A Summing Up — Question 7

Section 44-14 · Physics pages 7564–7565

Question 7 Photon scattering determines when radiation can travel freely At a trial epoch use electron density ne = 3.0 × 108 m−3, Thomson cross section 6.65 × 10−29 m2, c=3.00 × 108 m/s and H=4.0 × 10−14 s−1. many scatterings to free propagation Schematic; labels, not drawing lengths, specify the data. (a) Find photon scattering rate and Gamma/H. (b) If recombination reduces the free-electron fraction to .001 with other quantities fixed, find the new rate ratio and mean free path.
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Question 7 - Solution Photon scattering determines when radiation can travel freely many scatterings to free propagation (a) Method and calculation Γ = neσT c = 5.985 × 10−12 s−1 . Γ/H = 149.625 . (b) Interpretation and further calculation (Γ/H)after = .001(149.625) = .149625 . λafter = (.001neσT )−1 ≃5.01 × 1022 m . Physical check The rate comparison is local. Last-scattering probabilities require optical depth integrated along the photon trajectory through the changing ionization history.

Question 7

Photon scattering determines when radiation can travel freely

At a trial epoch use electron density ne=3.0×108n_e=3.0\times10^8 m−3^{-3}, Thomson cross section 6.65×10−296.65\times10^{-29} m2^2, c=3.00×1083.00\times10^8 m/s and H=4.0×10−144.0\times10^{-14} s−1^{-1}.

Diagram shown in the original SVG worksheet.

  1. Find photon scattering rate and Gamma/H.

  2. If recombination reduces the free-electron fraction to .001 with other quantities fixed, find the new rate ratio and mean free path.

Question 7 - Solution

Photon scattering determines when radiation can travel freely

Diagram shown in the original SVG worksheet.

(a) Method and calculation

Γ=neσTc=5.985×10−12s−1.\boxed{\Gamma=n_e\sigma_Tc=5.985\times10^{-12}\ {\mathrm{s^{-1}}}}.Γ/H=149.625.\boxed{\Gamma/H=149.625}.

(b) Interpretation and further calculation

(Γ/H)after=.001(149.625)=.149625.\boxed{(\Gamma/H)_{\mathrm{after}}=.001(149.625)=.149625}.λafter=(.001neσT)−1≃5.01×1022m.\boxed{\lambda_{\mathrm{after}}=(.001n_e\sigma_T)^{-1}\simeq5.01\times10^{22}\ {\mathrm{m}}}.

Physical check

The rate comparison is local. Last-scattering probabilities require optical depth integrated along the photon trajectory through the changing ionization history.