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introduction-weak-interaction-volume-one

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CHAPTER TbO : FIELD THEORY .<br />

2 .1 The Operators PCT .<br />

The parity or space reflection operator, P, reverses the sign of the<br />

x-co-ordinates of a wave function, which is equivalent to reflecting it in th e<br />

plan e<br />

x _ 0 . (2 .1 .1 )<br />

Most physical systems can be described by wave functions which are eigenfunction s<br />

of the P operator . For these, we may write<br />

P ).T(z) (-R) = E, 4r(r) . (2 .1 .2 )<br />

From geometrical considerations, it is obvious that<br />

P2 Ni(r.) _ (=) (2 .1 .3 )<br />

and henc e<br />

EZ = 1, C _ } 1 (2 .1 .4 )<br />

Thus, for systems with only <strong>one</strong> linearly independent eigenfunction correspondin g<br />

to a particular eigenvalue, the wave function has a definite intrinsic parity, P ,<br />

which may be even (P = 1) or odd (P = -1) .<br />

We assume that we may write a Hamiltonian in terms of the three-vector<br />

x and that<br />

(2 .1 .5 )<br />

i .e . the Hamiltonian is invariant under the P operator . The time-dependen t<br />

Schrddinger equation (1 .3 .7) written in Hamiltonian form i s<br />

H ( x ) 1)-(x, t ) _ jY(ox1t)<br />

(2 .1 .6 )<br />

in natural units ( = c =1) . Replacing x by -x in (2.1 .6) and defining<br />

' (x, t ) _ t ), (2 .1 .7 )<br />

we have, using (2 .1 .5) ,<br />

H(z) ~ '(x, _ t) _ J {x't )<br />

(2 .1 .8)<br />

a t<br />

Thus the function Zf'(x, t) is a solution to the same differential equatio n<br />

as 1Y(x, t) .<br />

For the Dirac equation, we write the equation of motion of a particl e

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