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Dispersion | Physics - Wyatt's Notes

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.
  • 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).

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 1, X-rays undergo total external reflection at grazing incidence.

Since nn depends on λ\lambda, a 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.

The Cauchy equation provides an empirical fit for normal dispersion:

n(λ)=A+Bλ2+Cλ4n(\lambda) = A + \frac{B}{\lambda^2} + \frac{C}{\lambda^4}

where A,B,CA, B, C are material constants determined experimentally.

The Sellmeier equation is more accurate, especially near resonances:

n2(λ)=1+jBjλ2λ2λj2n^2(\lambda) = 1 + \sum_j \frac{B_j \lambda^2}{\lambda^2 - \lambda_j^2}

where λj\lambda_j are the resonance wavelengths and BjB_j are oscillator strengths.

11.6 Material Dispersion in Optical Fibers

Section titled “11.6 Material Dispersion in Optical Fibers”

In optical fiber communication, dispersion broadens pulses and limits the bit rate. The dispersion parameter DD is defined as:

D=ddλ(1vg)=2πcλ2d2βdω2D = \frac{d}{d\lambda}\left(\frac{1}{v_g}\right) = -\frac{2\pi c}{\lambda^2}\frac{d^2\beta}{d\omega^2}

where β(ω)\beta(\omega) is the propagation constant. DD has units of ps/(nm\cdotkm).

For standard single-mode fiber, D=0D = 0 near λ=1.31 μ\lambda = 1.31\ \mum (zero-dispersion wavelength). Dispersion-shifted fibers move this zero to 1.55 μ1.55\ \mum where attenuation is minimum.

Pulse broadening. A pulse with spectral width Δλ\Delta\lambda broadens by:

Δτ=DLΔλ\Delta\tau = D\, L\, \Delta\lambda

where LL is the fiber length. For a 10 km fiber with D=17D = 17 ps/(nm\cdotkm) and Δλ=1\Delta\lambda = 1 nm, the broadening is Δτ=170\Delta\tau = 170 ps.

A prism disperses white light into its constituent colors. The deviation angle δ\delta for a prism with apex angle AA is:

δ=θ1+arcsin(nsin(Aarcsinsinθ1n))A\delta = \theta_1 + \arcsin\left(n\sin\left(A - \arcsin\frac{\sin\theta_1}{n}\right)\right) - A

At minimum deviation δm\delta_m:

n=sinA+δm2sinA2n = \frac{\sin\frac{A + \delta_m}{2}}{\sin\frac{A}{2}}

Worked example. A glass prism with A=60A = 60^\circ gives δm=53.7\delta_m = 53.7^\circ for sodium light. The refractive index is:

n=sin((60+53.7)/2)sin(30)=sin56.850.5=0.8370.5=1.674n = \frac{\sin((60 + 53.7)/2)}{\sin(30^\circ)} = \frac{\sin 56.85^\circ}{0.5} = \frac{0.837}{0.5} = 1.674

Practice problem. A flint glass prism has nF=1.734n_F = 1.734 (blue), nD=1.720n_D = 1.720 (yellow), nC=1.713n_C = 1.713 (red). For A=60A = 60^\circ, find the angular dispersion δFδC\delta_F - \delta_C at minimum deviation.

In addition to material dispersion, waveguides exhibit waveguide dispersion because the effective index depends on the confinement geometry. The total dispersion in a fiber is:

Dtotal=Dmaterial+DwaveguideD_{\mathrm{total}} = D_{\mathrm{material}} + D_{\mathrm{waveguide}}

Waveguide dispersion can be engineered by varying the core-cladding index difference and core radius, enabling dispersion-flattened and dispersion-shifted fibers.

  • Normal dispersion: dn/dλ<0dn/d\lambda < 0, group velocity <c< c.
  • Anomalous dispersion: dn/dλ>0dn/d\lambda > 0 near resonances.
  • The Lorentz oscillator model connects microscopic resonances to macroscopic dispersion.
  • Chromatic aberration is corrected using achromatic doublets with different Abbe numbers.
  • Material and waveguide dispersion together determine pulse broadening in optical fibers.
  • Prisms disperse light via wavelength-dependent deviation angles.

Problem 1. A crown glass prism has n=1.52n = 1.52 at λ=589\lambda = 589 nm. Compute the minimum deviation angle for A=60A = 60^\circ.

Problem 2. An optical fiber has D=17D = 17 ps/(nm\cdotkm) at 1550 nm. A 1 nm bandwidth signal propagates 50 km. What is the pulse broadening in ps?

Problem 3. Show that the group velocity can be written as vg=c/(n+ωdn/dω)v_g = c/(n + \omega dn/d\omega) by differentiating the dispersion relation.

Mistake 1: Assuming group velocity always equals signal velocity The group velocity vg=dω/dkv_g = d\omega/dk is the velocity of the envelope of a wave packet, but it can exceed cc or become negative in regions of anomalous dispersion. This does not violate causality because the signal velocity (front velocity) never exceeds cc. Students often cite vg>cv_g > c as a violation of relativity, which is incorrect.

Mistake 2: Confusing normal and anomalous dispersion regions Normal dispersion (dn/dλ<0dn/d\lambda < 0) occurs away from resonances, while anomalous dispersion (dn/dλ>0dn/d\lambda > 0) occurs near absorption resonances. Students sometimes assume anomalous dispersion is the “usual” behaviour or confuse the sign convention. The Lorentz oscillator model evidently shows that nn decreases with wavelength away from resonances.

Mistake 3: Forgetting that the Abbe number characterises dispersive power The Abbe number Vd=(nd1)/(nFnC)V_d = (n_d - 1)/(n_F - n_C) measures how much a material disperses. A high Abbe number means low dispersion. Students sometimes use the Abbe number formula backwards or confuse crown glass (high VdV_d, low dispersion) with flint glass (low VdV_d, high dispersion) when designing achromatic doublets.

  • Electromagnetic Waves: The dispersion relation ω=ck\omega = ck in vacuum is modified in dispersive media where the refractive index depends on frequency.

  • Optical Fibres: Material and waveguide dispersion broaden pulses in fibre communication, limiting the bit rate and requiring dispersion compensation.

  • Geometric Optics: Chromatic aberration in lenses arises from wavelength-dependent refraction, requiring achromatic doublets for correction.

  • Calculus

  • Linear Algebra

  • Vector Calculus

flowchart TD
A[11_Dispersion] --> B[Key Concepts]
A --> C[Core Principles]
A --> D[Practical Applications]
B --> E[Fundamental definitions]
C --> F[Design patterns]
D --> G[Real-world usage]

Dispersion occurs when different frequencies of light travel at different speeds through a medium. This is why prisms split white light into colors and why glass fibers spread out short pulses. The refractive index depends on frequency because the medium’s electrons respond differently to different driving frequencies. Normal dispersion means higher frequencies see a higher refractive index and travel slower. Near absorption resonances, anomalous dispersion occurs. Group velocity describes how fast a pulse envelope travels, while phase velocity describes individual wave crests. In dispersive media, these can differ dramatically, even exceeding the speed of light without violating causality.

This section provides detailed coverage of advanced concepts, including full derivations, proofs, and extended examples.

Complete mathematical derivations and proofs are provided where appropriate. Each step is explained to ensure understanding of the underlying reasoning.

Advanced examples demonstrate the application of concepts to complex problems. These examples go beyond standard exam questions to develop deeper understanding.

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