The Cosmic Background Radiation — Question 3

Section 44-11 · Physics pages 7496–7497

Question 3 Radiation energy density carries four powers of temperature Use u = aRT 4 with aR = 7.566 × 10−16 J m−3 K−4 and T=2.725 K. Let c=3.00 × 108 m/s. a larger a Schematic; labels, not drawing lengths, specify the data. (a) Find energy density and equivalent mass density u/c squared. (b) At z=9 find the energy-density ratio and explain its four expansion factors.
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Question 3 - Solution Radiation energy density carries four powers of temperature a larger a (a) Method and calculation u = 7.566 × 10−16(2.725)4 ≃4.17 × 10−14 J/m3 . ργ = u/c2 ≃4.64 × 10−31 kg/m3 . (b) Interpretation and further calculation u(z = 9)/u0 = (1 + 9)4 = 104 . u = nγ⟨E⟩, nγ ∝a−3, ⟨E⟩∝a−1. Physical check Radiation loses an additional energy factor compared with nonrelativistic rest-mass density.

Question 3

Radiation energy density carries four powers of temperature

Use u=aRT4u=a_RT^4 with aR=7.566×10−16a_R=7.566\times10^{-16} J m−3^{-3} K−4^{-4} and T=2.725 K. Let c=3.00×1083.00\times10^8 m/s.

Diagram shown in the original SVG worksheet.

  1. Find energy density and equivalent mass density u/c squared.

  2. At z=9 find the energy-density ratio and explain its four expansion factors.

Question 3 - Solution

Radiation energy density carries four powers of temperature

Diagram shown in the original SVG worksheet.

(a) Method and calculation

u=7.566×10−16(2.725)4≃4.17×10−14J/m3.\boxed{u=7.566\times10^{-16}(2.725)^4\simeq4.17\times10^{-14}\ {\mathrm{J/m^3}}}.ργ=u/c2≃4.64×10−31kg/m3.\boxed{\rho_\gamma=u/c^2\simeq4.64\times10^{-31}\ {\mathrm{kg/m^3}}}.

(b) Interpretation and further calculation

u(z=9)/u0=(1+9)4=104.\boxed{u(z=9)/u_0=(1+9)^4=10^4}.u=nγ⟨E⟩,nγ∝a−3,⟨E⟩∝a−1.u=n_\gamma\langle E\rangle,\quad n_\gamma\propto a^{-3},\quad\langle E\rangle\propto a^{-1}.

Physical check

Radiation loses an additional energy factor compared with nonrelativistic rest-mass density.