<br />

J<br />

J°0(0,0) JT0 0 (1,0) +<br />

r ,<br />

sin2 e (Jr(+,+) Jr(-,- )<br />

~ O ( r"~) Jr ,O(+4) ) ) (5.6.28 )<br />

r<br />

AY = 0 <strong>weak</strong> <strong>interaction</strong>s are usually difficult to study experimentally<br />

because they are masked by strong <strong>interaction</strong>s with a much larger amplitude .<br />

However, <strong>weak</strong> effects do give rise to parity-violating nuclear transitions,<br />

so that a nuclear state K no longer possesses a well-defined parity, bu t<br />

consists of a mixture of parities :<br />

1K> = IK + > + f (5.6.29 )<br />

where f is the parity-violating amplitude . From (5.6 .27) or (5.6 .28) we<br />

may predict (29 )<br />

f 10 7 . (5 .6.30 )<br />

Experiments use, for example, the fact that for the<br />

excited state of Ta 181 (482 keV, 5/2 1-<br />

a' ray connecting the<br />

) to the 7/2 + ground state, th e<br />

normal M1 transition matrix is suppressed by nuclear structure effect s 1° (30),<br />

so that the parity-violating II transition matrix produces an observabl e<br />

effect . Recent studies of the circular polarization in the gamma rays from<br />

Tal8l and L. 175 indicate that (31 )<br />

fTa<br />

, J° 0 (1,0) J°0(0,0) +<br />

r, r,<br />

+ JT°° (°, 0 ) Jr°° (°, 0)) )<br />

° (0 .4 - 4) x 10-7<br />

fLu = ( 2 - 8) x 10-7<br />

(5 .6.31 )<br />

(5 .6.32)

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