Energy and the New Reality, Volume 2: C-Free Energy Supply Chapter 8: Nuclear Energy L. D. Danny Harvey harvey@geog.utoronto.ca Publisher: Earthscan, UK Homepage: www.earthscan.co.uk/?tabid=101808 This material is intended for use in lectures, presentations and as handouts to students, and is provided in Powerpoint format so as to allow customization for the individual needs of course instructors. Permission of the author and publisher is required for any other usage. Please see www.earthscan.co.uk for contact details. Outline • • • • • • • • • • Basics of nuclear physics Fuels and reactions inside a nuclear reactor Types of nuclear power reactors The nuclear fuel chain Safety Nuclear weapons and terrorism risks Cost Embodied energy and GHG emissions Operational constraints Current capacity, future scenarios Basics of nuclear energy physics Nuclei and isotopes • A given chemical element has a fixed number of protons in its nucleus (number of protons = number of electrons) • A variable number of neutrons is possible, resulting in different isotopes of an element • Protons and neutrons together are called nucleons • The number of protons in the nucleus is called the atomic number, while the number of nucleons is called the mass number Superscripts and subscripts in front of the chemical symbol are used to represent the mass number and atomic number In 126C, for example, 12 is the mass number and 6 is the atomic number. Because the element name and atomic number are redundant, it is common to just write 12C instead of 126C. Forces in a nucleus • Electric force – repulsion between protons, varies with 1/distance2 • Nuclear force – attraction between any two nucleons (even having the same charge), varies much more strongly with distance (and so is significant only over a distance ~ diameter of the nucleus) • Can overcome the electric repulsive force at distances comparable to the radius of a nucleus • Thus, neutrons, by providing extra nuclear forces, act as a glue holding the protons in the nucleus together Neutron:proton ratio and stability of nuclei • As atomic number increases, the ratio of neutrons to protons required for stability of the nucleus increases • Nuclei with one or two less or one or two more neutrons are unstable – they eventually decay • If a heavy nucleus splits (fissions) into the nuclei of two lighter elements, it will often have too high a neutron:proton elements (depending on how the heavy nucleus splits), so the fission products will themselves often be unstable Figure 8.1 Neutron:proton ratios of the elements 140 Number of neutrons 120 Stable nuclei Unstable nuclei 100 80 neutron:proton = 1.5:1 60 neutron:proton = 1:1 40 20 0 0 10 20 30 40 50 Number of protons 60 70 80 90 Half lives of unstable nuclei • In a collection of unstable nuclei of a given isotope, not all the nuclei decay at once • Rather, it is observed that half of the nuclei existing at any given time will decay within a fixed length of time called the half-life • Thus, if the half life is 10 years and we start off with 1000 nuclei of a given isotope, there will be 500 left after 10 years, 250 left after 20 years, 125 left after 30 years, and so on Kinds of particles emitted during the radioactive decay of an unstable nucleus • Alpha particles, consisting of 2 protons and 2 neutrons (as in the nucleus of He) • Beta particles (electrons or, rarely, positrons) • Neutrons When alpha particles are emitted, the nucleus drops down by two atomic numbers. When an electron beta particle is emitted, a neutron in the nucleus turns into a proton, so the nucleus moves up by one atomic number. Gamma rays (very short wavelength, energetic electromagnetic radiation) are emitted when a nucleus drops from an excited to a ground state (perhaps following absorption of a neutron) Fission (splitting) of a nucleus • Can occur spontaneously (i.e., with no external stimulus) • Can also occur as a result of the absorption of a highenergy neutron – such nuclei are said to be fissionable • Can even occur (with some probability) when a neutron of arbitrarily low energy strikes the nucleus – such nuclei are said to fissile • When fission occurs, additional neutrons are released that can then sustain a fission chain reaction (and further neutrons will be released when the fission products themselves decay) • Some nuclei can absorb neutrons but without splitting – such nuclei are said to be fertile Fuels (or potential fuels) and decay reactions in a nuclear power reactor • Uranium (the overwhelmingly used fuel) • Plutonium (from recycling of spent fuel) • Thorium (usable in principle, has been demonstrated in the US) Natural Uranium • • • • 0.0055% U-234 (234U) 0.7205% U-235 99.275% U-238 All three isotopes are radioactive but with extremely long half-lives Note: The above percentages are in terms of numbers of atoms (atom%). When speaking of enrichment, percentages are given in terms of mass (mass%). 0.72atom% (U-235)= 0.71mass%. U-235 is fissile, and a sample reaction is 235U + n → 236U → 92Kr + 141Ba + 3n The fission products (92Kr and 141Ba here) and neutrons travel at high velocity, adding some of their kinetic energy to the atoms or molecules of the material through which they travel, heating it Note that, in the above, 1 neutron is absorbed and 3 are emitted. If one of the 3 that are emitted is subsequently absorbed by another 235U, the reaction will be self sustaining. Figure 8.2: Fission products of U-235 1.0E+01 1.0E+00 Yield (%) 1.0E-01 1.0E-02 1.0E-03 Stable Elements Half life > 100 yrs Half life 1 - 100 yrs Half life < 1 yr 1.0E-04 1.0E-05 70 80 90 100 110 120 130 Mass number 140 150 160 170 U-238 is fertile, and the reactions that occur are + n → 239U → 239Np + ß 239Np → 239Pu + ß 238U Pu-239 is both fissile and fertile – it can either absorb another neutron (followed by emission of a beta particle, just like 238U above), or it can split into two lighter elements (with a half life of 24,000 years) and emit more neutrons as it splits. The absorption of a neutron by 238U is the first in a sequence of transmutation reactions, shown in the next figure. Figure 8.3. Transmutation reactions beginning with U-238. n n Cm-242 Cm-243 Cm-244 n 10.1 hr 16.02 hr Am-241 n n Am-242 14.4 yr Pu-239 Pu-240 Pu-241 2.355 day n Am-243 Am-244 n Pu-242 n Np-239 23.5 min U-238 U-239 n Source: Modified from Wilson (1996, in The Nuclear Fuel Cycle, From Ore to Waste, Oxford University Press, Oxford ) To sum up, the reactions occurring inside a nuclear reactor are primarily: • Absorption of neutrons by 235U, producing 236U that then fissions and releases further neutrons • Absorption of some of the above neutrons by 238U, producing 239Np and 239Pu through the sequential emission of two beta particles (electrons) • Transmutation of 239Pu into successively heavier elements (the transuranic elements) through absorption of neutrons and emission of beta particles Thorium as a fuel • Thorium is fertile, meaning that it can absorb neutrons without splitting (like U-238) • It must be used in combination with U-235 or P-239, which serves as the neutron source • The end result is to produce U-233 (which does not occur naturally), which can be easily separated from the spent fuel and fed into another reactor as a fuel in a closed cycle • This would increase the energy that can be derived from a tonne of mined U by 85% compared to the usual once-through use of uranium • Significant new technologies would need to be developed to use the uranium-thorium cycle Sustaining nuclear chain reactions • Neutrons released by fission of U-235 after it absorbs a neutron move so fast that they have little chance of being absorbed by another U-235 (at least one neutron must be absorbed to sustain the process) • Thus, the neutrons must be slowed down using a moderator (water, heavy water, or graphite) – which absorbs energy from the neutrons without (ideally) absorbing the neutrons Stabilizing nuclear chain reactions • For the reaction not to grow exponentially out of control, exactly one neutron from each fission of U-235 must cause another fission • This ratio is maintained by inserting control rods between the uranium fuel rods – the more that are inserted, the more neutrons that are absorbed before they can cause another fission Thermal reactors • Neutrons that have been slowed down with a moderator are called thermal neutrons, and reactors using them are called thermal reactors • Those that use water as a moderator require that the uranium fuel (which is mostly U-238) be enriched in the fissile isotope U-235 (from about 0.7% to 3-4%). These are called light-water reactors • Reactors that use heavy water as a moderator (namely, the CANDU reactor) do not require enriched uranium. These are called heavy-water reactors. Fast and fast breeder reactors • Neutrons that have not been slowed down are called fast neutrons. They can still be used if the reactor has a high enough density of fissile material. This requires fuelling a reactor with U233, U-235, or Pu-239. These reactors are called fast reactors. • Pu-239 is a natural choice, since it is produced anyway in thermal reactors • If the Pu-239 content exceeds 10-20%, more Pu-239 will be created through absorption of neutrons by U-238 than is consumed during the fission that releases the neutrons, so these reactors are called fast breeder reactors Fast and fast breeder reactors (continued) • By repeatedly cycling nuclear fuel through fast breeder reactors, almost all of the U-238 in uranium (which accounts for > 99% of U) can be used as a fuel. Otherwise, only the U-235 (0.72%) serves as a fuel • The problem – Pu is ideal for making nuclear weapons. Vast amounts (1000s of tonnes) would need to be separated from spent fuel for recycling. Only 1-2 kg are needed to make a crude bomb. The elements produced with atomic number beyond uranium are called transuranic elements. Each of them is unstable and will eventually fission into lighter elements. Uranium and the transuranic elements, along with thorium, are referred to as actinides (they form a special series in the periodic table after the element actinium) Measures of nuclear radioactivity • Becquerel (Bq) – 1 Bq = a rate of one decay per second • Curie (Ci) – the rate of decay of one gram of radium 1 Ci = 3.7 x 1010 Bq • Gray (J/kg) or rad (100s of erg/gm) – amount of energy deposited per unit mass of living tissue • Sievert (Sv) or rem – the energy deposited (grays or rads) times a factor that accounts for the different amounts of damage caused by different kinds of radiation Sources of nuclear radiation: • Emission of beta particles during the transmutation of an actinide to an element with a higher atomic number (as in Fig. 8.3) • Emission of neutrons during the fission of an actinide • The fission products themselves, which are released with high velocity and are large, so they are quite damaging • Emission of beta particles during the eventual decay of the fission products themselves • Emission of alpha and beta particles produced by four different radioactive decay chains that proceed spontaneously without the absorption of a neutron Fission products of concern • Iodine-131, 8-day half life, becomes concentrated in milk, absorbed by thyroid gland. Of greatest concern for first few weeks after a potential nuclear accident • Stronium-90, 29-year half life, mimics calcium, becomes concentrated in bones • Cesium-137, 30-year half life, 6% of fission products, mimics potassium, distributed throughout body Radioactive decay chains • • • • Thorium series (Th-232 to Pb-208) Uranium series (U-238 to Pb-206) Actinium series (Pu-239 to Pb-207) Neptunium series (Pu-241 to Tl-205) The uranium series is shown in Fig 8.4 Figure 8.4a Uranium series radioactive decay chain U-238 =4.468 Gy 3 a=12.45x10 Th-234 =24.1 days 12 a=857.0x10 Pa-234m =1.17 min 15 a=73.99x10 U-234 =244.5 ky 6 a=231.4x10 Th-230 =77 ky 6 a=747.7x10 Ra-226 =1600 yr 9 a=36.62x10 Rn-222 =3.825 days 15 a=5.691x10 Po-218 =3.05 min 1 8 a=10.46x10 Pb-214 =26.8min 18 a=1.213x10 Bi-214 =19.9 min 18 a=1.634x10 Po-214 =164 sec 24 a=30.63x10 Pb-210 =22.3 yr 12 a=2.832x10 Bi-210 =5.01 days 15 a=4.592x10 Po-210 =138 days 12 a=166.3x10 Pb-206 Stable Figure 8.4b Uranium series radioactive decay chain 242 238 U 238 234 Mass Number 230 226 222 218 214 210 206 206 Pb 202 81 82 83 84 85 86 87 88 Atomic Number 89 90 91 92 93 Figure 8.5 U-238 Series Radiation 350 250 9 Radioactivity (10 Bq) 300 200 Rn-222 to Po-210 150 100 Ra-226 Th-230 50 U-234 U-238 Th-234 + Pa-234 0 103 104 105 106 107 Year 108 109 1010 107 Basis: PWR Spent Fuel 50 MWd/kg HM 4.5% initial enrichment Total 106 Fission Products 90 137 Si + Cs Total Actinides Figure 8.6 Sources of radioactivity from spent LWR fuel Ci/tHM 105 243 Pu 4 10 238 Pu Am241 3 10 240 Pu 239 Pu U238 Chain Am243 2 10 237 Np Chain 99 Tc 1 10 1 10 100 1000 10,000 100,000 1 million Years after Discharge Source: MIT (2003, The Future of Nuclear Power: An Interdisciplinary MIT Study) Partial summary so far: • Heat is produced inside a nuclear reactor from collisions of energetic particles produced by radioactive decay with the atoms of the material forming the reactor, or by the absorption of gamma rays • The kinds of radioactive decay are - the lighter nuclei produced by fission of U-235 (the predominant fissioning material) or by fission of transuranic elements (produced by neutron absorption) - beta particles emitted during the decay of transuranic elements that build up (mostly plutonium) - beta particles from the decay of the fission products themselves - gamma rays emitted following neutron capture by U235, U-238, or the transuranic elements Once the fuel has been removed from a nuclear reactor, • The reactions involving absorption of neutrons by 235U and 238U largely cease, as does the production of transuranic elements • The sources of radioactivity in spent nuclear fuel are -during the first year, the decay of fission products, with those having half lives of hours to days -one year after removal, the radioactivity has dropped to 1.3% of that at the time of removal, and is dominated by the decay of fission products with half lives of around 30 years (primarily Sr-90 and Cs-137) - thereafter, the decay of transuranic elements (especially Am-241, Pu-240 and Pu-239) dominates (until 100,000 years after removal) -finally, radioactivity from the U and Np series (which initially increases over time) dominates Nuclear Power Plant Reactor Technologies Nuclear Reactor Technologies • Boiling-water reactor (a LWR, thermal reactor) • Pressurized-water reactor (another LWR, thermal reactor) • CANDU HWR (also a thermal reactor) • High-temperature gas-cooled reactor (HTGR) Figure 8.7 Overview of nuclear powerplant technologies nuclear reactors thermal neutrons burners fast neutrons burners breeders Source: van Leeuwen (2007, Nuclear Power- The Energy Balance, Ceedata Consultancy, Chaarn, Netherlands, www.stormsmith.nl ) Figure 8.8a Boiling-water light-water reactor reactor vessel turbine generator steam electricity out uranium fuel condenser control rods water coolant/moderator in out cooling water Source: Wolfson (2003, Nuclear Choices: A Citizen’s Guide to Nuclear Technology, MIT Press, Cambridge) Figure 8.8b Pressurized-water light-water reactor control rods primary loop secondary loop turbine uranium fuel electricity out generator condenser reactor vessel pump out in cooling water Source: Wolfson (2003, Nuclear Choices: A Citizen’s Guide to Nuclear Technology, MIT Press, Cambridge) Figure 8.8c Liquid-metal fast breeder reactor heat exchanger core: U-235, Pu-239 steam generator steam to turbine liquid sodium liquid sodium U-238 blanket pump pump water in Source: Wolfson (2003, Nuclear Choices: A Citizen’s Guide to Nuclear Technology, MIT Press, Cambridge) Note: • The High Temperature Gas-Cooled Reactor (HTGR) uses uranium enriched to 93% U-235 (making it weapons-grade fuel), uses He as a coolant, and uses graphite (which is flammable) as a reactor. It has had mixed performance but is being reconsidered as a Generation IV reactor (see next slide). • The liquid-metal fast breeder reactor uses liquid sodium as a coolant, but sodium burns spontaneously on contact with air and reacts violently with water. Several were built but most have been shut down due to difficulties. Nuclear technology generations • Generation I: still a few in operation • Generation II: accounts for most of today’s reactors, based on military research of the 1940s and 1950s • Generation III: about 20 different designs are under development. Mostly incremental improvements from Generation II, but can still take decades to develop • Generation IV: 6 advanced concepts under development, most involving a closed cycle with reprocessing of spent fuel [on site] to separate and use plutonium. These exist only on paper at present, and would likely take 2-3 decades to develop. The Nuclear Fuel Chain Steps in the Nuclear Fuel Chain • Mining and milling of primary uranium, production of tailings waste • Enrichment of primary uranium, done by converting U to gaseous form and using centrifuges or membranes under pressure, creating a stream of depleted uranium (DU) waste. About 7 kg of natural uranium (0.7% U-235) are needed to produce 1 kg of U enriched to 3.6% U235, with U-235 depleted to 0.2% in the DU stream • Use of nuclear fuel (the burn-up is the amount of heat produced per kg of fuel) • Possible reprocessing of spent fuel, generating lots of liquid and gaseous wastes • Isolation (“disposal”) of spent fuel and/or reprocessing of wastes Fuel chain step 1: Separation of uranium from ores • Uranium occurs as oxides in uranium ores • The proportion of uranium ores containing U is quite small (ranging from 0.03% to 18.0% in commercial operations, but averaging only 0.2%) • The mass of ore that must be processed per unit mass of uranium, and the associated rock waste, is given by the reciprocal of the ore grade • Thus, for 0.2% grade ore, 500 tonnes of ore must be processed to obtain 1 tonne of U • However, in open-pit mines, up to 40 tonnes of rock might be excavated per tonne of ore that is extracted • The recovered ore is crushed and leached with sulfuric acid or alkaline fluids in order to separate out the uranium • The final product is called yellow-cake (U3O8) • 85% of the radionuclides in the original ore end up in the wastes, which are called tailings. • Management of the tailings (due to their radioactivity and toxicity) will need to continue essentially forever (several 100,000 years) Figure 8.9: World uranium extraction techniques in 2007 Heap leaching 2% Co-product mining 8% Other 0% Open pit mining 24% In situ leaching 28% Underground mining 38% Source: NEA/IAEA (2008, Uranium 2007: Resources, Production and Demand, OECD Publishing, Paris) Figure 8.10: Yellowcake – U3O8, produced from milling of the U ore followed by leaching from the crushed ore. Source: www.wise-uranium.org Fuel chain step 2: Enrichment of uranium in U-235 • Light-water reactors require the uranium fuel to be enriched in U-235 (from 0.7% in natural uranium to 3-5%) • This requires converting the uranium to a gaseous form (UF6), and using either gaseous diffusion through membranes under pressure, or centrifuges, to create 2 streams – one enriched in U-235 and the other depleted in U-235 • The depleted uranium has to be stored somewhere essentially forever Figure 8.11 Waste canisters containing depleted uranium, produced during the enrichment of natural uranium in U-235 Source: www.wise-uranium.org Fuel chain step 3: Use of U fuel • The various high-energy particles produced from the radioactive decay of the fuel (along with some gamma radiation) impart kinetic energy at the molecular scale to the surrounding materials through collisions with the atoms of the surrounding materials – that is, they heat it up • The amount of heat produced per unit mass of fuel is called the fuel burn-up. • Burn-ups have increased from about 20 GWd (gigawatt-days) per tonne in the 1970s to an average today of 45 GWd/t in BWRs and 50 GWd/t in PWRs • Electricity production per tonne of fuel is given by the burn-up times the thermal efficiency of the steam turbine • Higher burn-ups require the use of more enriched uranium and use of a greater fraction of the U-235 that is in the original fuel • Increasing the U-235 enrichment from 4.5% to 8.3% would double the burn-up from 40 GWd/t to 80 GWd/t, reduce the consumption of uranium ores by 7%, reduce the mass of spent fuel by 50%, and increase the concentration of radionuclides in the spent fuel (increasing the heat production per unit mass) Fuel Chain Step 4: Optional Reprocessing of spent fuel • Recycle into a LWR • Recycle into a HWR • Recycle into fast reactors or fast breeder reactors Spent reactor fuel contains • Most of the original U-238 and perhaps 20% of the original U-235 (the U-235 may have gone from an enriched concentration of 4% down to 0.8%) • Fission products • Plutonium and minor actinides (such as Np-237, Am-241 & Am-243, Cm-242 to Cm-248, and Cf249 to Cf-252) 30kg, FP 1kg, Tu 9kg, Put 8kg, U-235 U-235 31kg U-238 969kg U-238 952kg FRESH FUEL (3.1% ENRICHMENT) SPENT FUEL (33,000 MWd/t) 1 TONNE OF FUEL Figure 8.12 Composition of fresh and spent nuclear fuel Source: Albright and Feiveson (1988, Annual Review of Energy 13, 239–265) Reprocessing • Reprocessing requires separating the U-235 and Pu-239 (which can be used as a fuel) from the spent fuel • This is done by dissolving the spent fuel in a strong acid • The fission products and minor actinides are not useful as a fuel, and are highly radioactive, so they must be removed and stored in containers that are actively cooled Reprocessed Fuel • Consists of mixtures of oxides of U-235 and Pu, accounting for about 4.5% of the total if fed to LWRs, along with natural or depleted uranium (from previous enrichment activities) • It is therefore called Mixed Oxide (MOX) fuel • About 5-6 kg of spent fuel must be processed to make 1 kg of MOX Reprocessed Fuel (continued) • There will be a deficit in U-235 in the MOX, which can be made up either by adding Pu from dismantled nuclear weapons (thereby providing a way of getting rid of Pu if and as the world disarms), or by using the spent fuel from more than one LWR to provide the fuel for the equivalent of one LWR running on 100% reprocessed fuel • In practice, a LWR would take only 1/3 MOX and 2/3 fresh fuel • The net result is that using reprocessed fuel in LWRs extends the uranium supply by 20-25% Other reprocessing options: • Use spent LWR fuel directly in a CANDU HWR • Recycle in a fast reactor that is designed to exactly consume the amount of Pu and other transuranic elements produced from a LWR, leaving only the fission products (all of which have half lives of 30 years or less) • Recycle in a fast breeder reactor, having a net production of Pu (from U-238) that can be fed as fuel to other reactors Status of Reprocessing Today • US reprocessing shut down due to concerns about proliferation of nuclear weapons, especially after India made a bomb from extracted Pu in 1974 • Japanese reprocessing shut down in 1995 after a severe sodium fire; might be restarted • UK reprocessing shut down in 2005 after discovery of leakage of spent fuel dissolved in acid • France (1700 t/yr), Russia (400 t/yr), and India (275 t/yr) are the major reprocessors today • Other countries (including the US) had been reconsidering • Only 27 GW of nuclear plants out of 369 GW worldwide use some reprocessed fuel (1/3 of their total, so they are equivalent to 9 GW out of 369 running on 100% reprocessed fuel) Fuel Chain Step 5: Decommissioning of nuclear powerplants This involves: • Removal of the spent fuel • Cleaning and decontaminating the plant as thoroughly as possible • Altering the ventilation system • Removing all ancillary equipment and buildings • Dismantling or reducing in size and removing the remaining plant parts Decommissioning is rendered difficult and expensive because many of the plant materials will have been rendered radioactive during the operation of the plant. The radioactivity comes from activation products – nonradioactive isotopes in the plant materials that are turned into radio-active isotopes through the absorption of neutrons. Examples include Ca-41 and Cl-36 produced from Ca-40 and Cl35 in concrete and steel. Due to this radio-activity, the no-longer used plant must site idle for some time (up to 135 years allowed in the UK, up to 60 years in the US) before decommissioning begins. In Japan, idled plants must be decommissioned within 10 years of shutting down. Fuel Chain Step 6: Isolation (“disposal”) of nuclear waste Categories of nuclear waste • High level – spent fuel, liquid wastes from production and possible later reprocessing of spent fuel, solids into which such liquid wastes have been converted • Transuranic or intermediate-level wastes, produced during processing of spent fuel • Low-level waste, produced during most steps of the nuclear fuel chain Isolation Options • Reprocessing – using cycles designed to consume Pu-235 and other long-lived transuranic elements, leaving shorter-lived radioisotopes • Deep geological disposal – concerns about groundwater as climate changes • Transmutation – exceeding complex Geological repositories rely on one of two kinds of barriers to prevent spread of radio-nuclides: • Geological barriers – as in the proposed and then withdrawn and maybe re-instated Yucca Mountain site in Nevada (the assumption had been that there would never be groundwater flow through the site during the next 1 million years) • Engineered barriers, as in the Finnish and Swedish proposals The Swedish proposal requires • a 25 t cast-iron canister for every 2 t of waste • a 5-cm thick copper cladding around each canister • Placement of canistors 500 m below ground, packed with bentonite (a swelling clay) Uranium Mine Figure 8.13. Waste flow associated with 1 GWyr of electricity production, assuming: 108411.3 tU ore (216.8 tU) Uranium Mill 244.9 tU3O8 108,000 t mill tailings (207.6 tU) Conversion Plant 305.5 tUF6 542,000 t waste rock 145 t solid waste 3 1343 m liquid waste (206.6 tU) Enrichment Plant 5:1 waste rock/ore ratio, 0.2% grade, 38.0 t enriched UF (25.7 tU) enrichment Fuel Fabrication to 3.6%, Plant 42 GWd/tU burnup 267.6 t depleted UF6 (180.9 tU) 6 28.8 tUO2 3 12.7 m solid waste 288.7 m3 liquid waste (25.4 tU) Nuclear Power Plant 1 GW-yr of electricity 28.8 t spent fuel Nuclear fuel chain: alternative chains with some recycling Figure 8.14a Nuclear fuel once-through LWR chains Option 1a, Low Burnup: 50 GWd/t, n=0.33 Option 1b, High Burnup: 100 GWd/t, n=0.33 Source: MIT (2003, The Future of Nuclear Power: An Interdisciplinary MIT Study) 386,000 t natural U 286,000 t natural U 29864 t spent fuel, 50 GWd/tHM burnup 14932 t spent fuel, 100 GWd/tHM 27893 t/yr U (93.4%) 13055 t/yr U (87.43%) 1538 t/yr FP (5.15%) 1538 t/yr FP (10.30%) 397 t/yr Pu (1.33%) 294 t/yr Pu (1.97%) 36 t/yr MA (0.12%) 45 t/yr MA (0.30%) Figure 8.14b Nuclear fuel chain Option 2, recycling of Pu from spent fuel and use of depleted U in a LWR with 50 GWd/t burnup, n = 0.33 Pu: 233 t/yr Source: MIT (2003, The Future of Nuclear Power: An Interdisciplinary MIT Study) Figure 8.14c Nuclear fuel chain Option 3, LWR with 50 GWd/t burnup, CF=0.9, n=0.33; and FR with 120 GWd/t burnup, CF=0.9, n=0.44 Source: MIT (2003, The Future of Nuclear Power: An Interdisciplinary MIT Study) Safety Issues • • • • Routine operation of nuclear power plants Terrorist attacks on nuclear power plant Military strikes on nuclear power plants Accidents at reprocessing plants (several have already occurred, and we’re hardly doing any reprocessing) Nuclear weapons proliferation issues There is concern both about more states acquiring nuclear weapons, and about sub-national or terrorist groups getting enough materials to make a crude nuclear bomb. There are two distinct points of risk • Enrichment of U-235 for power generation – 2/3 of the effort require to make bomb-grade uranium (90% U-235) already has to be expended just to make reactor-grade uranium (3.5% U-235) • Separation of Pu from spent fuel (which is highly radioactive and thereby inhibits handling), thereby making it relatively safe and easy to use Figure 8.15: Effort (represented by Separative Work Units) to enrich uranium in U-235 Separative Work Units per kg of U-235 300 Reactor grade 250 200 Cd=0.002 150 Cd=0.003 100 Bomb grade 50 0 0.0 0.2 0.4 0.6 U-235 Fraction 0.8 1.0 Cost of nuclear electricity Factors contributing to the cost of nuclear electricity • • • • Capital cost Capacity factor Fuel cost Decommissioning and long-term isolation of nuclear wastes Capital Cost • Big unknown for complicated, new technologies, especially if not mass produced (such as Generation III or IV nuclear reactors) • Early (2000-2005) estimates of future construction costs clustered around $2000/kW • Many recent reactors have cost $3000-4000/kW • Some analysts have projected costs of $600010000/kW Figure 8.16 Capital cost of nuclear power plants 12000 Overnight Capital Cost ($/kW) 10000 Wall Street & Independent Analysts 8000 6000 Completed Nuclear Reactors Utilities 4000 Early Vendors, Government & Academics 2000 0 1970 1975 1980 1985 1990 1995 2000 2005 Year Source: Cooper (2009, Institute for Energy and the Environment, Vermont Law School) 2010 Note: The preceding slide gives “overnight” capital costs. These costs • Do not include interest that accrues during the construction period (which can be up to 10 years) • Do not include inflation of component costs during the construction period (which have tended to exceed the general rate of inflation) • Do not include additional utility costs, such as the cost of upgrading the grid to accept a large new source of power Rather, overnight costs are the costs for the powerplant alone if everything could be bought at once and the plant could be constructed overnight. Final costs are typically 50-75% greater than the overnight cost, but have been as high as double the overnight cost. Fuel costs • Fuel is a very small contributor to the overall cost of nuclear electricity, and the cost of uranium itself is a small factor in the overall fuel cost • Thus, the price of uranium can increase greatly (due to future scarcity) with little impact on the overall cost of nuclear energy (but increased uranium cost would make more uranium economically available) Decommissioning and long-term isolation costs • These are likely to significantly increase the overall cost of nuclear electricity • Most current assessments seem to vastly underestimate these costs • In any case, there are very few firm data available Figure 8.17: Estimated cost of decommissioning graphite-moderated nuclear power plants in the UK Estimated Decommissioning Cost ($/kW) 12000 10000 8000 6000 4000 2000 0 0 200 400 600 800 Powerplant Size (MW) 1000 1200 Figure 8.18 Cost of nuclear energy 0.30 Cost of electricity (2008$/kWh) 0.25 Wall Street & Independent Analysts 0.20 0.15 Completed Nuclear Reactors Utilities 0.10 Early Venders, Government & Academics 0.05 0.00 1970 1975 1980 1985 1990 1995 2000 2005 Year Source: Cooper (2009, Institute for Energy and the Environment, Vermont Law School) 2010 Note: The preceding costs assume essentially zero insurance and liability costs compared to the potential cost of a nuclear accident. This is because no private investors would be prepared to accept the risk, and no insurance companying would be prepared to sell insurance, if the nuclear power plant operators would be financially responsible for the majority of the potential damage in the event of a serious accident. EROEI and GHG Emissions Figure 8.19 Fraction of uranium recovered from ore as a function of the ore grade Source: van Leeuwen (2007, Nuclear Power- The Energy Balance, Ceedata Consultancy, Chaarn, Netherlands, www.stormsmith.nl ) Supplemental figure: The Escondida copper mine in Chile. Source: van Leeuwen (2007, Nuclear Power - The Energy Balance, Ceedata Consultancy, Chaarn, Netherlands, www.stormsmith.nl ) Figure 8.20 Cross section of the proposed open-pit Olympic uranium mine h1 h2 h3 Source: van Leeuwen (2007, Nuclear Power- The Energy Balance, Ceedata Consultancy, Chaarn, Netherlands, www.stormsmith.nl ) Energy Inputs Related to Nuclear Energy • Energy is required to make all of the materials that go into a nuclear powerplant (cement, steel, copper, aluminum especially) • Energy is also used during mining and milling of uranium ores, during the enrichment process, during the operation of the nuclear power plant, and later during decommissioning, possible reprocessing of spent fuel, excavation of the longterm repository for nuclear wastes, and packaging of the wastes Energy Return Over Energy Invested (EROEI) • The EROEI can be computed based on the ratio of all the electrical energy generated to all secondary energy inputs (fuels and electricity) • Alternatively, it can be based on the primary energy saved when nuclear electricity is produced (assuming that fossil fuel electricity generated at 40% efficiency is displaced) and the total primary energy inputs • The effective efficiency in using fuels can be computed as the net electricity production (electricity produced minus all electricity inputs) divided by the fuel primary energy • The EROEI and effective efficiency drop sharply as the ore grade decreases from 0.1% to 0.01%. Figure 8.21 Published estimates of the amount of energy required to construct a 1 GW nuclear powerplant 40 Construction Energy (PJ) 44, 81, 107, 269 30 Based on input-output analysis Based on economy-wide AEI Based on process analysis 20 10 0 LWR BWR PWR HTGR HTR Type of Reactor AEI=average energy intensity (KJ/$) FBR HWR AGR Figure 8.22 Energy use over the 40-year life of a 1-GW LWR nuclear powerplant with a capacity factor of 0.87 1000 Handling overburden, 1.35 x ore mass MMR, underground mine Lifetime Energy Use (PJ) 800 Spent fuel Decommissioning Waste operations 600 Fuel production & reactor operations Construction of reactor 400 200 0 1 0.5 0.15 0.1 0.06 0.05 Ore Grade (%U3O8) 0.04 0.03 0.02 0.01 24 1200 20 1000 16 800 12 600 8 Fuel efficiency, Underground mine Fuel efficiency, Open-pit mine EROEI, Underground mine EROEI, Open-pit mine EROEI, ISL - Low energy estimate EROEI, ISL - High energy estimate 4 0 1 0.1 Ore Grade (%) 400 200 0 0.01 Fuel Efficiency (%) Lifetime EROEI Figure 8.23 EROEI based on secondary energy for the nuclear powerplant featured in Fig. 8.22 (left scale) and fuel efficiency (net electrical energy generated divided by fossil fuel use) (right scale). Note: the present world average grade of ore is about 0.2% GHG Emissions • Wide range of estimates • Middle value is about 1/3 that of a state-of-art the natural gas combined cycle powerplant (at 60% efficiency) • Would increase with a decrease in the average grade of the ore being mined (due to greater energy use during mining and milling operations) Nuclear Energy Today Figure 8.24 Nuclear Share of Electricity France Lithuania Slovak Republic Belgium Switzerland Ukraine Bulgaria Armenia Slovenia South Korea Hungary Switzerland Germany Czech Republic Japan Finland Spain USA UK Russia Canada 0 10 20 30 40 50 Percent Source: www.iaea.org/programmes/a2/index.html 60 70 80 90 Figure 8.25 Growth in nuclear energy TWh/yr Electricity Generation 2500 2000 Asia Pacific Africa FSU Europe S & C America North America 1500 1000 500 0 1965 1970 1975 1980 1985 1990 1995 2000 2005 Year Figure 8.26 Nuclear powerplant capacity factors 100 90 80 Capacity Factor 70 60 50 40 30 20 10 20 05 20 03 20 01 19 99 19 97 19 95 19 93 19 91 19 89 19 87 19 85 19 83 19 81 19 79 19 77 19 75 19 73 19 71 0 Source: WEC (2007, 2007 Survey of Energy Resources, World Energy Council, London) Figure 8.27 Nuclear reactor ages 35 Number of Reactors 30 25 20 15 10 5 0 0 5 10 15 20 25 30 Age (Years) Source: Data from www.iaea.org/programmes/a2/index.html 35 40 45 Figure 8.28 World Uranium Resources Other 11.5% Ukraine 3.6% Australia 22.7% Niger 5.0% Namibia 5.0% Brazil 5.1% Kazakhstan 14.9% USA 6.2% Canada 7.9% South Africa 8.0% Russia 10.0% Potential Future Contribution of Nuclear Energy Maintaining existing capacity • As of April 2007, 114 out of 436 nuclear power reactors in the world were more than 30 years old • Assuming the normal reactor lifetime of 40 years, 114 new reactors will be needed during the next 10 years, or an average of one every 5 weeks – just to maintain the existing capacity • The following decade, a new reactor would be needed every 22 days on average just to maintain the existing capacity Limits on expansion • To maintain a nuclear fleet with 1000 GW capacity (about 25% of current total world electrical capacity but almost 3 times the 2007 nuclear capacity of 369 GW) would generate 20,000 tonnes of spent fuel per year (assuming a 90% capacity factor and burn-up of 50 GWd/t), or 10,000 tonnes of spent fuel per year (if a 100 GWd/t burn-up is achieved). • This would require the establishment of a new Yucca Mountain scale waste repository every 3.5 to 7 years, or • Reprocessing would require 6-12 times the current French reprocessing capacity (1700 t/yr). • Included in this would be production of 195-264 tonnes of Pu per year Resource Constraints • Its hard to say how much uranium might become available with large increases in the price of uranium (due to scarcity) • However, in the absence of reprocessing and use of fast breeder reactors (which pose enormous terrorism risks in today’s world), the supply would likely not be adequate for more than 100 years (and possibly much less), given a fleet of 1000 GW. • As lower grades of uranium ore are exploited, the energy cost associated with extracting and processing the ore would rise sharply (at present the nuclear lifecycle GHG emissions are about 1/3 that of a natural gas powerplant at 60% efficiency) Figure 8.29 Distribution of “identified” uranium resources with respect to the ore grade Mass of Uranium (kt) 2000 1600 Total 1200 800 Soft or mixed 400 0 100 10 1 0.1 0.01 Ore grade (% U3O8) Source: van Leeuwen (2007, Nuclear Power- The Energy Balance, Ceedata Consultancy, Chaarn, Netherlands, www.stormsmith.nl ) Figure 8.30 Cost of uranium vs the grade of ore supplying the uranium Source: van Leeuwen (2007, Nuclear Power- The Energy Balance, Ceedata Consultancy, Chaarn, Netherlands, www.stormsmith.nl ) Concluding Thoughts Given that nuclear energy could supply 25% of our electricity needs for at most 100 years, after which we’ll have to find alternatives anyway, and that the next 100,000 years or more of generations will be burdened with dangerous wastes, can we ethically justify such a short fling with nuclear energy now? In any case, it is not possible to ramp up nuclear energy fast enough to make a noticeable difference to our GHG emissions before 2050. This is not soon enough – large reductions are needed during the next 30 years in order to significantly reduce the risk of or extent of the foreseeable global ecological catastrophe