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Subatomic Physics

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298 The Electromagnetic Interaction<br />

ˆɛ must be in the xy plane. With the angles θ and ϕ as defined in Fig. 10.6, the components<br />

of 〈β|x|α〉 and ˆɛ are 〈β|x|α〉 = |〈β|x|α〉|(sin θ, 0, cos θ), ˆɛ =(cosϕ, sin ϕ, 0).<br />

Performing the scalar product in Eq. (10.74) then gives<br />

dwβα = e2<br />

2π� 4 c 3 E3 γ |〈β|x|α〉|2 sin 2 θ cos 2 ϕdΩ. (10.75)<br />

If the polarization of the emitted photon is not observed, dwβα must be integrated<br />

over the angle ϕ and summed over the two polarization states. The sum introduces<br />

afactor2;with<br />

dΩ =sinθdθdϕ and<br />

� 2π<br />

the transition rate for an unpolarized photon becomes<br />

0<br />

dϕ cos 2 ϕ = π,<br />

dwβα = e2<br />

� 4 c 3 E3 γ|〈β|x|α〉| 2 sin 3 θdθ. (10.76)<br />

The total transition rate wβα is obtained by integration over dθ,<br />

wβα =<br />

� π<br />

The lifetime (mean life) is the reciprocal of wβα.<br />

0<br />

dwβα = 4 e<br />

3<br />

2<br />

�4c3 E3 γ |〈β|x|α〉|2 . (10.77)<br />

The physical content of the expression (10.77) for the total transition rate becomes<br />

more transparent if appropriate units are introduced. If the decaying system<br />

or particle has a mass m, then the characteristic length associated with it is the<br />

Compton wavelength, λc = �/mc, andE0 = mc 2 is the characteristic energy. The<br />

time that it takes light to move the distance λc is given by t0 = �/mc 2 ,andthe<br />

inverse of this time, w0 =1/t0 = mc 2 /�, is the characteristic transition rate. With<br />

λc,E0 = mc 2 ,andw0, the transition rate is rewritten as<br />

wβα<br />

w0<br />

= 4<br />

3<br />

� e 2<br />

�c<br />

��<br />

Eγ<br />

mc2 �3 2 |〈β|x|α〉|<br />

λ 2 . (10.78)<br />

c<br />

The transition rate, expressed in terms of the “natural” rate w0, becomes a product<br />

of three dimensionless factors, each of which has a clear physical interpretation.<br />

The last term, |〈β|x|α〉| 2 /λ 2 c , contains the information about the structure of the<br />

decaying system. If the wave functions Φα and Φβ are known, the electric dipole<br />

matrix element 〈β|x|α〉 can be computed. Even without calculation, however, some<br />

properties can be deduced. For instance, the states |α〉 and |β〉 must have opposite<br />

parities; otherwise 〈β|x|α〉 vanishes, and no electric dipole radiation can be emitted.

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