TE/VSC and DGS/RP
Study of radioactive neutral isotopes propagation at ISOLDE: a Monte - - PowerPoint PPT Presentation
Study of radioactive neutral isotopes propagation at ISOLDE: a Monte - - PowerPoint PPT Presentation
Study of radioactive neutral isotopes propagation at ISOLDE: a Monte Carlo and a spectroscopic analysis Maddalena Maietta Universita` degli Studi di Napoli Federico II TE Vacuum, Surface & Coating, IVM Radioprotection DGS/RP 7 th
TE/VSC and DGS/RP
- Introduction: Description of ISOLDE facility
Main scopes of the project
- Numerical Methods: Simulation theory
Practical development Results
- Experimental Analysis: Two experiments
Description of experimental set up Results
- Next steps
- Conclusion
Outline of this talk
TE/VSC and DGS/RP
LINAC 2 BOOSTER ISOLDE
Introduction: ISOLDE
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Introduction: ISOLDE
1.4 GeV
Intensity: 3.5 ∗ 1013 protons/1.2s Energy of products: 60 keV
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HRS31 HRS23 HRS25 HRS22 HRS24 HRS32
My project
Analysis of the progression of neutral radioactive gas species along the ISOLDE beam line:
- Monte Carlo simulation
- Experimental Analysis
Tape station
- Construction of a general tool for RIB
vacuum;
- Define a zone separation, according to level
- f contamination
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Why contamination study is so important?
Isolde vacuum system:
The Front Ends zone
The separators zone The Experimental Hall
- Venting to atmosphere
via Filters and Monitoring RFQ
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Which species are targeted by the study?
Target with high dose rates: U (i.e. UCx) and Th (α emitters); Pb; Ta. First transfer function (“filter”): Target choice IONS: Transported by the beam optics NEUTRALS: Diffusing according to Maxwell- Boltzmann statistics and direction distribution
Neutrons Protons
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For neutral contamination study Isolde Users
1) Choice of target temperature; 2a) Choice of transfer line temperature 2b) Conductance of transfer line; 3) Ionization Efficiency (~10%).
Volatility; 1 - Ionization Efficiency (~90%).
Which species are targeted by the study?
Noble gases (few volatile metals e.g. Zn, Cd, Hg ?)
TARGET OVEN
1
TRANSFE R LINE
2
ION SOURCE
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EXTRACTION ANALYSIS GAS INLET Quartz tube Transfer tube Tantalum tube with the target material
Ion species targeted
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Numerical Methods : Monte Carlo simulation
Pills of Physics of molecules in vacuum : two important equations… Maxwell Boltzmann Lambert’s cosine law
𝑒𝑂/𝑒𝑤 𝑂 = 4π𝑤2 𝑛 2𝜌𝑙𝐶𝑈
3/2
exp 1 2 𝑛𝑤2 𝑙𝐶𝑈 < 𝑤 > = 8𝑙𝐶𝑈 𝜌𝑛 = 8𝑆𝑈 𝜌𝑛 𝑄 𝑒ω = 𝑒ω 𝜌 𝑑𝑝𝑡𝜄
n dω θ
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Numerical Methods : Monte Carlo simulation
Pills of Physics of molecules in vacuum : some hypothesis… Ideal Gas Molecular Flow 𝑸𝑾 = 𝑶𝒍𝑪𝑼 The molecules in the chamber move independently of each other. P·d < 10-2 mbar · cm Pumping speed vs sticking factor 𝒘𝒒𝒕 = 𝒈𝒃𝒅𝒇𝒖 𝒃𝒔𝒇𝒃 ∗ 𝒃𝒘𝒇𝒔𝒃𝒉𝒇 𝒏𝒑𝒎𝒇𝒅𝒗𝒎𝒇 𝒕𝒒𝒇𝒇𝒆 ∗ 𝒕𝒖𝒋𝒅𝒍𝒋𝒐𝒉 𝒈𝒃𝒅𝒖𝒑𝒔 𝟓
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Calculation of Pressure Profiles and conductances Analytical Methods Numerical Methods
- No universal formulas
- Only simple geometry
- No simplification is needed
Numerical Methods : Monte Carlo simulation
MOLFLOW + a Test Particle Monte-Carlo code developed at CERN allows import of stl files From steady state to time-dependent simulation
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From official Drawings.. ..to 3D CAD (Inventor…)… ..and STL file for Molflow Simulation
Numerical Methods : Monte Carlo simulation
Chamber walls are described by planar polygons (facets)
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Numerical Methods : Molflow+
Pumping speed or Sticking factor Desorption value Time depending pressure profile
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1 2 3 4 5 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 x 10
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Time [s] Pressure [mbar] Fit He Simulated values He
Numerical Methods : Monte Carlo simulation
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1 2 3 4 5 6 7 8 1 2 3 x 10
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Time [s] Pressure [mbar] He Ne Ar Kr Xe Rn
Numerical Methods : Monte Carlo simulation
1 2 3 4 5 6 7 8 0.5 1 1.5 2 2.5 3 x 10
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Time [s] Pressure [mbar] Kr Xe Rn
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50 100 150 200 250
- 0.05
0.00 0.05 0.10 0.15 0.20 0.25 0.30
Transmission Probability [%] Molecular mass [g/mol]
Equation y =(x)^A
- Adj. R-Square 0.99719
Value Standard Error T.P. (%) A
- 0.94306
0.00978
Numerical Methods : Monte Carlo simulation
𝜏𝑈.𝑄. =
1 𝑜 1 − 𝑈. 𝑄. (*)
*Y.Suetsugu, Application of the Monte Carlo method to pressure calculation
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50 100 150 200 250 0.5 1.0 1.5 2.0 2.5 3.0 3.5
Time of flight [s] Molecular mass [g/mol]
Equation y =B+(x)^A
- Adj. R-Square
0.98943 Value Standard Error tof (s) A 0.23961 0.00576 tof (s) B
- 0.61299
0.07159
Numerical Methods : Monte Carlo simulation
𝜏𝑢𝑝𝑔.=0.01s
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On-line Sampling :
- Realized along the primary pumping system, with active carbon and
cellulose filters installed downstream of the turbomolecular pumps;
- Spectroscopy Analysis.
Experimental Analysis
Experiment 1
Filter position
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HRS31 HRS23 HRS25 HRS22 HRS24 HRS32
Filters positions
Experimental Analysis
HRS filters Date of installation: 17th June 2014 Date of removal: 13th September 2014 Number of target change in this period: 5 Type of targets: ZrO, UC2-C
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HRS 31 HRS 23
Filters positions in HRS and RFQ
HRS 32 HRS 43 HRS 42 HRS24
Experimental Analysis
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Experimental Analysis
HPGe detector:
Low relative efficiency; High energy resolution; Low work temperature (~77 K). Analyzed samples : Resolution (FWHM) of 1.79 keV to 1.33 MeV; and of 0.82 keV to 122 keV Peak/Compton ratio of 65:1.
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1 10 100 1000 10000 100000 1000000 HRS 23 HRS 24 HRS 25 HRS 31 HRS 32 HRS 42 HRS 43
Log Activity (Bq\unit) Filter Position
Po-206
Bi-206 Bi-205 Pt-188 Os-185 Ba-140 I-125 Te- 121
Some spectroscopy results
Separators zone RFQ
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Some spectroscopy results
Ech No. Activités Isotopes (Bq /unit) Incert. TP HRS 32 Filtre CA Se-75 3.6E+01 33% Sb-120 4.4E+01 20% Te-121 3.6E+02 20% Te-121m 4.4E+01 61% Te-123 8.9E+01 39% Sb-124 3.1E+02 12% I-125 3.2E+03 76% Sb-125 1.8E+02 19% Sb-126 2.0E+02 10% I-131 5.0E+01 40% Ba-140 5.1E+01 29% Os-185 1.9E+01 100% Pt-188 4.7E+01 38% Ir-189 1.4E+02 33% Au-194 3.1E+02 17% Pt-195 3.6E+02 28% Bi-205 9.0E+02 10% Bi-206 9.7E+02 8% Po-206 4.3E+02 17% Bi-207 3.3E+01 33% Ech No. Activités Isotopes (Bq /unit) Incert. TP HRS 42 Filtre CA Te-121 2.1E+01 20% Te-123 1.6E+00 57% I-125 3.3E+01 124% I-131 1.4E+00 171% Ba-140 9.2E+00 17% Os-185 4.1E+00 53% Pt-188 9.0E+00 19% Bi-205 5.1E+01 10% Bi-206 1.9E+02 7% Po-206 9.1E+01 9% Bi-207 9.8E-01 70% Ech No. Activités Isotopes (Bq /unit) Incert. TP HRS
43 Filtre
CA Te-121 3.1E+00 15% I-125 6.9E+00 92% Ba-140 7.8E+00 9% Ce-141 5.0E-01 29% Os-185 5.9E+00 12% Pt-188 1.4E+01 8% Ir-189 2.1E+01 13% Pt-195 3.7E+01 11% Hg-203 1.6E+01 13% Bi-205 1.7E+00 20% Bi-206 8.8E+00 8% Po-206 4.5E+00 18%
Before He injection After He injection
Injection stopping Cooling Accumulation extraction
…Where are the noble gases?
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What Fantasy thinks that radiation can produce:
Elements on radioactive decays
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Elements on radioactive decays
What happens in reality: e- p 𝑄∗ → 𝑄 + 𝛿
𝑎 𝐵 𝑎 𝐵
𝑄 → 𝐸 + α
2 4 𝑎−2 𝐵−4 𝑎 𝐵
𝑞 → 𝑜 + 𝛾+ + ν 𝑜 → 𝑞 + 𝛾− + ν 𝜸+ 𝜸−
Alpha Decay Gamma Decay Beta Decay Electron capture
𝑞 + 𝑓− → 𝑜 + ν
PAPER ALUMINIUM LEAD 25
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Elements on radioactive decays: Nuclides chart
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Elements on radioactive decays: Nuclides chart
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Some example
121I 205Bi 121Te 185Os
ε
121Xe
β+
205Po
β+
205At
β+ β+
205Rn
α
209Rn 185Ir
β+
185Pt
β+ β+
185Hg
β+
185Au 140Cs 140Ba
β-
140Xe
β-
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Future step
Qualitative to quantitative analysis:
- Use of Monte Carlo simulations to evaluate transmission
probability in different position (filters);
- Comparison with spectroscopic results;
- Application of the tool to HRS and GPS filters analysis.
Use of a Tape Station to:
- analyze ACTIVITY and evaluate the TIME OF FLIGHT of different
gas species (spectroscopy);
- TEST the accuracy of Monte Carlo model (time dependent mode).
Experiment 2
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Future steps
Tape station
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1 2 3 4 5 6 7 10 20 30 40 50 60 70
Beta counts Time after proton impact [s]
1 2 3 4 5 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5 x 10
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Time [s] Pressure [mbar] Fit He Simulated values He
Future experimental steps
6He 4He
Courtesy of A. Gottberg
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Conclusions
This work open different ways to be explored: Monte Carlo Analysis: Molflow+ simulation of Noble gases behavior in GPS and evaluation of transmission probability and time of arrival; Use of time-dependent mode; Tool application to HRS and experimental benchmarking (next step); Try to take the RFQ into account (next tech. student?). Spectroscopic analysis: HRS: Activity decrease from frontend to main switchyard; Analysis of GPS and hall filters (next step);
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Special thanks to:
- Giovanna Vandoni (TE/VSC-IVM)
- J. Vollaire, A. Dorsival, N. Riggaz, S. Castelli, (DGS/RP-AS)
- R. Kersevan and M. Ady (TE/VSC-IVM)
- A. Gottberg , T. Stora (EN/STI-RBS Isolde Target Group)
- J.A. Ferreira Somoza, H. Rambeau, P. Chiggiato, R. Catherall, M. Lozano,
- S. Marzari, V. Barozier, H. Montano.
- Friederike, Ida, Maria (Girls open space support group!)
Acknowledgments
TE/VSC and DGS/RP