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 Q 4 1 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 UCSD 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 7 Spring 2013 € € € Q 8 2 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 9 Physics 12 Spring 2013 UCSD 10 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 11 Spring 2013 12 3 Nuclear Fission Spring 2013 Physics 12 UCSD Physics 12 UCSD Barium and Krypton represent just one of many potential outcomes Spring 2013 UCSD 13 Physics 12 Spring 2013 14 Physics 12 UCSD 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 15 Spring 2013 3×Q 16 4 Nuclear Fission Spring 2013 UCSD Spring 2013 UCSD Physics 12 17 Physics 12 Physics 12 UCSD Spring 2013 18 Physics 12 UCSD • 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 19 Spring 2013 20 5 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 21 Physics 12 23 Spring 2013 stable nuclide radioactive (unstable) nuclide Physics 12 UCSD Spring 2013 22 Q 24 6 Nuclear Fission Spring 2013 UCSD Spring 2013 Lecture 16 Physics 12 25 7