The Cosmic Background Radiation — Question 7

Section 44-11 · Physics pages 7504–7505

Question 7 The Rayleigh-Jeans approximation can be checked before calibrating a detector At frequency nu=30 GHz and T=2.725 K use x = hν/(kBT), with h/kB = 4.799 × 10−11 K s. The exact-to-Rayleigh-Jeans intensity ratio is x/(ex −1). ν Bν Schematic; labels, not drawing lengths, specify the data. (a) Find x and this intensity ratio. (b) Find the percentage by which the Rayleigh-Jeans prediction exceeds the exact Planck intensity.
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Question 7 - Solution The Rayleigh-Jeans approximation can be checked before calibrating a detector ν Bν (a) Method and calculation x = (4.799 × 10−11)(30 × 109)/2.725 = .528330 . BPlanck/BRJ = x/(ex −1) ≃.7590 . (b) Interpretation and further calculation BRJ −BPlanck BPlanck = ex −1 x −1. overestimate ≃31.8% . Physical check Low frequency must mean h nu much smaller than kT, not merely a frequency described informally as radio.

Question 7

The Rayleigh-Jeans approximation can be checked before calibrating a detector

At frequency nu=30 GHz and T=2.725 K use x=hν/(kBT)x=h\nu/(k_BT), with h/kB=4.799×10−11h/k_B=4.799\times10^{-11} K s. The exact-to-Rayleigh-Jeans intensity ratio is x/(ex−1)x/(e^x-1).

Diagram shown in the original SVG worksheet.

  1. Find x and this intensity ratio.

  2. Find the percentage by which the Rayleigh-Jeans prediction exceeds the exact Planck intensity.

Question 7 - Solution

The Rayleigh-Jeans approximation can be checked before calibrating a detector

Diagram shown in the original SVG worksheet.

(a) Method and calculation

x=(4.799×10−11)(30×109)/2.725=.528330.\boxed{x=(4.799\times10^{-11})(30\times10^9)/2.725=.528330}.BPlanck/BRJ=x/(ex−1)≃.7590.\boxed{B_{\mathrm{Planck}}/B_{\mathrm{RJ}}=x/(e^x-1)\simeq.7590}.

(b) Interpretation and further calculation

BRJ−BPlanckBPlanck=ex−1x−1.\frac{B_{\mathrm{RJ}}-B_{\mathrm{Planck}}}{B_{\mathrm{Planck}}}=\frac{e^x-1}{x}-1.overestimate≃31.8%.\boxed{\text{overestimate}\simeq31.8\%}.

Physical check

Low frequency must mean h nu much smaller than kT, not merely a frequency described informally as radio.