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Dispersion

11.1 Normal and Anomalous Dispersion

The refractive index varies with frequency:

n(ω)=1+Ne22meε0jfjω0j2ω2iγjωn(\omega) = 1 + \frac{Ne^2}{2m_e\varepsilon_0} \sum_j \frac{f_j}{\omega_{0j}^2 - \omega^2 - i\gamma_j\omega}

Where NN is the electron density, fjf_j are oscillator strengths, ω0j\omega_{0j} are resonance Frequencies, and γj\gamma_j are damping constants.

  • Normal dispersion (dn/dλ<0dn/d\lambda \lt 0): away from resonances, nn decreases with increasing λ\lambda.
  • Anomalous dispersion (dn/dλ>0dn/d\lambda \gt 0): near resonances, nn increases with λ\lambda.

11.2 Group and Phase Velocity

  • Phase velocity: vp=ω/k=c/nv_p = \omega/k = c/n.
  • Group velocity: vg=dω/dk=c/(n+ωdn/dω)v_g = d\omega/dk = c/(n + \omega\, dn/d\omega).

For normal dispersion, vg<vpv_g \lt v_p. In regions of anomalous dispersion, vgv_g can exceed cc or Even become negative, but this does not violate causality (signal velocity remains c\leq c).

11.3 Dispersion Relation in a Medium

Starting from the Lorentz oscillator model for a single resonance:

n2(ω)=1+Ne2meε01ω02ω2iγωn^2(\omega) = 1 + \frac{Ne^2}{m_e\varepsilon_0}\frac{1}{\omega_0^2 - \omega^2 - i\gamma\omega}

The real part n(ω)=Reϵ(ω)n(\omega) = \mathrm{Re}\sqrt{\epsilon(\omega)} gives the refractive index. The Imaginary part gives absorption:

αabs=2ωcImn(ω)\alpha_{\mathrm{abs} = \frac{2\omega}{c}\,\mathrm{Im}\, n(\omega)}

Worked example. For X-rays (ωω0\omega \gg \omega_0):

n1Ne22meε0ω2=1ωp22ω2n \approx 1 - \frac{Ne^2}{2m_e\varepsilon_0\omega^2} = 1 - \frac{\omega_p^2}{2\omega^2}

Where ωp=Ne2/(meε0)\omega_p = \sqrt{Ne^2/(m_e\varepsilon_0)} is the plasma frequency. Since n<1n \lt 1X-rays Undergo total external reflection at grazing incidence.

11.4 Chromatic Aberration

Since nn depends on λ\lambdaA lens has different focal lengths for different wavelengths. The Longitudinal chromatic aberration is:

Δf=f(λ1)f(λ2)\Delta f = f(\lambda_1) - f(\lambda_2)

Achromatic doublet. Two lenses of different materials (e.g., crown and flint glass) with Different dispersive powers are combined to cancel chromatic aberration at two wavelengths. The Condition is:

ω1f1+ω2f2=0\frac{\omega_1}{f_1} + \frac{\omega_2}{f_2} = 0

Where ωi=(ni,Fni,C)/(ni,d1)\omega_i = (n_{i,F} - n_{i,C})/(n_{i,d} - 1) is the Abbe number for glass ii.