The Big Bang — Question 1

Section 44-13 · Physics pages 7532–7533

Question 1 A radiation-era clock links temperature to cosmic age In a supplied radiation-dominated model with constant relativistic degrees of freedom, t = 1.0 s (1 MeV/kBT)2 and a ∝t1/2. t T Schematic; labels, not drawing lengths, specify the data. (a) Find the ages when thermal energy kT is 2.0 MeV and .10 MeV. (b) Find the scale-factor and temperature ratios between those epochs and verify entropy-free cooling.
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Question 1 - Solution A radiation-era clock links temperature to cosmic age t T (a) Method and calculation t2 = 1/22 = .25 s . t.10 = 1/(.10)2 = 100 s . (b) Interpretation and further calculation a2/a1 = √ 100/.25 = 20 . T2/T1 = .10/2 = .05 = 1/20, aT = constant . Physical check The normalization and constant-degree assumption are supplied approximations. Particle thresholds can change the temperature-time relation.

Question 1

A radiation-era clock links temperature to cosmic age

In a supplied radiation-dominated model with constant relativistic degrees of freedom, t=1.0s(1MeV/kBT)2t=1.0\ {\mathrm{s}}\,(1\ {\mathrm{MeV}}/k_BT)^2 and a∝t1/2a\propto t^{1/2}.

Diagram shown in the original SVG worksheet.

  1. Find the ages when thermal energy kT is 2.0 MeV and .10 MeV.

  2. Find the scale-factor and temperature ratios between those epochs and verify entropy-free cooling.

Question 1 - Solution

A radiation-era clock links temperature to cosmic age

Diagram shown in the original SVG worksheet.

(a) Method and calculation

t2=1/22=.25s.\boxed{t_{2}=1/2^2=.25\ {\mathrm{s}}}.t.10=1/(.10)2=100s.\boxed{t_{.10}=1/(.10)^2=100\ {\mathrm{s}}}.

(b) Interpretation and further calculation

a2/a1=100/.25=20.\boxed{a_2/a_1=\sqrt{100/.25}=20}.T2/T1=.10/2=.05=1/20,aT=constant.\boxed{T_2/T_1=.10/2=.05=1/20,\quad aT=\text{constant}}.

Physical check

The normalization and constant-degree assumption are supplied approximations. Particle thresholds can change the temperature-time relation.