28.01.2015 Views

Stars as Laboratories for Fundamental Physics - MPP Theory Group

Stars as Laboratories for Fundamental Physics - MPP Theory Group

Stars as Laboratories for Fundamental Physics - MPP Theory Group

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

Particle Dispersion and Decays in Media 217<br />

<strong>as</strong> a resonance with a finite width Γ L . The approximate uncertainty<br />

±Γ L (k) of the energy ω(k) is shown in Fig. 6.4 <strong>as</strong> a shaded area.<br />

The damping rate Eq. (6.50) does not show a threshold effect at<br />

k = ω because it w<strong>as</strong> calculated nonrelativistically so that the highenergy<br />

tail of the electron distribution contains particles with velocities<br />

exceeding the speed of light. Tsytovich (1961) calculated a relativistic<br />

result with the correct threshold behavior. However, because the<br />

damping rate is exceedingly small <strong>for</strong> k ≪ k D , the correction is very<br />

small if ω P ≪ k D , equivalent to T ≪ m e . For the degenerate c<strong>as</strong>e,<br />

explicit expressions <strong>for</strong> the imaginary parts of π T,L (ω, k) were derived<br />

by Altherr, Petitgirard, and del Río Gaztelurrutia (1993).<br />

The general expressions Eq. (6.38) <strong>for</strong> the real parts of π L and<br />

π T were derived without the need to <strong>as</strong>sume that K w<strong>as</strong> time-like.<br />

There<strong>for</strong>e, they should also apply “below the light cone,” even though<br />

Braaten and Segel (1993) confined their discussion to the region k < ω.<br />

As expected, these expressions break down <strong>for</strong> k > ω/v ∗ where Landau<br />

damping becomes strong.<br />

6.3.6 Renormalization Constants Z T,L<br />

Armed with the dispersion relation one may determine the vertex renormalization<br />

constants Z T,L relevant <strong>for</strong> the coupling of external photons<br />

or pl<strong>as</strong>mons to an electron in the medium (Sect. 6.2.3),<br />

ZT,L −1 = 1 − ∂π ∣<br />

T,L(ω, k) ∣∣∣∣ω<br />

. (6.51)<br />

∂ω 2 2 −k 2 =π T,L (ω,k)<br />

With the same approximations <strong>as</strong> be<strong>for</strong>e, Braaten and Segel (1993)<br />

found an analytic representation accurate to O(α),<br />

Z T =<br />

Z L =<br />

2ω 2 (ω 2 − v 2 ∗k 2 )<br />

ω 2 [3ω 2 P − 2 (ω 2 − k 2 )] + (ω 2 + k 2 )(ω 2 − v 2 ∗k 2 ) ,<br />

2 (ω 2 − v 2 ∗k 2 )<br />

3ω 2 P − (ω 2 − v 2 ∗k 2 )<br />

ω 2<br />

ω 2 − k 2 . (6.52)<br />

In each c<strong>as</strong>e ω and k are “on shell,” i.e. they are related by the dispersion<br />

relation relevant <strong>for</strong> the T and L c<strong>as</strong>e, respectively.<br />

Inspection of Eq. (6.52) reveals that Z T is always very close to unity,<br />

<strong>as</strong> expected <strong>for</strong> excitations with only a small deviation from a m<strong>as</strong>siveparticle<br />

dispersion relation. The contours in Fig. 6.7 confirm that Z T<br />

never deviates from unity by more than a few percent.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!