Physics: Principles with Applications (7th Edition)

Published by Pearson
ISBN 10: 0-32162-592-7
ISBN 13: 978-0-32162-592-2

Chapter 33 - Astrophysics and Cosmology - General Problems - Page 983: 48

Answer

a. $1.6\times10^{17}K$. b. This is in the electroweak era.

Work Step by Step

a. Use the temperature–kinetic energy relationship $kT=KE$, from section 33–7. Find the temperature. $$T=\frac{KE}{k}=\frac{(14\times10^{12}eV)(1.60\times10^{-19}J/eV)}{1.38\times10^{-23}J/K}=1.6\times10^{17}K$$ This is extraordinarily hot. b. Looking at Figure 33–29, a temperature of $1.6\times10^{17}K$ is in the electroweak era.
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