01.08.2021 Views

Energy and Human Ambitions on a Finite Planet, 2021a

Energy and Human Ambitions on a Finite Planet, 2021a

Energy and Human Ambitions on a Finite Planet, 2021a

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

15 Nuclear <str<strong>on</strong>g>Energy</str<strong>on</strong>g> 270<br />

56<br />

3. How many neutr<strong>on</strong>s does the isotope Fe c<strong>on</strong>tain?<br />

12 13<br />

4. Use the informati<strong>on</strong> in the boxes for C <str<strong>on</strong>g>and</str<strong>on</strong>g> C in Figure 15.4<br />

to determine the weighted composite mass of a natural blend of<br />

carb<strong>on</strong>—showing work—<str<strong>on</strong>g>and</str<strong>on</strong>g> compare this to the number in the<br />

left-most box for carb<strong>on</strong> in the same figure.<br />

5. In Figure 15.4, what are the <strong>on</strong>ly mass numbers, A, for which no<br />

stable nuclei exist?<br />

6. What are the <strong>on</strong>ly three l<strong>on</strong>g-lived radioactive isotopes in the<br />

porti<strong>on</strong> of the Chart of the Nuclides appearing in Figure 15.4, <str<strong>on</strong>g>and</str<strong>on</strong>g><br />

which <strong>on</strong>e lives the l<strong>on</strong>gest (how l<strong>on</strong>g)?<br />

7. Cosmic rays impinging <strong>on</strong> our atmosphere generate radioactive<br />

14<br />

C from<br />

14 N nuclei. 78 14<br />

These C atoms so<strong>on</strong> team up with oxygen 78: Nitrogen is the principal c<strong>on</strong>stituent in<br />

to form CO 2 , so that plants absorbing CO 2 from the air will have Earth’s atmosphere.<br />

about <strong>on</strong>e in a trilli<strong>on</strong> of their carb<strong>on</strong> atoms in this form. Animals<br />

eating these plants 79 will also have this fracti<strong>on</strong> of carb<strong>on</strong> in their 79: . . . <str<strong>on</strong>g>and</str<strong>on</strong>g>/or eating the animals that eat<br />

bodies, until they die <str<strong>on</strong>g>and</str<strong>on</strong>g> stop cycling carb<strong>on</strong> into their bodies. At these plants<br />

14<br />

this point, the fracti<strong>on</strong> of carb<strong>on</strong> atoms in the form of C in the The wording is l<strong>on</strong>g because without c<strong>on</strong>text,<br />

it’s just math. The real learning is in<br />

body declines, with a half life of 5,715 years. If you dig up a human<br />

skull, <str<strong>on</strong>g>and</str<strong>on</strong>g> discover that <strong>on</strong>ly <strong>on</strong>e-eighth of the usual <strong>on</strong>e-trilli<strong>on</strong>th<br />

the applicati<strong>on</strong> of math to the world.<br />

14<br />

of carb<strong>on</strong> atoms are C, how old do you deem the skull to be?<br />

8. If a friend creates a nucleus whose half-life is 4 hours <str<strong>on</strong>g>and</str<strong>on</strong>g> gives it<br />

to you at no<strong>on</strong>, what is the probability that it will not have decayed<br />

by no<strong>on</strong> the following day?<br />

235 238<br />

9. In close analog to the half-lives of U <str<strong>on</strong>g>and</str<strong>on</strong>g> U, let’s say two<br />

elements have half lives of 4.5 billi<strong>on</strong> years <str<strong>on</strong>g>and</str<strong>on</strong>g> 750 milli<strong>on</strong> years. 80<br />

If we start out having the same number of each (1:1 ratio), what<br />

will the ratio be after 4.5 billi<strong>on</strong> years? Express as x:1, where x is<br />

the larger of the two.<br />

10. C<strong>on</strong>trol rods in nuclear reactors tend to c<strong>on</strong>tain 10 B, which has<br />

a high neutr<strong>on</strong> absorpti<strong>on</strong> cross secti<strong>on</strong>. 81 What happens to this<br />

nucleus when it absorbs a neutr<strong>on</strong>, <str<strong>on</strong>g>and</str<strong>on</strong>g> is the result stable? If not,<br />

track the decay chain until it l<str<strong>on</strong>g>and</str<strong>on</strong>g>s <strong>on</strong> a stable nucleus.<br />

80: ...afactorof6different<br />

81: ...asindicated by the orange lower-half<br />

of the corresp<strong>on</strong>ding box in Figure 15.4<br />

14<br />

11. If some<strong>on</strong>e managed to create a B nucleus, what would its fate<br />

be? Track the decay chain <strong>on</strong> Figure 15.4—indicating the type of<br />

decay at each step—until it reaches stability, <str<strong>on</strong>g>and</str<strong>on</strong>g> indicate how<br />

l<strong>on</strong>g each step is likely to take.<br />

12. A particular nuclide is found to have lost 3 neutr<strong>on</strong>s <str<strong>on</strong>g>and</str<strong>on</strong>g> 1 prot<strong>on</strong><br />

after a decay chain. What combinati<strong>on</strong> of α <str<strong>on</strong>g>and</str<strong>on</strong>g> β decays could<br />

account for this result?<br />

13. How would you qualitatively describe the overall sense from<br />

Figure 15.8 in terms of where 82 <strong>on</strong> the chart <strong>on</strong>e is likely to see α<br />

82: Regi<strong>on</strong> descripti<strong>on</strong>s can include references<br />

to the mass range (e.g., low mass<br />

or high mass), above or below the stable<br />

elements (prot<strong>on</strong>-rich or neutr<strong>on</strong>-rich).<br />

© 2021 T. W. Murphy, Jr.; Creative Comm<strong>on</strong>s Attributi<strong>on</strong>-N<strong>on</strong>Commercial 4.0 Internati<strong>on</strong>al Lic.;<br />

Freely available at: https://escholarship.org/uc/energy_ambiti<strong>on</strong>s.

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!