The Big Bang — Question 9

Section 44-13 · Physics pages 7548–7549

Question 9 The particle horizon is a history integral in a radiation universe Assume a(t) = At1/2 from t=0 and define proper particle horizon Dp(t) = a(t) ∫t 0 c dt′/a(t′). Dp causal horizon Schematic; labels, not drawing lengths, specify the data. (a) Evaluate the integral and compare with c times the cosmic age. (b) At t=100 s find Dp using c=3.00 × 108 m/s, and compare with the Hubble radius in this model.
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Question 9 - Solution The particle horizon is a history integral in a radiation universe Dp causal horizon (a) Method and calculation Dp = At1/2(c/A) ∫t 0 (t′)−1/2dt′. Dp = 2ct̸ = ct . (b) Interpretation and further calculation Dp(100 s) = 6.00 × 1010 m . H = 1/(2t) ⇒c/H = 2ct = Dp for this particular history . Physical check The equality of the Hubble radius and particle horizon here is model-specific. The integral assumes the power law extends back to zero.

Question 9

The particle horizon is a history integral in a radiation universe

Assume a(t)=At1/2a(t)=A t^{1/2} from t=0 and define proper particle horizon Dp(t)=a(t)∫0tcdt′/a(t′)D_p(t)=a(t)\int_0^t c\,dt^\prime/a(t^\prime).

Diagram shown in the original SVG worksheet.

  1. Evaluate the integral and compare with c times the cosmic age.

  2. At t=100 s find Dp using c=3.00×1083.00\times10^8 m/s, and compare with the Hubble radius in this model.

Question 9 - Solution

The particle horizon is a history integral in a radiation universe

Diagram shown in the original SVG worksheet.

(a) Method and calculation

Dp=At1/2(c/A)∫0t(t′)−1/2dt′.D_p=At^{1/2}(c/A)\int_0^t(t^\prime)^{-1/2}dt^\prime.Dp=2ct≠ct.\boxed{D_p=2ct\ne ct}.

(b) Interpretation and further calculation

Dp(100s)=6.00×1010m.\boxed{D_p(100\ {\mathrm{s}})=6.00\times10^{10}\ {\mathrm{m}}}.H=1/(2t)⇒c/H=2ct=Dpfor this particular history.H=1/(2t)\Rightarrow\boxed{c/H=2ct=D_p\ \text{for this particular history}}.

Physical check

The equality of the Hubble radius and particle horizon here is model-specific. The integral assumes the power law extends back to zero.