Science A 52 Lecture 22 May 1, 2006 Nuclear Power What is it? What are its problems and prospects? Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 1 Nuclear Fission On of the most interesting accounts a fission and the discovery of the release of two or more neutrons during fission is on the WEB along with the voices of the major participants. You can almost feel the excitement in their voices as they described their reactions as experimental results came in. Let us listed to a few. http://www.aip.org/history/mod/fission/fission1/02.html Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 2 History of Nuclear Fission http://www.aip.org/history/mod/fission/fission1/02.html Here is a summary from the above site. It was only in 1938 that many scientists began to focus their attention on uranium, the heaviest of known elements. Leading the pack were two German chemists, Otto Hahn and Fritz Strassmann. For over thirty years, Hahn had been working with another talented scientist, Lise Meitner. However, Meitner was of Jewish ancestry, and had to flee Nazi Germany. Otto Hahn recalls... Miss Meitner - Professor Meitner - had left our laboratory on July 1938 on account of these Hitler regime things and she had to go to Sweden. And Strassmann and myself, we had to work alone again and in the autumn of '38 we found strange results.© Harvard Science, A 52 FHA+MBM Spring 2006 Lecture 22, 3 Fission History - continued By 1938, Hahn and Strassmann were among a number of scientists who were trying to find out what products are formed if you shoot neutrons into heavy elements. They hoped to find elements even heavier than uranium. Such altogether new elements would surely have scientific interest, and perhaps even practical uses. But the substances Hahn and Strassmann produced looked like radium or barium, two known and almost chemically identical elements... HAHN: We made precipitations, Strassmann and myself, where we could be absolutely sure that there could be nothing else but either radium or barium. Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 4 Now Meitner and Frisch -her nephew -understood what had happened in Hahn and Strassmann's experiment. The neutrons which they had shot into uranium had indeed been captured by the uranium nucleus. But then the nucleus changed shape, vibrated, and came apart entirely. This was not the usual slight transformation of a nucleus. The picture did however fit neatly with a recent theory of Niels Bohr's. He believed that a nucleus behaves like a liquid drop, and a liquid drop when hit hard enough, might stretch until it broke in two. Now, if that happened to a nucleus, a lot of energy would be released—atom for atom, far more energy than any process seen till then. This is what Meitner and Frisch thought happened to the nucleus of uranium after it had captured a neutron Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 5 A cartoon of U235 neutron capture http://www.atomicarchive.com/Fission/Images/fission.gif The target 92 U235 nucleus is often unstable with the additional neutron,and in ~ 10-14 seconds it splits into two fragments of nearly equal mass that are also unstable and in turn eject neutrons and γ rays. Not all captures of a neutron of 92 U235 results in a fission. Some captures produce 92 U236+ γ ray energy. Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 6 Let us listen to comments on one who was there when the first reactor went critical. http://www.aip.org/history/mod/fission/fission1/09.html Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 7 Energy release during fission To make the calculation of the energy released in fission we need to make a mass balance of all of the particles before and after fission - we will fine that the mass after fission is less that that before. The “missing” mass has been converted to energy. Some of the energy will be in the kinetic energy of the fission fragments, of the neutrons, and the gamma rays. In particle physics energy is generally expressed in electron volts. 1 eV = 1.6x10-19J 1eV is a very small unit of energy,but a proton has a very small mass. Let us see how to use this unit of energy. Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 8 Charge on the electron http://www.recipeland.com/facts/Oil-drop_experiment - The_apparatus Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 9 Energy expressed in Electron Volts http://hyperphysics.phy-astr.gsu.edu/hbase/electric/ev.html#c2 Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 10 http://hyperphysics.phy-astr.gsu.edu/hbase/electric/ev.html#c1 Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 11 Fission Calculation of mass conversion to energy We can use Einstein’s mass-energy relation: E = mc2 For nuclear calculations it is most useful to express the energy in MeV ⇒million electron volts. An electron volt is the amount of energy given to an electron accelerating it through a voltage difference of one volt. We need the famous equation of Einstein cast in mass units used in particle physics. Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 12 Fission Calculation of mass conversion to energy E(MeV) = m(amu) X 931 One atomic mass units (amu) is 1/16th the mass of O 16 . Using this scale the mass of the proton and the neutron are nearly 1. Mass of hydrogen atom = 1.00813 amu Mass of the proton = 1.00758 amu Mass of the neutron = 1.00897 amu Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 13 Fission Calculation of mass conversion to energy • We are now prepared to make a calculation of the energy released in fission of 92U235. What we need to do is to determine the products of fission when this nucleus captures a neutron and fissions. • The fission reaction is: U235 +neutron →2 fission fragments + ν neutrons +β- and γ-rays + energy To proceed we need to know the fission fragments and then their weight in amu. The fission yield of fission fragments from U 235 are known. Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 14 Glasstone, Samuel and Edlund,Milton; Nuclear Reactor Theory, van Nostrand, 1952, pg.67 Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 15 Fission Calculation of mass conversion to energy The isotopic weight of U235 = 235.124 amu, and the neutron involved in fission has an amu =1.00897. Therefore the reacting particles have a total weight of 236.133 amu and a mass number of 235 + 1 = 236 The most probable type of fission, nearly 6.4% of the total, gives products with mass numbers of 95 and 139, adding gives a mass number of 234 - two mass numbers less that the input, hence this fission must yield 2 neutrons. The fission products are stable nuclides with masses of 94.945 and 138.955, respectively. Doing the mass balances Before = After Fission 236.133 = mass converted to energy +(94.945+138.955) + 2x1.00897 ∴mass converted to energy = 236.133 - 235.918 = 0.215 amu Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 16 Fission Calculation of mass conversion to energy ∴Energy released in this fission would be 931x0.215 = 198 MeV The average values for all fissions of U235 Glasstone, Samuel, Nuclear Reactor Engineering,van Nostrand, 1955; pg.22 Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 17 Fission Neutrons per Capture •Fission of 92 U235 leads to the possibility of a chain reaction because an average of 2.5 neutrons are released in each fission of 235. 92 U •Not every time a U235 atom captures a neutron does fission occur, sometimes just this reaction occurs: U235 + neutron →U236 +γ-rays •Making an allowance for non-fission capture, there are only 2.1 neutrons released for each time a neutron is captured in U235 Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 18 Heat released by 1 pound of Fissionable Material is 3.6 x 1010 BTU or fission of 1 gram of material gives roughly 1 Mw day of power Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 19 Natural Uranium • Isotopic Composition of Natural Uranium Spring 2006 Mass number 234 % .006 235 0.712 238 99.282 © Harvard Science, A 52 FHA+MBM Lecture 22, 20 Making a Nuclear Reactor • It is impossible to make a nuclear power reactor using natural uranium since the concentration of U235 is so low. Only 2.1 neutron are available for the chain reaction. • Fission neutrons are released with high KE, and fission occurs most easily with thermal neutrons low neutron absorbing material is needed to slow the neutrons down without capture. Steel tubes and the like easily absorb thermal neutrons and cannot be used in a reactor using natural U. • The first reactors built used natural U and were very large - very pure graphite moderators. • Now slightly enriched U is used in power reactors. Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 21 Making a Nuclear Reactor • The first reactors built at Oak Ridge and Hanford were not for power but to create Plutonium239 a two step decay product from neutron capture in U238. • Pu239 can be used for bomb making and is separated from U and fission products chemically. • About 5% of the power of the reactor is in the decay of the fission products (FP). • This means that when the reactor is shut down, heat continues to be released by the FP and cooling must be provided. • Disposal of the FP and the Pu produced remains a serious problem. Spring 2006 © Harvard Science, A 52 FHA+MBM Lecture 22, 22