A Comprehensive Study of Spallation Models for Proton-Induced Spallation Product Yields Utilized in Transport Calculation

A Comprehensive Study of Spallation Models for Proton-Induced Spallation Product Yields Utilized in Transport Calculation

EPJ Web of Conferences 239, 06001 (2020) https://doi.org/10.1051/epjconf/202023906001 ND2019 A comprehensive study of spallation models for proton-induced spallation product yields utilized in transport calculation 1, 1, 1, Hiroki Iwamoto ∗, Shin-ichiro Meigo , and Hiroki Matsuda 1J-PARC Center, Japan Atomic Energy Agency, 2-4, Shirakata, Tokai-mura, Naka-gun, Ibaraki 319-1195, Japan Abstract. In order to understand the current status of the predictive performance of spallation models and issues towards further improvement, a comprehensive study of the proton-induced spallation product yields was con- ducted. In this study, four kinds of the latest spallation models (i.e. INCL++/ABLA07, INCL++/GEMINI++, INCL4.6/GEM, and CEM03.03), utilized in Monte Carlo particle transport calculation, are employed, and six pieces of cross section data measured at GSI, RIKEN, and J-PARC are used for comparison. As a result, the INCL++/ABLA07 calculations are in general agreement with the GSI and RIKEN experimental data, whereas some discrepancies are observed especially in the comparisons with the J-PARC experiments. Finally, several key issues inherent in each spallation model are described. 1 Introduction et al. [15], was employed. The INCL4.6/GEM and CEM03.03 calculations were performed by the use of nu- In the neutronic and shielding design of high-energy accel- clear reaction calculation options of the Particle and Heavy erator facilities such as accelerator-driven systems (ADSs) Ion Transport code System (PHITS) version 3.08 and the and spallation neutron sources, spallation models imple- general-purpose Monte Carlo N-Particle code (MCNP) mented in Monte Carlo particle transport codes [1-4] version 6.1, respectively. The calculated cross sections provide us the information of spallation product yields, were compared with experimental data measured at GSI as well as energy spectra and angular distributions of sec- [16-19], RIKEN [20], and J-PARC [21] as listedin ondary particles. Although an exhaustive benchmark anal- Table 2, where the GSI data were taken from the EX- ysis was conducted under the auspices of the International change FORmat (EXFOR) experimental nuclear reaction Atomic Energy Agency (IAEA) [5 ] and a great deal of database [22]. effort has been devoted to improving the spallation mod- Table 1. Spallation models used. els, discrepancies with experimental data, especially for the spallation product yields, still have been reported in model name INC deexcitation recent analyses [6,7 ]. To understand the current status of the predictive per- INCL++/ABLA07 INCL++ (ver.6.0) ABLA07 formance of the spallation models and their issues to- INCL++/GEMINI++ INCL++ (ver.6.0) GEMINI++ wards further improvement, a comprehensive study for the INCL4.6/GEM INCL (ver.4.6) GEM proton-induced spallation product yields was conducted. CEM03.03 CEM03.03 GEM2 Experimental data used for comparison. 2 Method Table 2. target E (MeV) institute reference no. In this study, the proton-induced nuclide production cross p 208Pb 1000 GSI [16] sections were calculated using different kinds of spal- 238U 1000 GSI [17,18] lation models based on the intranuclear cascade (INC) 136Xe 1000 GSI [19] plus deexcitation model (i.e., INCL++/ABLA07 [8,9], 137Cs 185 RIKEN [20] INCL++/GEMINI++ [10], INCL4.6/GEM [11,12], and 209Bi 400 J-PARC [21] CEM03.03 [13]), which are summarized in Table1. Here 209Bi 3000 J-PARC [21] CEM03.03 contains the deexcitation model GEM devel- oped by Furihata [12], in which some parameters were modified to account for fission cross sections; this model is referred to as GEM2 [14]. For the calculations by 3 Results and discussion INCL++/ABLA07 and INCL++/GEMINI++, a stand-alone 3.1 Comparison with GSI data for 208Pb and 238U nuclear reaction simulation code, developed by Mancusi, Figures 1 and 2 illustrate the calculated mass number ∗e-mail: [email protected] distributions of the spallation products for the p(1 GeV) © The Authors, published by EDP Sciences. This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/). EPJ Web of Conferences 239, 06001 (2020) https://doi.org/10.1051/epjconf/202023906001 ND2019 Figure 1. Comparison of mass number distribution between the GSI experiment and the model calculations for p(1 GeV) + 208Pb reaction. Figure 3. Two-dimensional η distribution between the GSI experiment and model calculations for the p(1 GeV) + 208Pb reaction (top panel: INCL++/ABLA07, upper panel: Figure 2. Same as Figure 1, but for p(1 GeV) + 238U reaction. INCL++/GEMINI++, lower panel: INCL4.6/GEM, bottom panel: CEM03.03). 208 238 + Pb and p(1 GeV) + U reactions, respectively, to- the experimental data (η) for each (A, Z) value: gether with experimental data measured at GSI with the inverse-kinematics technique. Here, we classify the spal- η(A, Z) sgn σ (A, Z) σ (A, Z) ≡ calc − expt lation products into four groups according to their pro- 2 σ(calc(A, Z) σexpt(A, Z) ) duction mechanisms: light charged particle (LCP), inter- − , (1) · σ (A, Z) mediate mass fragment (IMF), fission fragment (FF), and ( expt ) evaporation residue (ER). A single Gaussian-like hump where A and Z denote the mass and proton (or charge) for mass numbers from 50 to 130 in Figure 1 and that numbers of the spallation products, respectively; σcalc and for mass numbers from 60 to 150 in Figure 2 indicate σexpt represent the calculated and experimental nuclide FFs. Meanwhile, the spallation products at mass numbers production cross sections, respectively. higher than FFs indicate ERs. For both FFs and ERs, con- Figure 3 displays the two-dimensional η distribu- siderable discrepancies can be observed between the ex- tion between the GSI experimental data and the model perimental data and the model calculations. For IMFs, no calculations for the p(1 GeV) + 208Pb reaction, where p experimental data are found in EXFOR for the (1 GeV) the red and blue colors denote “overestimation” and “un- + 208Pb reaction; however, Figure 2 suggests that IMFs derestimation”, respectively, whereas the white color in- are presumably produced from the spallation reactions, for dicates “agreement”. It is seen from the top panel which only ABLA07 appears to account for the IMF pro- that INCL++/ABLA07 broadly reproduces the experimental duction. data. In contrast, blue, white, and red colored stripes are To understand the discrepancies observed in Figures observed in the ER region for the upper and lower pan- 1 and 2 in detail, we define an index of difference from els, and the opposite stripe is seen in the bottom panel. 2 EPJ Web of Conferences 239, 06001 (2020) https://doi.org/10.1051/epjconf/202023906001 ND2019 Figure 1. Comparison of mass number distribution between the Figure 5. Comparison of mass number distribution between the GSI experiment and the model calculations for p(1 GeV) + 208Pb GSI experiment and the model calculations for p(1 GeV) + 136Xe reaction. reaction. Figure 3. Two-dimensional η distribution between the GSI Figure 4. Same as Figure 3, but for p(1 GeV) + 238U reaction. experiment and model calculations for the p(1 GeV) + 208Pb reaction (top panel: INCL++/ABLA07, upper panel: Figure 2. Same as Figure 1, but for p(1 GeV) + 238U reaction. INCL++/GEMINI++, lower panel: INCL4.6/GEM, bottom panel: CEM03.03). This means that INCL++/GEMINI++ and INCL4.6/GEM es- timate ERs as neutron rich for the same Z number, whereas + 208Pb and p(1 GeV) + 238U reactions, respectively, to- the experimental data (η) for each (A, Z) value: CEM03.03 estimates ERs as neutron poor for the same Z gether with experimental data measured at GSI with the number, implying that parametrizations in GEMINI++, inverse-kinematics technique. Here, we classify the spal- η , σ , σ , (A Z) sgn calc(A Z) expt(A Z) GEM, and GEM2, would not match those of INCL++, lation products into four groups according to their pro- ≡ − σ( (A, Z) σ (A, Z) 2) INCL4.6, and CEM, respectively. Furthermore, as pointed duction mechanisms: light charged particle (LCP), inter- calc expt − , (1) out in Iwamoto et al. [6,23], it is seen in this figure that mediate mass fragment (IMF), fission fragment (FF), and · σexpt(A, Z) ( ) INCL4.6/GEM overall underestimates FFs. evaporation residue (ER). A single Gaussian-like hump where A and Z denote the mass and proton (or charge) for mass numbers from 50 to 130 in Figure 1 and that numbers of the spallation products, respectively; σcalc and Figure ?? shows the two-dimensional η distribution for mass numbers from 60 to 150 in Figure 2 indicate σexpt represent the calculated and experimental nuclide between the GSI experimental data and the model cal- FFs. Meanwhile, the spallation products at mass numbers production cross sections, respectively. culations for the p(1 GeV) + 238U reaction. The trends higher than FFs indicate ERs. For both FFs and ERs, con- Figure 3 displays the two-dimensional η distribu- of η distributions are similar to the case of the 208Pb tar- siderable discrepancies can be observed between the ex- tion between the GSI experimental data and the model get; that is, INCL++/ABLA07 shows overall in good agree- perimental data and the model calculations. For IMFs, no calculations for the p(1 GeV) + 208Pb reaction, where ment with the experimental data, and INCL++/GEMINI++ experimental data are found in EXFOR for the p(1 GeV) the red and blue colors denote “overestimation” and “un- and INCL4.6/GEM estimate ERs as neutron rich for the + 136 + 208Pb reaction; however, Figure 2 suggests that IMFs Figure 6. Same as Figure 3, but for p(1 GeV) Xe reaction.

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