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Energy and Human Ambitions on a Finite Planet, 2021a

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15 Nuclear <str<strong>on</strong>g>Energy</str<strong>on</strong>g> 247<br />

to 1.8 × 10 −9 J of energy. Since 1 MeV is 1.6 × 10 −13 J, we end up with<br />

11,200 MeV corresp<strong>on</strong>ding to 12 a.m.u. (1 a.m.u. is 931.5 MeV).<br />

In practice, <str<strong>on</strong>g>and</str<strong>on</strong>g> perhaps surprisingly, atoms (nuclei) weigh less than<br />

the sum of their parts due to binding energy. In order to rip a nucleus<br />

completely apart <str<strong>on</strong>g>and</str<strong>on</strong>g> move all the nucle<strong>on</strong>s far from each other, energy<br />

must be put in (left part of Figure 15.9). And any change in energy is<br />

accompanied by a change in mass, via ΔE Δmc 2 . All the energy that<br />

must be injected to completely dismantle the nucleus weighs something!<br />

So the mass of the individual pieces after dismantling the nucleus is<br />

effectively the mass of the original nucleus plus the mass-equivalent of<br />

all the energy that was put in to tear it apart (middle panel of Figure<br />

15.9). Therefore, binding energy effectively reduces the mass of a nucleus,<br />

which we will now explore quantitatively.<br />

+ <str<strong>on</strong>g>Energy</str<strong>on</strong>g><br />

+ <str<strong>on</strong>g>Energy</str<strong>on</strong>g><br />

<str<strong>on</strong>g>Energy</str<strong>on</strong>g><br />

Figure 15.9: One must add energy to overcome<br />

nuclear binding energy in order to<br />

bust up a nucleus into its c<strong>on</strong>stituent nucle<strong>on</strong>s<br />

(left). Thus, the collective mass of<br />

a nucleus plus the mass associated with<br />

the energy it takes to break it apart (via<br />

E mc 2 ) must be equal to the sum of the<br />

masses of the c<strong>on</strong>stituent parts (middle).<br />

Therefore, if we compare the mass of the<br />

nucleus al<strong>on</strong>e (removing the energy’s mass<br />

from the scale) it must be less than the mass<br />

of the loose collecti<strong>on</strong> of nucle<strong>on</strong>s (right).<br />

A careful look at Figure 15.4 reveals that lighter stable nuclei (graysquares)<br />

at the lower left of the chart have a mass a little larger than the<br />

corresp<strong>on</strong>ding mass number, but by the upper right—around oxygen—<br />

the mass has edged just lower than A. Table 15.3 shows this trend,<br />

c<strong>on</strong>firmable in Figure 15.4 for the first four nuclides in the table. The<br />

difference between mass <str<strong>on</strong>g>and</str<strong>on</strong>g> A is most negative around ir<strong>on</strong>, then turns<br />

around <str<strong>on</strong>g>and</str<strong>on</strong>g> becomes positive again for heavy elements like uranium.<br />

What is going <strong>on</strong> here? If the mass of a nucleus were just the sum of its<br />

parts, we would expect the total mass to just track linearly as we add<br />

more pieces. In fact, if we try to build a neutral carb<strong>on</strong> atom out of 6<br />

prot<strong>on</strong>s, 6 neutr<strong>on</strong>s, <str<strong>on</strong>g>and</str<strong>on</strong>g> 6 electr<strong>on</strong>s, the sum, according to Table 15.4,<br />

should be 12.099 a.m.u., not 12.000. The discrepancy is due to nuclear<br />

binding energy, as was introduced in Figure 15.9.<br />

Particle a.m.u. 10 −27 kg MeV/c 2<br />

prot<strong>on</strong> 1.0072765 1.6726219 938.2720882<br />

neutr<strong>on</strong> 1.0086649 1.6749275 939.5654205<br />

electr<strong>on</strong> 0.00054858 0.000911 0.510999<br />

(a.m.u.) 1.0000000 1.660539 931.494102<br />

Table 15.3: Example mass progressi<strong>on</strong>.<br />

Nuclide A mass (a.m.u.)<br />

2H<br />

2 2.014<br />

4He<br />

4 4.003<br />

12C<br />

12 12.000<br />

16O<br />

16 15.995<br />

56Fe<br />

56 55.935<br />

235U<br />

235 235.044<br />

Table 15.4: C<strong>on</strong>stituent masses of atomic<br />

building blocks, expressing the same basic<br />

thing in three comm<strong>on</strong> units systems.<br />

Nuclear binding energy is incredibly str<strong>on</strong>g 15 <str<strong>on</strong>g>and</str<strong>on</strong>g> is able to overpower<br />

the natural electric repulsi<strong>on</strong> between positively charged prot<strong>on</strong>s <str<strong>on</strong>g>and</str<strong>on</strong>g><br />

stick them together in an unwilling bunch. The str<strong>on</strong>g nuclear force<br />

15: . . . relating to what we call the str<strong>on</strong>g<br />

nuclear force<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.

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