1. Sep.21 2007, Oslo, NorwayY. Kadi1 CERN, Switzerland 20-21 September 2007, Nuclear Risks - Safety and Security, Oslo, Norway From Waste to Value : Accelerator-based Inherently Safe Nuclear Power

2. Sep.21 2007, Oslo, NorwayY. Kadi2 A new primary energy source  By 2050, the world’s consumption (+ 2%/y) should reach 34 TW, of which 20 TW should come from new energy sources:  A major innovation is needed in order to replace the expected “decay” of the traditional energy sources!  This implies a strong R&D effort, which is the only hope to solve the energy problem on the long term. This R&D should not exclude any direction a priori! *Renewables *Nuclear (fission and fusion) *Use of hydrogen  Can nuclear energy play a major role?  Nuclear energy has the potential to satisfy the demand for a long time (at least 15 centuries for fission, essentially infinite for fusion if it ever works), and is obviously appealing from the point of view of atmospheric emissions.

3. Sep.21 2007, Oslo, NorwayY. Kadi3 Which type of nuclear energy?  Nuclear fusion energy: not yet proven to be practical. Conceptual level not reached (magnetic or inertial confinement?). ITER a step, hopefully in the right direction.  Nuclear fission energy: well understood, and the technology exists, with a long (≥ 50 years) experience, however, present scheme has its own problems: Military proliferation (production and extraction of plutonium); Possibility of accidents (Chernobyl [1986]; Three Mile island [1979]); Waste management.  However, it is not given by Nature, that the way we use nuclear fission energy today is the only and best way to do it. One should rather ask the question: Could nuclear fission be exploited in a way that is acceptable to Society?  To answer this question, Scientists around the world have carried out, since the 1990’s, an extensive experimental programme which has led to a conceptual design of a new type of nuclear fission system, driven by a proton accelerator, with very attractive properties.

4. Sep.21 2007, Oslo, NorwayY. Kadi4 Historical Background p The idea of producing neutrons by spallation with an accelerator has been around for a long time: + In 1950, Ernest O. Lawrence at Berkeley proposed to produce plutonium from depleted uranium at Oak Ridge. The Material Testing Accelerator (MTA) project was abandoned in 1954. + In 1952, W. B. Lewis in Canada proposed to use an accelerator to produce 233 U from thorium, in an attempt to close the fuel cycle for CANDU type reactors.  Concept of accelerator breeder : exploiting the spallation process to breed fissile material directly  soon abandoned.  Ip ≈ 300 mA + Renewed interest in the 1980's and beginning of the 1990's, in particular in Japan (OMEGA project at Japan Atomic Energy Research Institute), in the US (Hiroshi Takahashi et al. proposal of a fast neutron hybrid system at Brookhaven for minor actinide transmutation and Charles Bowman a thermal neutron molten salt system based on the thorium cycle at Los Alamos), and in Europe (SPIN program at the French-CEA).

5. Sep.21 2007, Oslo, NorwayY. Kadi5 Transmutation of nuclear waste Direct use of spallation neutrons ? Where :q fp = fraction of FP to be transmuted ( 99 Tc, 129 I, 135 Cs, 90 Sr, 85 Kr and 93 Zr ≈ 28%) E p = incident proton energy (1000 MeV)  sp = spallation neutron yield (≈ 30 for Pb target)  b = electrical efficiency for accelerating protons (≈ 50%)  T = thermal efficiency (≈ 33%) This would represent 60/200 ≈ 30% of the total fission energy produce  not economical !

6. Sep.21 2007, Oslo, NorwayY. Kadi6 Basic Principle of Energy Amplifier Systems  One way to obtain intense neutron sources is to use a hybrid sub-critical reactor-accelerator system called Accelerator- Driven System:  The accelerator bombards a target with high-energy protons which produces a very intense neutron source through the spallation process.  These neutrons can consequently be multiplied (fission and n,xn) in the sub- critical core which surrounds the spallation target.

7. Sep.21 2007, Oslo, NorwayY. Kadi7 Neutron Multiplication In and ADS ? Where :k = neutron multiplication factor * = source importance (≈ 1.5) = neutrons emitted per fission (≈ 2.5) E f = energy generated per fission (≈ 3.1x10 -10 W) i = accelerator current C = charge of a proton (= 1.6x10 -19 C) In order for the process to be self-sufficient

8. Sep.21 2007, Oslo, NorwayY. Kadi8 The FEAT experiment 3.6 tons of natural uranium

9. Sep.21 2007, Oslo, NorwayY. Kadi9 Main FEAT results

10. Sep.21 2007, Oslo, NorwayY. Kadi10 Physics of Sub-Critical Systems

11. Sep.21 2007, Oslo, NorwayY. Kadi11 Advantages of Sub-Critical Systems 1.EAs operate in a non self-sustained chain reaction mode  minimises criticality and power excursions EAs are operated in a sub-critical mode  stays sub-critical whether accelerator is on or off  extra level of safety against criticality accidents 1.The accelerator provides a control mechanism for sub-critical systems  more convenient than control rods in critical reactor  safety concerns, neutron economy 1.EAs accept fuels that would not be acceptable in critical reactors  Minor Actinides  High Pu content  LLFF... 1.EAs operate in a non self-sustained chain reaction mode  minimises criticality and power excursions EAs are operated in a sub-critical mode  stays sub-critical whether accelerator is on or off  extra level of safety against criticality accidents 1.The accelerator provides a control mechanism for sub-critical systems  more convenient than control rods in critical reactor  safety concerns, neutron economy 1.EAs accept fuels that would not be acceptable in critical reactors  Minor Actinides  High Pu content  LLFF...  Figure extracted from C. Rubbia et al., CERN/AT/95-53 9 (ET) showing the effect of a rapid reactivity insertion in the Energy Amplifier for two values of subcriticality (0.98 and 0.96), compared with a Fast Breeder Critical Reactor.  2.5 $ (k/k ~ 6.510 –3 ) of reactivity change corresponds to the sudden extraction of all control rods from the reactor. There is a spectacular difference between a critical reactor and an EA (reactivity in $ =  /  ;  = (k–1)/k) :

12. Sep.21 2007, Oslo, NorwayY. Kadi12 Energy Amplifiers vs Critical Reactors Main objective is to reduce the production of nuclear waste (TRU)  Energy Amplifier : * sub-critical * fast neutrons * Thorium + 233 U +TRU (Pu + Minor Actinides)  Reactor : * critical * slow neutrons * Uranium + Pu

13. Sep.21 2007, Oslo, NorwayY. Kadi13 Fast neutrons and high burn-up Fast neutrons allow a more efficient use of the fuel by allowing an extended burnup

14. Sep.21 2007, Oslo, NorwayY. Kadi14 Evolution of radiotoxicity of nuclear waste  TRU constitute by far the main waste problem [long lifetime – reactivity]. The system should be optimized to destroy TRU. Same as optimizing for a system that minimises TRU production. Interesting for energy production! Typically 250kg of TRU and 830 kg of FF per Gwe

15. Sep.21 2007, Oslo, NorwayY. Kadi15 Nuclear waste:  TRU: (1.1%) produced by neutron capture; dominated by plutonium:  destroy them through fission  Fission Fragments: (4%) the results of fissions  transform them into stable elements through neutron capture Note: thermal fission resilient elements  The strategy consists in using the hardest possible neutron flux, so that all actinides can fission instead of accumulating as waste.

16. Sep.21 2007, Oslo, NorwayY. Kadi16 Principle of LLFP destruction

17. Sep.21 2007, Oslo, NorwayY. Kadi17 Experimental Setup

18. Sep.21 2007, Oslo, NorwayY. Kadi18 TARC Results (2)

19. Sep.21 2007, Oslo, NorwayY. Kadi19 Energy Amplifiers vs Critical Reactors Main objective is to reduce the production of nuclear waste (TRU)  Energy Amplifier : * sub-critical * fast neutrons * Thorium + 233 U +TRU (Pu + Minor Actinides)  Reactor : * critical * slow neutrons * Uranium + Pu

20. Sep.21 2007, Oslo, NorwayY. Kadi20 Radiotoxicity  The radiotoxicity of spent fuel reaches the level of coal ashes after only 500 years, and is similar to what is predicted for future hypothetical fusion systems

21. Sep.21 2007, Oslo, NorwayY. Kadi21 General Features of Energy Amplifier Systems Subcritical system driven by a proton accelerator: * Fast neutrons (to fission all transuranic elements) * Fuel cycle based on thorium (minimisation of nuclear waste) * Lead as target to produce neutrons through spallation, as neutron moderator and as heat carrier * Deterministic safety with passive safety elements (protection against core melt down and beam window failure)

22. Sep.21 2007, Oslo, NorwayY. Kadi22 Detailed Features of Energy Amplifier Systems

23. Sep.21 2007, Oslo, NorwayY. Kadi23 R&D Activity in Europe Vast R&D activity in Europe over last 10 years: 12 countries, 43 institutions EU  31 MEuros Member States  100 MEuros Vast R&D activity in Europe over last 10 years: 12 countries, 43 institutions EU  31 MEuros Member States  100 MEuros

24. Sep.21 2007, Oslo, NorwayY. Kadi24  In FP5, a complementory combination of test facilities was set up in Europe.  EUROTRANS is fully using these test facilities. STELLA Loop CEA CIRCE Loop ENEA TALL Loop KTH CIRCO Loop CIEMAT CorrWett Loop PSI VICE Loop SCK-CEN CHEOPE Loop ENEA DEMETRA: Test Facilities

25. Sep.21 2007, Oslo, NorwayY. Kadi25 Gelina @ Geel (UE- Belgium) GSI @ Darmstadt (Germany) Cyclotron @ Uppsala (Sweden) nTOF @ CERN (Switzerland) and its TAS  -calorimeter Neutron capture (n,  ) resonances in one actinide NUDATA: Experimental Facilities

26. Sep.21 2007, Oslo, NorwayY. Kadi26 F. Groeschel et al. (PSI)  MEGAPIE Project at PSI  0.59 GeV proton beam  1.3 MW beam power  Goals:  Demonstrate feasablility  One year service life  Operating since August 2006 Proton Beam MEGAPIE TARGET

27. Sep.21 2007, Oslo, NorwayY. Kadi27 80 MW LBE-cooled XADS 80 MW Gas-cooled XADS 50 MW LBE-cooled XADS ( MYRRHA) The eXperimental Accelerator-Driven System (XADS) in the 5° FP of the EU

28. Sep.21 2007, Oslo, NorwayY. Kadi28 Worldwide Programs ProjectNeutron SourceCorePurpose FEAT (CERN) Proton (0.6 to 2.75 GeV) (~10 10 p/s) Thermal (≈ 1 W) Reactor physics of thermal subcritical system (k≈0.9) with spallation source TARC (CERN) Proton (1.5 & 2.75 GeV) (~10 10 p/s) Fast (≈ 1 W) Lead slowing down spectrometry and transmutation of LLFP MUSE (France) DT (~10 10 n/s) Fast (< 1 kW) Reactor physics of fast subcritical system YALINA (Belorus) DT (~10 10 n/s) Fast (< 1 kW) Reactor physics of thermal & fast subcritical system MEGAPIE (Switzerland) Proton (600 MeV) + Pb-Bi (1MW) -----Demonstration of 1MW target for short period TRADE (Italy) Proton (140 MeV) + Ta (40 kW) Thermal (200 kW) Demonstration of ADS with thermal feedback TEF-P (Japan) Proton (600 MeV) + Pb-Bi (10W, ~10 12 n/s) Fast (< 1 kW) Coupling of fast subcritical system with spallation source including MA fueled configuration SAD (Russia) Proton (660 MeV) + Pb-Bi (1 kW) Fast (20 kW) Coupling of fast subcritical system with spallation source TEF-T (Japan) Proton (600 MeV) + Pb-Bi (200 kW) ----- Dedicated facility for demonstration and accumulation of material data base for long term MYRRHA (Belgium) Proton (350 MeV) + Pb-Bi (1.75 MW) Fast (35 MW) Experimental ADS EADF (Europe) Proton (600 MeV) + Pb-Bi (4-5 MW) Fast (100-300 MW) Prototype Energy Amplifier Reference EA Proton ( ≈ 1 GeV) + Pb-Bi (≈ 10 MW) Fast (1500 MW) Energy Production & Transmutation of MA and LLFP

29. Sep.21 2007, Oslo, NorwayY. Kadi29 Conclusions  Can atomic power be green ? Physics suggests it can !!  Present accelerator technology can provide a suitable proton accelerator to drive new types of nuclear systems to destroy nuclear waste (including nuclear weapons) and/or to produce energy.  An Energy Amplifier could destroy TRU through fission at about x4 the rate at which they are produced in LWRs. LLFF such as 129 I and 99 Tc could be transmuted into stable elements in a parasitic mode, around the EA core, making use of the ARC method.  Next step: DEMO ? when ? where ?