Nuclear Fission Spring 2013 Lecture 16 1

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Nuclear Fission
Spring 2013
UCSD
Physics 12
Physics 12
UCSD
Spring 2013
UCSD
Spring 2013
Lecture 16
Physics 12
3
2
Physics 12
UCSD
Spring 2013
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Nuclear Fission
Spring 2013
Physics 12
UCSD
proton
Poof!
Physics 12
UCSD
electron
neutron
Spring 2013
UCSD
anti-neutrino
5
Physics 12
Spring 2013
Q
6
Physics 12
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A
Z
XN
12
€6 C6
14
6 C8
235
92 143
238
92 146
239
94
145
U
U
Pu
€
€
Spring 2013
Lecture 16
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Spring 2013
€
€
€
Q
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Nuclear Fission
Spring 2013
UCSD
Physics 12
Physics 12
UCSD
Chart of the Nuclides
β+
3
α
2
Z
β-
1
0
Spring 2013
UCSD
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Physics 12
Spring 2013
UCSD
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Physics 12
source: http://www.epa.gov/radiation/understand/calculate.html
1 mrem carries 0.000055% chance of developing cancer: 350 mrem/yr  expect cancer in 5000 years
Spring 2013
Lecture 16
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Spring 2013
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Nuclear Fission
Spring 2013
Physics 12
UCSD
Physics 12
UCSD
Barium and Krypton represent just one of many potential outcomes
Spring 2013
UCSD
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Physics 12
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Physics 12
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Bottom line: at thermal energies (arrow), 235U is 1000 times more likely
to undergo fission than 238U even when smacked hard
Spring 2013
Lecture 16
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Spring 2013
3×Q
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Nuclear Fission
Spring 2013
UCSD
Spring 2013
UCSD
Physics 12
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Physics 12
Physics 12
UCSD
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Physics 12
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•  Iron (Fe) is at the peak
•  On the heavy side of iron, fission delivers energy
•  On the lighter side of iron, fusion delivers energy
•  This is why normal stars stop fusion after iron
•  Huge energy step to be gained in going from
hydrogen (H) to helium-4 via fusion
Spring 2013
Lecture 16
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Nuclear Fission
Spring 2013
UCSD
Physics 12
Physics 12
UCSD
daughter nuclei from fission are neutron-rich, and β- decay toward black (stable) nuclei
some can fall outside of neutron “drip line” in white region (don’t have to be right on red line)
235U
daughter 1
daughter 2
Spring 2013
UCSD
Spring 2013
Lecture 16
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Physics 12
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Spring 2013
stable nuclide
radioactive (unstable) nuclide
Physics 12
UCSD
Spring 2013
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Q
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Nuclear Fission
Spring 2013
UCSD
Spring 2013
Lecture 16
Physics 12
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7
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