Physics: Principles with Applications (7th Edition)

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

Chapter 31 - Nuclear Energy; Effects and Uses of Radiation - Problems - Page 911: 24

Answer

25 collisions.

Work Step by Step

With each collision, one-half of the kinetic energy is lost. In that case, we can find the energy after N collisions. $$E_N=E_0\left(\frac{1}{2} \right)^N$$ Use the given information. $$0.040eV=(1.0\times10^6 eV)\left(\frac{1}{2} \right)^N$$ $$\frac{0.040eV}{1.0\times10^6 eV}=\left(\frac{1}{2} \right)^N$$ $$N=\frac{ln\frac{0.040eV }{1.0\times10^6 eV }}{ln\frac{1}{2}}=24.58$$ We round up to 25 colliisons.
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