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
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> 259<br />
<strong>on</strong>e of the three fissile nuclei, we can c<strong>on</strong>vert 43 238 239<br />
U into the fissile Pu<br />
the following way.<br />
238 239<br />
1. A U may absorb a w<str<strong>on</strong>g>and</str<strong>on</strong>g>ering neutr<strong>on</strong> to become U.<br />
239<br />
2. U, whose half life is 23.5 minutes, undergoes β − to become<br />
239Np<br />
in short order.<br />
239<br />
3. Np also undergoes β − with a half life of 2.4 days to become<br />
239<br />
fissile Pu.<br />
Figure 15.17 highlights this process in a simplified regi<strong>on</strong> of the Chart<br />
of the Nuclides, while Figure 15.18 shows complete details for the<br />
entire regi<strong>on</strong> around the fissile materials—the <strong>on</strong>es with red isotope<br />
names—which can be used to track the sequence outlined above.<br />
43: . . . called transmutati<strong>on</strong><br />
<br />
Pu239 Pu240 Pu241<br />
24.10 kyr 6.56 kyr 14.4 yr<br />
<br />
Np238 Np239<br />
2.117 d 2.355 d<br />
Np240<br />
1.032 h<br />
<br />
<br />
<br />
U237 U238 U239<br />
6.75 d 99.2745 23.47 m<br />
4.47 Gyr<br />
<br />
<br />
n<br />
Figure 15.17: Breeder route to<br />
239 Pu.<br />
95<br />
94<br />
93<br />
92<br />
91<br />
90<br />
89<br />
Am<br />
Americium<br />
Pu<br />
Plut<strong>on</strong>ium<br />
Np<br />
Neptunium<br />
U<br />
Uranium<br />
238.02891<br />
Pa<br />
Protactinium<br />
231.03588<br />
Th<br />
Thorium<br />
232.0381<br />
Ac<br />
Actinium<br />
Am235 Am236 Am237 Am238 Am239 Am240 Am241 Am242 Am243<br />
15 m 4 m<br />
1.22 h 1.63 h 11.9 h 2.12 d 432.7 yr 141 yr 7.37 kyr<br />
e - capture ? e - capture e - capture e - capture e - capture e - capture <br />
E 2.6 E 3.3<br />
E 1.5<br />
E 2.3 E 0.803 E 1.38 241.056823<br />
243.061373<br />
Pu234 Pu235 Pu236 Pu237 Pu238 Pu239 Pu240 Pu241 Pu242<br />
8.8 h 25.3 m 2.87 yr 45.2 d 87.7 yr 24.10 kyr 6.56 kyr 14.4 yr 375 kyr<br />
e - capture e - capture <br />
e - capture <br />
<br />
<br />
E 0.39 E 1.14 236.046048 E 0.22 238.049553 239.052157 240.053087 E 0.0208 242.058737<br />
Np233 Np234 Np235 Np236 Np237 Np238 Np239 Np240 Np241<br />
36.2 m 4.4 d 1.085 yr 155 kyr 2.14 Myr 2.117 d 2.355 d 1.032 h 13.9 m<br />
e - capture e - capture e - capture e - capture <br />
E 1.0 E 1.81 E 0.124 E 0.9 237.048167 E 1.292 E 0.722 E 2.20 E 1.3<br />
U232 U233 U234 U235 U236 U237 U238 U239 U240<br />
69.8 yr 159.2 kyr 0.0055 0.7200 23.42 Myr 6.75 d 99.2745 23.47 m 14.1 h<br />
<br />
<br />
246 kyr<br />
<br />
704 Myr<br />
<br />
<br />
4.47 Gyr<br />
<br />
<br />
232.037146 233.039628 234.040946 235.043923 236.045562 E 0.519 238.050783 E 1.263 E 0.39<br />
Pa231 Pa232 Pa233 Pa234 Pa235 Pa236 Pa237 Pa238<br />
32.8 kyr 1.31 d 26.967 d 6.69 h 24.4 m 9.1 m 8.1 m 2.3 m<br />
<br />
231.035879 E 1.34 E 0.570 E 2.195 E 1.4<br />
E 2.9<br />
E 2.3 E 3.5<br />
Th230 Th231 Th232 Th233 Th234 Th235 Th236 Th237 Th238<br />
75.4 kyr 1.063 d 100 21.83 m 24.10 d 7.2 m 37.5 m 4.8 m ~9.4 m<br />
14.0 Gyr<br />
<br />
<br />
<br />
<br />
<br />
230.033127 E 0.390 232.038050 E 1.245 E 0.273 E 1.9 E 1.0 E 2.6 E 1.6<br />
Ac229 Ac230 Ac231 Ac232 Ac233 Ac234 146 147 148<br />
1.04 h 2.03 m 7.5 m 2.0 m 2.4 m<br />
40s<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
E 1.10 E 2.7<br />
E 2.1<br />
E 3.7<br />
E 2.8 E 4.5<br />
Z N 140 141 142 143 144 145<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
<br />
Pu239<br />
24.10 kyr<br />
239.052157<br />
U238<br />
99.2745<br />
4.47 Gyr<br />
<br />
238.050783<br />
isotope<br />
half life (radioactive)<br />
primary decay path<br />
mass or decay energy (MeV)<br />
naturally ocurring isotope<br />
% abundance<br />
half life<br />
primary decay path<br />
mass, a.m.u.<br />
Top Half Coloring:<br />
Half Life Guide<br />
< 1 day<br />
1 to 10 days<br />
10 to 100 days<br />
100 days to 10 yr<br />
10 yr to 500 Myr<br />
> 500 Myr or stable<br />
Bottom Half Coloring:<br />
Neutr<strong>on</strong> Absorpti<strong>on</strong> (Barns)<br />
< 10<br />
10 to 100<br />
100 to 500<br />
500 to 1000<br />
>1000<br />
1 a.m.u. = 1.66054e-27 kg<br />
1 a.m.u. = 931.49432 MeV/c 2<br />
1 MeV = 1.6022e-13 J<br />
U233, U235, Pu239 are slow-neutr<strong>on</strong> fissile<br />
Figure 15.18: Chart of the Nuclides in the fissi<strong>on</strong> regi<strong>on</strong>. See also Figure 15.4 for the lower-left corner.<br />
238 239<br />
The result is that sterile U can be turned into fissile Pu that can be<br />
used in fissi<strong>on</strong> reactors. This process of transmuting an inert nucleus<br />
into a fissile <strong>on</strong>e is called breeding, <str<strong>on</strong>g>and</str<strong>on</strong>g> is how we get any plut<strong>on</strong>ium<br />
at all. 44<br />
238<br />
A nuclear reactor is a great place to introduce U to neutr<strong>on</strong>s:<br />
both are already in attendance. In fact, breeding happens as a matter of<br />
course in a nuclear reactor: it is estimated that <strong>on</strong>e-third of the fissi<strong>on</strong><br />
44: . . . e.g., for weap<strong>on</strong>s<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.