Kern- und Teilchenphysik I Lecture 6: Nuclear fission Prof. Nico Serra Dr. Patrick Owen, Dr. Silva Coutinho http://www.physik.uzh.ch/de/lehre/PHY211/HS2016.html Nuclear Fission and Fusion We have seen that fission is the fragmentation of a heavy nucleus into 2 more stable components Usually requires to be triggered by a slow neutron For these nuclei it is energetically favourable (exothermic reaction) to fuse into a single nucleus Nico Serra 2 Nuclear and Particle Physics I Nuclear Fission Nuclides with Z>40 can in principle split, however the barrier is so high that the tunnelling effect is very improbable, so in practice only nuclides with very large A split. Nico Serra 3 Nuclear and Particle Physics I Nuclear Fission Let’s consider an ✏ deformation of the sphere into an ellipsoid of axis a = R(1+✏) and b = (1 ✏/2) • The surface energy becomes Es = as A2/3 (1 + 25 ✏2 + ...) • The Coulomb energy becomes Ec = ac Z 2 A • The di↵erence in energy becomes E= 1/3 (1 ✏2 2/3 (2a A s 5 In order for the deformation to be favourable implies: Z2 2as ' 48 A ac 1 2 5✏ + ...) ac Z 2 A 1/3 ) E should be negative, which This happens for nuclei with Z > 114 and A > 270 Nico Serra 4 Nuclear and Particle Physics I Induced Fission If a large A material (e.g. 235U) breaks into smaller nuclei, close to the iron binding energy peak, it releases energy Spontaneous Fission is rare because it is suppressed by the tunnelling of the Coulomb barrier It is possible to perturbate the nucleus, such that it is in unstable state and breaks, this is called induced fission Nico Serra 5 Nuclear and Particle Physics I Neutron Interaction • Scattering: the neutron bounces o↵, with or without the same energy • Activation: the neutron is absorbed and the resulting nuclide is radioactive Inelastic Scattering: Scattered neutron, E2 e le c tro n – The nucleus emit a gamma ray ne utro n Incident neutron, E1 p ro to n – Fission follows absorption Gamma Photon, Eγ E1 = Eγ + E2 Scattered neutron, E2 Elastic Scattering: e le c tro n ne utro n Incident neutron, E1 p ro to n a EA E1 = EA + E2 Gamma Photon, Eγ E γ ~ 7 MeV Neutron Absorption: e le c tro n ne utro n Incident thermal neutron, E Nico Serra 6 p ro to n Nuclear and Particle Physics I Induced Fission A neutron splits a uranium nucleus, releasing energy (quickly turned to heat) and more neutrons, which can repeat the process. Nico Serra The energy appears mostly in the kinetic energy of the fission products and in the beta and gamma radiation. 7 Nuclear and Particle Physics I Outcome • Energy is released (the quantity M (A, Z)⇤ nMn ) M (A1 , Z1 ) M (A2 , Z2 ) • One neutron triggers the reaction, 2 or 3 (on average) are produced and can induce more fission • Depending on the fission material, the shape and the mass the reaction can be self-perpetuating (critical mass) • Nuclear reactors are designed to have self-sustaining and controllable reaction Nico Serra 8 Nuclear and Particle Physics I Fission • Only a few nuclides can fission • Nuclides that can fission for any incoming neutron are called fissile • The only naturally occurring fissile nuclide is 235 • Other fissile nuclides are 233 U , 239 P u and naturally to any appreciable extent P u, none of this is present 241 U • Nuclides that can be induced to fission only by neutrons of energy higher than a certain threshold are called fissionable, e.g. 238 U and 240 P u Nico Serra 9 Nuclear and Particle Physics I Energy by fission Energy released per fission ~ 200 MeV [~ 3.2*10-11 J]. ! This is hundreds of thousands, or millions, of times greater than energy produced by combustion, but still only ~0.09% of mass energy of uranium nucleus! ! The energy released appears mostly (85%) as kinetic energy of the fission fragments, and in small part (15%) as the kinetic energy of the neutrons and other particles. ! The energy is quickly reduced to heat (random kinetic energy) as the fission fragments are stopped by the surrounding atoms. ! The heat is used to make steam by boiling water, ! The steams turns a turbine and generates electricity. ! Nico Serra 10 Nuclear and Particle Physics I
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