Nuclear Physics Institute, Academy of Sciences of the Czech Republic

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Presentation transcript:

Nuclear Physics Institute, Academy of Sciences of the Czech Republic Department of Nuclear Reactors, Faculty of Nuclear Sciences and Physical Engineering, Czech Technical University in Prague Monte Carlo Simulations of Natural Uranium Setups Irradiated With Relativistic Deuterons by Means of MCNPX Code Martin Suchopár XXI International Baldin Seminar on High Energy Physics Problems Relativistic Nuclear Physics and Quantum Chromodynamics JINR Dubna, Russia, September 10-15, 2012

Outline Energy + Transmutation & Kvinta setup description Method and models used in MCNPX simulations Beam monitoring and input parameters Computation results Conclusion Setup Method Results Beam monitors Conclusion Mezinárodní kolaborace E&T RAW se věnuje studiu tříštivých reakcí, produkci a transportu neutronů v sestavách tlustých terčů s blanketem (moderátorem). Dále se zabývá studiem transmutací štepných produktů a vyšších aktinidů v takovýchto sestavách. První tři terče již byly uznány jako oficiální IAEA benchmark terče.

Energy + Transmutation Setup E+T setup Kvinta setup Method Results Beam monitors Conclusion Sestava tlustého olověného terče obklopeného blanketem z přírodního uranu (přes 200 kg). Je umístěná v biologickém stínění z granulovaného polyethylénu a kadmia na vnitřní straně bedny. Ozářena na Nuclotronu protony a deuterony od 0.7 AGeV do 4 AGeV. Neutronové pole měřeno pomocí aktivačních detektorů. m natU = 206 kg

Kvinta 2010 and 2011 Setup Kvinta 2010 setup Kvinta 2011 setup Setup E+T setup Kvinta setup Method Results Beam monitors Conclusion 3 sections 4 detector plates Pb shielding 5 sections 6 detector plates no Pb shielding m natU = 315 kg m natU = 512 kg

Kvinta-M 2011 Setup Setup Method Results Beam monitors Conclusion E+T setup Kvinta setup Method Results Beam monitors Conclusion

Kvinta-M 2011 Setup Y p, d Z Setup Method Results Beam monitors 120 r 40 114 Target sections (U-238) p, d Y Z 262 393 131 17 524 655 700 Beam window, Ø 80 March 2011 irradiation Setup E+T setup Kvinta setup Method Results Beam monitors Conclusion 6 6

mounting pits for detector plates Kvinta-M 2011 Setup 900 beam entrance window 150×150 mm lead shielding 100 mm d Y Z 114 120 r 40 262 393 131 17 524 655 700 section U-238 mounting pits for detector plates Setup E+T setup Kvinta setup Method Results Beam monitors Conclusion December 2011 irradiation 7 7

Kvinta-M 2011 Setup Setup Method Results Beam monitors Conclusion E+T setup Kvinta setup Method Results Beam monitors Conclusion

Energy + Transmutation and Kvinta Irradiations Setup E+T setup Kvinta setup Irradiations Method Results Beam monitors Conclusion Energy + Transmutation set-up Beam energy [GeV] Beam particles Year Irradiation time [h:m] Integral beam flux [x1013] 0.7 protons 2004 8:51 1.47 1.0 2003 6:03 3.40 1.5 2001 12:03 1.14 2.0 7:43 1.25 1.6 deuterons 2006 8:00 2.45 2.52 2005 6:46 0.65 4.0 2009 17:48 1.99 9 9

Energy + Transmutation and Kvinta Irradiations Setup E+T setup Kvinta setup Irradiations Method Results Beam monitors Conclusion Kvinta set-up Beam energy [GeV] Beam particles Month Year Irradiation time [h:m] Integral beam flux [x1013] 2.0 deuterons March 2011 18:50 1.69 4.0 17:58 1.41 6.0 17:13 1.93 1.0 Decem 2011 14:26 1.53 12:24 March 2012 04:56 1.9 08:52 2.7 8.0 09:01 0.37 10 10

p, d QUINTA-M setup layout at the irradiation position Target «Quinta-М» QUINTA-M setup layout at the irradiation position Plate (700х400х16) Platform p, d SSNTD and AD positions on the QUINTA-M target surface Rails Beam window Pad with Pb foil monitor and SSNTD Detector plates Setup E+T setup Kvinta setup Irradiations Method Results Beam monitors Conclusion 11 11

QUINTA setup and equipment layout during an experiment at F-3 focus (December 2011) 3320 Beam extraction Ionization chamber Activation foil Profilometer QUINTA Polyethylene shielding Sc telescope 2 detectors Demon (NE213) ISOMER 20° 90° 160° Platform (turned by 2° relatively to the beam axis) detector Не3 Activation detectors Solid State Track detectors NE213, Stilben neutron detectors He-3 neutron detectors Setup E+T setup Kvinta setup Irradiations Method Results Beam monitors Conclusion 12 12

Main Objectives of the Kvinta Setup To have another set-up for benchmark studies of neutron production and transport simulation codes (e.g. MCNPX code) To have systematic of deuteron beams with energies above 1 GeV To obtain strong source of neutrons for transmutation tests Measurement of neutrons and delayed neutrons during low intensity beam irradiation by scintillation detectors Measurement of neutron field during high intensity beam irradiation by threshold activation and solid state track detectors Measurement of fission yields in thorium and natural uranium samples in fast neutron spectra Setup E+T setup Kvinta setup Irradiations Method Results Beam monitors Conclusion 13 13

Comparison of E+T and Kvinta Setup E + T setup model Kvinta 2011 setup model Setup Method Setup model MCNPX simulation Results Beam monitors Conclusion 30 U rods 54 U rods 61 U rods

Kvinta Setup with Lead Shielding Kvinta 2012 setup model Setup Method Setup model MCNPX simulation Results Beam monitors Conclusion front view 54 U rods 61 U rods side view top view 15 15

MCNPX simulations Used version MCNPX 2.7a Setup Method Setup model MCNPX simulation Results Beam monitors Conclusion Used version MCNPX 2.7a Used Los Alamos la150n neutron and la150h proton libraries All available physics models in the code tested Most preferred combination of models for spectra calculation – INCL-ABLA+FLUKA (time-consuming computation but provides the most reliable results)

Beam Monitoring deuteron beam with energies of 1, 2, 4, 6 and 8 GeV common measurement of beam intensity using ionization chambers aluminium and copper foils + SSNTD for beam monitoring aluminium foil – integral number of deuterons determination, placed several meters away from the set-up copper foil – deuteron cross-section measurement, placed together with the aluminium foil copper foil cut into pieces – beam position and profile determination, placed directly on the beginning of the target copper foil – beam alignment with the target axis, placed on the back of the target (2, 4, 6 GeV experiments without Pb shielding) Setup Method Results Beam monitors Conclusion

Beam Monitors Setup Method Results Beam monitors Conclusion Beam integral determination by Al foil Setup Method Results Beam monitors Conclusion Correction for Coincidences Peak area Dead time correction Self-absorption correction Decay during cooling and measurement Decay during irradiation Detector efficiency Beam instability correction g line –intensity per decay Correction for geometry change Square-emitter correction λ – decay constant, tirr – irradiation time, treal – real measurement time, tlive – live time of the detector, t0 – cooling time. 18 18

Beam Monitors Setup Method Results Beam monitors Conclusion Nyield – total amount of produced 24Na nuclei, A – molar weight, σ - cross-section, m – weight of the foil, S – area of the foil, NA – Avogadro’s number. 19 19

Beam Monitors Setup Method Results Beam monitors Conclusion Cu foil cut into 16 pieces 2x2 cm 4 most active foils cut again into 16 pieces 1x1 cm example of beam position and shape determination (6 GeV exp) beam centre beam FWHM xc 1.42 ± 0.05 cm xf 1.56 ± 0.05 cm yc -0.18 ± 0.05 cm yf 2.24 ± 0.05 cm beam centre beam FWHM xc 1.94 ± 0.10 cm xf 2.39 ± 0.20 cm yc 0.03 ± 0.10 cm yf 2.83 ± 0.20 cm 20 results from SSNTD (A. Potapenko) results from activation foils (Řež group) 20

Kvinta neutron fluxes Setup Method Results Beam monitors Conclusion neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding simulated neutron flux in Al foils

Kvinta neutron fluxes Setup Method Results Beam monitors Conclusion neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding simulated neutron flux in Al foils

Kvinta neutron fluxes Setup Method Results Beam monitors Conclusion neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Different types of Kvinta setups simulated neutron flux in Al foils

Kvinta neutron spectra Kvinta setup with Pb shielding simulated neutron spectra in Al foil Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Convolution of cross-sections calculated by TALYS+MCNPX with spectral fluences calculated by MCNPX for neutrons, protons, deuterons and pions

Kvinta neutron distribution Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding longitudinal neutron distribution Experiment 4 GeV December 2011 Kvinta setup with Pb shielding radial neutron distribution Experiment 4 GeV December 2011

Kvinta neutron distribution Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding longitudinal neutron distribution Experiment 4 GeV December 2011

Kvinta neutron distribution Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding radial neutron distribution Experiment 4 GeV December 2011

Kvinta neutron distribution Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding longitudinal neutron distribution Experiment 1 GeV March 2012

Kvinta neutron distribution Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding radial neutron distribution Experiment 1 GeV March 2012

Kvinta neutron distribution Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding longitudinal neutron distribution Experiment 4 GeV March 2012

Kvinta neutron distribution Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta setup with Pb shielding radial neutron distribution Experiment 4 GeV March 2012

Simulated multiplicity – various models Kvinta 5 sections setup neutron multiplicity Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta 5 sections setup with Pb shielding neutron multiplicity

Simulated multiplicity – various models Kvinta 5 sections setup neutron multiplicity per GeV Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta 5 sections setup with Pb shielding neutron multiplicity per GeV

Simulated multiplicity – various models Comparison of Kvinta 5 sections setup with and without Pb shielding neutron multiplicity Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Comparison of Kvinta 5 sections setup with and without Pb shielding neutron multiplicity per GeV

Neutron multiplicity from various models Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta 5 sections 4 sections 3 sections + Pb Model 2 GeV 4 GeV Bertini-ABLA 115.7 209.6 112.5 204.1 116.2 208.0 Bertini-Dresner 108.9 197.3 106.1 192.4 109.7 196.4 CEM03 118.3 213.1 115.2 207.7 114.7 204.7 INCL-ABLA 112.6 203.3 108.4 197.2 113.8 205.2 INCL-Dresner 104.1 186.6 100.6 181.6 105.8 189.4 ISABEL-ABLA 113.6 201.9 110.3 196.2 114.5 201.3 ISABEL-Dresner 189.3 102.7 183.9 106.7

Neutron multiplicity from various models Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Kvinta 5 sections 5 sections + Pb Model 1 GeV 2 GeV 4 GeV Bertini-ABLA 56.4 115.7 209.6 60.7 125.5 229.6 Bertini-Dresner 53.4 108.9 197.3 57.4 118.2 216.5 CEM03 58.5 118.3 213.1 60.4 123.6 224.9 INCL-ABLA 54.0 112.6 203.3 57.8 122.5 225.2 INCL-Dresner 50.7 104.1 186.6 54.6 113.5 207.6 ISABEL-ABLA 56.8 113.6 201.9 61.0 123.7 222.9 ISABEL-Dresner 52.8 105.8 189.3 57.0 115.5 209.0 36 36

Simulated multiplicity – various models Comparison of models in combination with FLUKA or LAQGSM - neutron multiplicity Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Comparison of models in combination with FLUKA or LAQGSM - neutron multiplicity/GeV

Simulated multiplicity – various models Comparison of models in combination with FLUKA or LAQGSM above 1 GeV - neutron multiplicity Setup Method Results neutron spectra neutron distribution MCNPX models Multiplicity in various models Beam monitors Conclusion Comparison of models in combination with FLUKA or LAQGSM above 1 GeV - neutron multiplicity/GeV

Conclusion Setup Method Results Beam monitors Conclusion made detailed model of the new Kvinta setup consisting of uranium target and blanket calculated neutron multiplicity of several modifications of the new Kvinta setup performed beam integral, position, shape and alignment monitoring using aluminium and copper foils beam characteristics used as input parameters for simulations simulated neutron fluxes and spectra in diverse positions in the new Kvinta setup and obtained experiment/simulation yield ratios studied dependency on various physics models included in MCNPX 39 39

Thank you for your attention