{"id":18305,"date":"2018-08-07T13:22:41","date_gmt":"2018-08-07T13:22:41","guid":{"rendered":"http:\/\/sitepourvtc.com\/?page_id=18305"},"modified":"2023-01-31T12:32:50","modified_gmt":"2023-01-31T12:32:50","slug":"nuclear-fission-vs-fusion","status":"publish","type":"page","link":"https:\/\/sitepourvtc.com\/nuclear-power\/fission\/nuclear-fission-vs-fusion\/","title":{"rendered":"Nuclear Fission vs Fusion"},"content":{"rendered":"
Nuclear fission<\/strong>\u00a0and nuclear fusion<\/strong> are different types of reactions that release energy (when exothermic) due to the formation of nuclei with higher nuclear binding energy<\/a>.<\/p>\n This is the main difference. Whether the reaction is exothermic or not depends on the binding energy of the resulting nuclei.<\/p>\n <\/a><\/p>\n Nuclear fission<\/strong>\u00a0is a\u00a0nuclear reaction<\/a>\u00a0in which the nucleus of an atom\u00a0splits<\/strong>\u00a0into smaller parts (lighter nuclei). The fission process often produces\u00a0free neutrons<\/a>\u00a0and\u00a0photons<\/a>\u00a0(in the form of\u00a0gamma rays<\/a>) and releases a large amount of energy<\/strong>. Nuclear fission is either a nuclear reaction\u00a0<\/strong>or a radioactive decay process <\/strong>in nuclear physics. The decay process is called spontaneous fission,<\/strong> and it is a very rare process. In reactor physics, neutron-induced nuclear fission<\/strong>\u00a0is the process of the greatest practical importance.<\/p>\n The total energy released<\/strong><\/a> in fission can be calculated from binding energies of the initial target nucleus to be fissioned and binding energies of\u00a0fission products<\/a>. But not all the total energy can be recovered in a reactor.<\/p>\n In nuclear physics,\u00a0nuclear fusion<\/strong> is a nuclear reaction in which two or more atomic nuclei collide at very high energy and fuse together into a new nucleus, e.g., helium. If light nuclei are forced together, they will fuse with a yield of energy because the mass of the combination will be less than the sum of the masses of the individual nuclei. Suppose the combined nuclear mass is less than that of iron at the peak of the\u00a0binding energy curve. In that case,<\/strong> the nuclear particles will be more tightly bound than they were in the lighter nuclei, and that decrease in mass comes off in the form of energy, according to the Albert Einstein relationship. For elements like uranium and thorium, fission will yield energy. Fusion reactions have an energy density many times greater than\u00a0nuclear fission<\/a>, and fusion reactions are millions of times more energetic than chemical reactions.<\/p>\n Uranium 235<\/a>\u00a0is a\u00a0fissile isotope<\/a>,\u00a0and its\u00a0fission cross-section<\/a>\u00a0for thermal neutrons is about\u00a0585 barns<\/strong> (for 0.0253 eV neutron). For fast neutrons, its fission cross-section is\u00a0on the order of barns<\/strong>. Most absorption reactions result in fission reactions, but a minority results in radiative capture<\/a>\u00a0forming\u00a0236<\/sup>U. The cross-section for radiative capture for thermal neutrons is about\u00a099 barns<\/strong> (for 0.0253 eV neutron). Therefore about 15% of all absorption reactions result in radiative capture of neutrons. About 85% of all absorption reactions result in fission.<\/p>\n <\/a> Most of these fission fragments are\u00a0highly unstable<\/strong>\u00a0(radioactive) and\u00a0undergo further\u00a0radioactive decays<\/a>\u00a0to\u00a0stabilize itself<\/a>.\u00a0Fission fragments\u00a0interact strongly with the surrounding atoms or molecules traveling\u00a0at high speed, causing them to ionize.<\/p>\n Most energy released by one fission\u00a0(~160MeV of total ~200MeV)<\/strong>\u00a0appears as kinetic energy of the fission fragments.<\/p>\n See also: Conservation of Energy in Nuclear Reactions<\/a><\/p><\/div><\/div> The fusion reaction<\/strong>\u00a0of deuterium and tritium is particularly interesting because of its potential of providing energy for the future.<\/p>\n 3T (d, n) 4He<\/strong><\/p>\n The reaction yields ~17 MeV of energy per reaction. Still, it requires an enormous temperature of approximately 40 million Kelvins<\/strong> to overcome the coulomb barrier by the attractive nuclear force, stronger at close distances. The deuterium fuel is abundant, but tritium must be either bred from lithium or gotten in the operation of the deuterium cycle.<\/p>\n The Q-value of this reaction can be calculated from the atom masses of the reactants and products:<\/p>\n m(3<\/sup>T) = 3.0160 amu<\/p>\n m(2<\/sup>D) = 2.0141 amu<\/p>\n m(1<\/sup>n) = 1.0087 amu<\/p>\n m(4<\/sup>He) = 4.0026 amu<\/p>\n Using the\u00a0mass-energy equivalence<\/a>, we get the\u00a0Q-value<\/strong>\u00a0of this reaction as:<\/p>\n Q = {(3.0160+2.0141) [amu] \u2013 (1.0087+4.0026) [amu]} x 931.481 [MeV\/amu]\n<\/p> = 0.0188 x 931.481 =\u00a017.5 MeV<\/strong><\/p>\n See also: Q-value<\/a><\/p><\/div><\/div> In general, nuclear fission<\/strong>\u00a0results in the release of\u00a0enormous quantities of energy<\/strong>. This energy can be used in nuclear power plants to produce electricity or process heat.\u00a0A typical\u00a0nuclear power plant<\/strong><\/a>\u00a0has an electric-generating capacity of\u00a01000 MWe<\/strong>. The heat source in the nuclear power plant is a\u00a0nuclear reactor<\/strong><\/a>. As is typical in all conventional thermal power stations, the heat is used to generate steam which drives a steam turbine<\/a>\u00a0<\/strong>connected to a generator that produces electricity. The turbines are heat engines subject to the efficiency limitations imposed by the second law of thermodynamics<\/strong><\/a>. In modern nuclear power plants, the overall thermodynamic efficiency is about one-third\u00a0<\/strong>(33%), so\u00a03000 MWth<\/strong>\u00a0of thermal power from the fission reaction is needed to generate\u00a01000 MWe<\/strong>\u00a0of electrical power.<\/p>\n This\u00a0thermal power<\/a>\u00a0is generated in a\u00a0reactor core<\/a>, especially the nuclear fuel (fuel assemblies), the moderator<\/a>,\u00a0and the\u00a0control rods<\/a>. The reactor’s core contains all the nuclear fuel assemblies and generates most of the heat (fraction of the heat is generated outside the reactor \u2013 e.g., gamma rays energy). According to a fuel loading pattern, the assemblies are exactly placed in the reactor.<\/p>\n Consumption of a 3000MWth<\/a> (~1000MWe) reactor (12-months fuel cycle):<\/strong><\/p>\n The Sun<\/strong> is a hot star. Really hot star. But all of the heat and light coming from the Sun comes from the fusion reactions happening inside the core of the Sun. Inside the Sun, the pressure is millions of times more than the surface of the Earth, and the temperature reaches more than\u00a015 million Kelvin<\/strong>. Massive gravitational forces create these conditions for nuclear fusion. On Earth, it is impossible to achieve such conditions.<\/p>\n\n
Nuclear Fission<\/h2>\n
Nuclear Fusion<\/h2>\n
Nuclear Fission vs Fusion – Reactions<\/h2>\n
Uranium – 235 Fission<\/h2>\n
\nThe average of the fragment mass is about 118, but very few fragments near that average are found. It is much more probable to break up into unequal fragments, and the most probable fragment masses are around mass 95 (Krypton) and 137 (Barium).<\/p>\nDeuterium-Tritium Fusion<\/h2>\n
Nuclear Fission vs Fusion – Examples<\/h2>\n<\/div><\/div>
Fission Powers Nuclear Reactors<\/h2>\n
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Fusion Powers the Sun<\/h2>\n