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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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198 Chapter 6<br />

only refers to scattering in the <strong>for</strong>ward direction, but that all properties<br />

of the wave and the scatterer are left unchanged. If the medium particles<br />

have a distribution of momenta, spins, etc. the <strong>for</strong>ward scattering<br />

amplitude must be averaged over those quantities, and different species<br />

of medium particles must be summed over.<br />

For a practical calculation it helps to recall that dσ/dΩ = |f(θ)| 2<br />

so that |f 0 | is the square root of the <strong>for</strong>ward differential cross section.<br />

For example, the Thomson cross section <strong>for</strong> photons interacting with<br />

nonrelativistic electrons is dσ/dΩ = (α/m e ) 2 |ϵ · ϵ ′ | 2 with the polarization<br />

vectors ϵ and ϵ ′ of the initial- and final-state photon. Forward<br />

scattering implies |ϵ · ϵ ′ | 2 = 1 so that |f 0 | = α/m e . The dispersion relation<br />

is then ω 2 = k 2 + ωP 2 with the pl<strong>as</strong>ma frequency ωP 2 = 4πα n e /m e .<br />

Of course, the absolute sign of f 0 h<strong>as</strong> to be derived from some other<br />

in<strong>for</strong>mation—<strong>for</strong> photon dispersion see Sect. 6.3.<br />

The <strong>for</strong>ward scattering amplitude and the refractive index are generally<br />

complex numbers. Physically it is evident that in a medium the<br />

intensity of a beam is depleted <strong>as</strong> e −z/l . The mean free path is given by<br />

l −1 = σnv where σ is the total scattering cross section, n is the number<br />

density of scatterers, and v is the velocity of propagation. Thus the<br />

amplitude of a plane wave varies <strong>as</strong> e ikz−z/2l . Moreover, the derivation<br />

of the refractive index indicates that the amplitude varies according to<br />

e inrefrωz , yielding k = Re n refr ω and (2l) −1 = Im n refr ω. For relativistic<br />

propagation (v = 1) the l<strong>as</strong>t equation implies σ(ω) = (4π/ω) Im f 0 (ω),<br />

a relationship known <strong>as</strong> the optical theorem.<br />

For the applications discussed in this book specific interaction models<br />

between the propagating particles and the medium will be <strong>as</strong>sumed<br />

so that it is usually straight<strong>for</strong>ward to calculate the dispersion relation<br />

according to Eq. (6.5). One should keep in mind, however, that n refr <strong>as</strong><br />

a function of ω h<strong>as</strong> a number of general properties, independently of the<br />

interaction model. For example, its real and imaginary part are connected<br />

by the Kramers-Kronig relations (Sakurai 1967; Jackson 1975).<br />

6.2.2 Particle Momentum and Velocity<br />

The four-vector (ω, k) which governs the spatial and temporal behavior<br />

of a plane wave can be time-like (ω 2 − k 2 > 0) <strong>as</strong> <strong>for</strong> m<strong>as</strong>sive particles<br />

in vacuum, it can be light-like (ω 2 − k 2 = 0) <strong>as</strong> <strong>for</strong> photons in vacuum,<br />

or it can be space-like (ω 2 − k 2 < 0) <strong>as</strong> <strong>for</strong> visible light in water or air.<br />

Because the quantized excitations of such field modes are interpreted<br />

<strong>as</strong> particles, E = ¯hω is the particle’s energy. (I have temporarily restored<br />

¯h even though it is 1 in natural units.) Similarly one may be

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