introduction-weak-interaction-volume-one
introduction-weak-interaction-volume-one
introduction-weak-interaction-volume-one
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We find that any wave function 14r(x) satisfies both the free Dirac equatio n<br />
( r (Zxr) + m)q( x ) = o , (3 .6 .18 )<br />
and also the 'chirality' relation<br />
+ ( 1 + Y 5 ) 5(x) = X ( x ) . (3 .6 .19 )<br />
We now postulate that all spin - particles may be described by two-comp<strong>one</strong>n t<br />
spinors of the form x(x), and from our definition (3 .6 .16), (3 .6 .17), we<br />
may immediately deduce that l<br />
e<br />
1 (1 + Y 5) (3 .6 .20 )<br />
This now implies a V - A structure for beta decay in the same manner a s<br />
did the Marshak-Sudarshan formulation (46) .<br />
The third theoretical justification for a V - A <strong>interaction</strong> wa s<br />
proposed by Sakurai in 1958 (49) . He noticed that the Dirac equation<br />
was invariant under the two transformations<br />
9 Y 5 (3 .6 .21a )<br />
m >,- m (3 .6 .21b )<br />
applied simultaneously, where<br />
2<br />
= 1 . (3 .6 .21c )<br />
This is known as 'mass-reversal' invariance . We now observe that th e<br />
relativistic requiremen t<br />
m2 = p0 2 -<br />
1 2 1 2 (3 .6 .22 )<br />
involves only m2 and not m, and hence does not determine its sign . Thus<br />
we are forced to conclude that the relation<br />
(fr (a/axr ) - m) r 5 " V(x) = 0 (3 .6 .23 )<br />
is exactly equivalent to the usual Dirac equation (3 .6 .18) . Using the<br />
argument outlined above, we see that the Sakurai formulation also<br />
predicts a V - A form for the beta decay <strong>interaction</strong> Hamiltonian . We<br />
note, however, that sofar, we have produced no theoretical or experimental<br />
evidence concerning the relative signs of the V and A couplings .<br />
1 . Assuming 'chirality invariance' .