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Nuclear Chemistry III. Fission & Fusion (Nuclear reactions that are NOT radioactive decay.) III. Fission & Fusion (Nuclear reactions that are NOT radioactive decay.)
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A. F ission Splitting a large (heavy) nucleus into two or more smaller nuclei. Neutrons are always involved! Neutron bombardment causes fission. (Fission = splitting) Neutrons are also products of fission. 1 g of fission fuel = 3 tons of coal
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A. F ission Chain Reaction = self-propagating fission rxn Propagated by 1 n Free neutrons cause fission Each fission makes more Which sets off more fission! Making more Repeat ad infinitum!
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A. F ission Critical Mass = minimum mass required to sustain a chain reaction Chain reaction requires a certain “concentration” of fission fuel nearby. Otherwise the neutrons don’t get enough chances to keep things going.
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B. Fusion Joining two small (light) nuclei into one larger nucleus. Parent nuclides collide at extremely high velocity Forming one daughter nuclide with greater mass. Neutrons are usually released to stabilize the daughter nuclide. Ejecting neutrons corrects the p:n ratio.
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B. Fusion Thermonuclear: A temperature of 40,000,000 K is needed to sustain hydrogen fusion! At normal temperatures the two parent atoms would just make a chemical bond. (Their nuclei would never interact at all.) Fusion is even more energy efficient than fission: 1 g of fusion fuel = 20 tons of coal
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B. Fusion Fusion occurs naturally in stars. Our sun is fusing hydrogen into helium right now–fusion reactions generate the heat and light of stars. Supergiant stars fuse even larger nuclei After fusing H into He, the He is fused, then successive elements. All atoms other than 1 H were created by fusion in a supergiant star.
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C. Johannesson C. Fission vs. Fusion 235 U is limited danger of meltdown toxic waste thermal pollution fuel is abundant no danger of meltdown no toxic waste not yet sustainable FISSIONFISSION FUSIONFUSION
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Which reaction type? Less Energy More Energy
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