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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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146 Chapter 4<br />

4.6.6 Cl<strong>as</strong>sical vs. Quantum Result<br />

In order to make contact with the quantum calculation that led to the<br />

axion emission rate in Eq. (4.6) it is useful to juxtapose it with the<br />

cl<strong>as</strong>sical result in terms of the spin-density structure function. The<br />

cl<strong>as</strong>sical calculation led to<br />

S σ (ω) = Γ σ<br />

ω 2 × ω 2<br />

ω 2 + Γ 2 σ/4<br />

while the quantum result is<br />

S σ (ω) = Γ σ<br />

ω 2 × s(ω/T ) × { 1 <strong>for</strong> ω > 0,<br />

e ω/T <strong>for</strong> ω < 0.<br />

(4.70)<br />

(4.71)<br />

The function s(x) h<strong>as</strong> the property s(0) = 1, it is even, and according<br />

to the f-sum rule must decre<strong>as</strong>e <strong>for</strong> large x. In Fig. 4.7 the cl<strong>as</strong>sical and<br />

quantum results are shown <strong>as</strong> dotted and d<strong>as</strong>hed lines, respectively,<br />

where <strong>for</strong> the purpose of illustration s(x) = (1 + x 2 /4) −1/4 h<strong>as</strong> been<br />

<strong>as</strong>sumed.<br />

Fig. 4.7. Cl<strong>as</strong>sical, quantum, and compound spin-density structure function<br />

in the nondegenerate limit according to Eq. (4.70) and Eq. (4.71) with<br />

Γ σ /T = 0.2 and s(x) = (1 + x 2 /4) −1/4 .<br />

This comparison highlights an important weakness of the cl<strong>as</strong>sical<br />

result: it does not obey the detailed-balance requirement S σ (ω) =<br />

S σ (−ω) e ω/T . The cl<strong>as</strong>sical correlators are invariant under time reflection<br />

t → −t and thus symmetric under ω → −ω. Again, the cl<strong>as</strong>sical<br />

result is adequate only <strong>for</strong> |ω| ∼ < T .

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