Physics for Scientists and Engineers: A Strategic Approach with Modern Physics (3rd Edition)

Published by Pearson
ISBN 10: 0321740904
ISBN 13: 978-0-32174-090-8

Chapter 42 - Nuclear Physics - Exercises and Problems - Page 1275: 49

Answer

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Work Step by Step

$$\color{blue}{\bf [a]}$$ We need to calculate the Time to Boil the Water. So we need to find the Energy Released Per Decay. The decay of $ ^{223}\text{Ra} $ releases energy when it emits an alpha particle and transforms into $ ^{219}\text{Rn} $. We know that $$E_{\rm released}=\Delta mc^2$$ where $ c^2 = 931.49 \, \text{MeV}/\text{u} $, and the mass difference is given by $\Delta m=m_{( ^{223}\text{Ra})} - m_{(^{219}\text{Rn})} - m_{(^4\text{He}) }$; $$ E_{\rm released} = \left[ m_{( ^{223}\text{Ra})} - m_{(^{219}\text{Rn})} - m_{(^4\text{He}) }\right] (931.49 ) $$ Substituting the known: $$ E_{\rm released} = [223.018499 - 219.009477 - 4.002602 ](931.49 ) $$ $$ E_{\rm released} =\bf 5.98 \; \rm {MeV} =\bf 9.581 \times 10^{-13} \rm \; J\tag 1 $$ This means that each alpha decay process, it releases $ 9.581 \times 10^{-13} \, \text{J} $. Now we need to calculate the Energy Needed to Heat the 100 mL (or 0.1 kg where $m=\rho /V$) of water from 18$^\circ$C to 100$^\circ$C. So, $$ Q = mc\Delta T $$ Substituting the known: $$ Q = (0.1 ) (4190 ) (100 - 18) =\bf 34400 \rm \, {J}\tag 2 $$ Now we need to calculate the Number of Decays Needed to provide a $ 34,400 \, \text{J} $ of energy. $$ N_\text{decays} = \frac{Q}{E_{\rm released}} $$ Plug from (1) and (2); $$ N_\text{decay} = \frac{34400 }{9.581 \times 10^{-13} }=\bf 3.59 \times 10^{16}\;\rm decay $$ Now we need to find the Initial Number of $ ^{223}\text{Ra} $ atoms. We know that the molar mass of $ ^{223}\text{Ra} $ is 223 g/mol, so for 1.0 g: $$ N_0 =\dfrac{m_{\rm sample}}{M}N_A$$ where $N_A$ is Avogadro's number. Plug the known; $$N_0= \frac{1.0 \, \text{g}}{223 \, \text{g/mol}} ( 6.022 \times 10^{23} \, \text{atoms/mol}) $$ $$ N_0 =\bf 2.70 \times 10^{21} \, \rm {atoms} $$ Now we need to find the Time Required for $ 3.59 \times 10^{16} $ Decays, where the decay rate is given by: $$ \frac{dN}{dt} = -rN $$ where $ r = \dfrac{\ln(2)}{t_{1/2}} $ $$\frac{dN}{dt} = -\dfrac{\ln(2)}{t_{1/2}}N $$ Replacing $dN/dt$ by $\Delta N/\Delta t$, and solving for $\Delta t$ $$ \Delta t= \frac{\Delta N}{ -\dfrac{\ln(2)}{t_{1/2}}N } $$ $$ \Delta t=\dfrac{-t_{1/2}}{\ln(2)} \frac{\Delta N}{ N } $$ where $N=N_0$, and $\Delta N=- N_{\rm decay}$ $$ \Delta t=\dfrac{-t_{1/2}}{\ln(2)} \frac{ N_{\rm decay}}{ N_0 } $$ Plug the known; $$ \Delta t=\dfrac{-(11.43\times 24\times 3600)}{\ln(2)}\cdot \frac{-(3.59 \times 10^{16})}{( 2.70 \times 10^{21}) } $$ $$ \Delta t= \color{red}{\bf 18.94}\;\rm s $$ $$\color{blue}{\bf [b]}$$ Alpha particles can ionize water molecules, potentially splitting $ \text{H}_2\text{O} $ into $ \text{H}_2 $ and $ \text{O}_2 $ gases, causing bubbles. However, the water's chemistry remains largely unchanged.
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