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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Particle Dispersion and Decays in Media 215<br />

Fig. 6.5. Dispersion relation <strong>for</strong> transverse modes according to Eq. (6.44).<br />

Fig. 6.6. Dispersion relation <strong>for</strong> longitudinal modes according to Eq. (6.44).<br />

Second, <strong>for</strong> v ∗ < 1 there is always a wave number k 1 where ω(k)<br />

“crosses the light cone” (ω/k = 1),<br />

k 2 1 = 4α π<br />

= ω 2 P<br />

∫ ∞<br />

3<br />

0<br />

v 2 ∗<br />

p 2 [ ( )<br />

1 1 + v<br />

dp f p<br />

E v log 1 − v<br />

[ ( )<br />

1 1 + v∗<br />

log − 1<br />

2v ∗ 1 − v ∗<br />

]<br />

− 1<br />

]<br />

. (6.48)<br />

The second identity (Braaten and Segel 1993) applies at the same level<br />

of approximation <strong>as</strong> π T,L in Eq. (6.38). Some analytic limiting c<strong>as</strong>es

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