Low and medium energy deuteron-induced reactions on {}^{63,65}Cu nuclei

Low and medium energy deuteron-induced reactions on Cu nuclei

E. Šimečková simeckova@ujf.cas.cz    P. Bém    M. Honusek    M. Štefánik Euratom/IPP.CR Fusion Association, Nuclear Physics Institute, 25068 Řež, Czech Republic    U. Fischer    S.P. Simakov Euratom/FZK Fusion Association, Karlsruhe Institute of Technology (KIT), Hermann-von-Helmholtz-Platz, 1, 76344 Eggenstein-Leopoldshafen, Germany    R.A. Forrest Nuclear Data Section, International Atomic Energy Agency, A-1400 Vienna, Austria    A.J. Koning Nuclear Research and Consultancy Group, P.O. Box 25, NL-1755 ZG Petten, The Netherlands    J.-C. Sublet Euratom/UKAEA Fusion Association, Culham Centre for Fusion Energy, Abingdon OX14 3DB, United Kingdom    M. Avrigeanu mavrig@ifin.nipne.ro    F.L. Roman    V. Avrigeanu “Horia Hulubei” National Institute for Physics and Nuclear Engineering, P.O. Box MG-6, 077125 Bucharest-Magurele, Romania
July 16, 2019
Abstract

The activation cross sections of , , , and reactions on Cu were measured in the energy range from 4 to 20 MeV using the stacked-foils technique. Then, following the available elastic-scattering data analysis that provided the optical potential for reaction cross sections calculations, an increased effort has been devoted to the breakup mechanism, the direct reaction stripping, and the pre-equilibrium and compound-nucleus cross section calculations, corrected for the breakup and stripping decrease of the total reaction cross section. The overall agreement between the measured and calculated deuteron activation cross sections proves the correctness of the nuclear mechanisms account, next to the simultaneous analysis of the elastic-scattering and reaction data.

pacs:
24.10.Eq,24.10.Ht,25.45.-z,25.45.De,25.45.Hi,27.50.+e

I Introduction

Among the projects of powerful neutron sources for nuclear energy generation, the International Fusion Material Irradiation Facility (IFMIF) requests high accuracy deuteron evaluated nuclear data for the assessment of induced radioactivity of the accelerator components, targets and beam stoppers. The IFMIF facility needs such data for estimation of the potential radiation hazards from the accelerating cavities and beam transport elements (Al, Fe, Cr, Cu, Nb) and metal and gaseous impurities of the Li loop (Be, C, O, N, Na, K, S, Ca, Fe, Cr, Ni) in the energy range from the threshold up to 40 MeV. However, it is known that the actual experimental and evaluated data for deuteron-induced reactions are less extensive and accurate than for neutrons, so that further measurements and improved model calculations are needed.

The weak binding energy of the deuteron, =2.224 MeV, is responsible for the high complexity of the interaction process that involves a variety of reactions initiated by the neutrons and protons coming from deuteron breakup. Such a wide diversity of nuclear reactions initiated by deuteron interaction with nuclei has hampered so far the comprehensive analysis involving large A-range of targets and incident-energy domain. The difficulties to interpret the deuteron-induced reaction data in terms of the usual reaction mechanism models have recently been investigated bem08 (); ma09 (); bem09 (); ma10a (); ma10b (); es10 (), looking for a consistent way to also include the breakup contribution within the activation cross section calculations. Second, the total reaction cross sections are less accurately described since, unlike the nucleon case, there are no global optical model potentials (OMP) which describe the scattering data over a wide range of nuclei and energies sufficiently well. Therefore, a simultaneous analysis of the deuteron elastic scattering ma09 () and induced activation bem09 (), which appears essential for the IFMIF engineering design, is extended in the present work for the Cu target nuclei.

Ii Measurements

ii.1 Samples and irradiations

Isotope T E I
(keV) (%)
Zn 244.26 d 1115.5 50.6
Cu 12.7 h 1345.8 0.473
Zn 9.186 h 596.6 26
548.4 15.3
Ni 2.5172 h 1481.8 24
Zn 38.47 min 669.6 8
962.1 6.5
Cu 5.12 min 1039.2 9
Table 1: Half-lives, main gamma lines and their intensities of the measured isotopes chu99 ().

The variable energy NPI cyclotron provides protons and deuterons in energy range 11-37 MeV and 11-20 MeV, respectively. The irradiation was carried out using an external deuteron beam of the NPI cyclotron U-120M operating in the negative-ion mode of acceleration. From the stripping-foil extractor the beam was delivered to the reaction chamber through a beam line consisting of one dipole and two quadrupole magnets.

The incident deuteron energy was determined by computational procedure based on measured trajectory (the frequency and actual extraction radius) of acceleration. This procedure was experimentally tested using the activation foil method and the surface-barrier-detector technique. The energy was determined with a resulting accuracy of 1.0%, the FWHM spread of the incident beam up to 1.8% was observed.

The activation cross sections induced by deuterons bombarding high purity natural aluminum and copper foils were measured by a stacked-foil technique. A collimated deuteron beam strikes the stack of foils in a Faraday-cup-like reaction chamber enabling the cooling of stacked foils without a lost of accuracy in the beam current and charge monitoring (10%). To enlarge the number of energy bins in the measured excitation functions and to check the internal consistency of the measured data, the foils were stacked with different Al vs Cu sequences in two independent runs. The stock of eleven Al and eleven Cu foils placed alternately was bombarded by a deuteron beam of initial deuteron energy 19.95 MeV, with mean beam current 90 nA during an exposure time of 15 min. The initial deuteron energy, the beam current and the irradiation time for the second run were 20.18 MeV, 330 nA and 5 min, respectively. The aluminum cross section data were reported earlier bem09 ().

To enable the measurement of the relatively short-living isotopes Zn (T=38.47 min) and Cu (T=5.12 min), three extra runs were carried out. The initial deuteron energy was 19.79, 20.09 and 19.79 MeV, the beam current was 0.24, 0.36 and 0.17 A and the irradiation time was 6, 5 and 9.3 min, respectively. The thickness of the high purity natural Cu and Al foils (purity of 99.99%, Goodfellow product) was 25 and 50 m, respectively. Foils were weighted (with a 2% uncertainty) to avoid the relatively large uncertainties in the foil thickness declared by the producer. The mean deuteron energy and energy thickness were determined using the SRIM 2003 code zieg03 (). The overall thickness of the available 22 foil stacks covers the excitation-curve range from 20 to full beam stop.

In preliminary reports bem08 (); es10 (), different initial energies were reported due to errors in the orbit calculation of the cyclotron operated in the negative-ion mode of acceleration. In the present report, corrected energy values 19.95 and 20.18 MeV for the first two runs were established and the relevant energies and energy thicknesses of each foil were recalculated.

Energy Reaction
(MeV) CuCu CuZn CuZn CuCu CuZn CuNi
1.49 (149) 13.3 (16)
4.25 (86) 85.9 (91) 9.7 (12)
4.56 (79) 1.70 (19) 123 (14)
5.29 (75) 195 (23) 92 (11)
5.96 (67) 1.58 (17) 282 (33)
6.00 (66) 258 (32)
6.92 (63) 214 (24) 243 (25)
7.13 (60) 8.29 (92) 322 (36)
7.69 (59) 253 (33) 445 (53)
8.21 (54) 42.0 (48) 290 (37)
9.00 (53) 216 (28) 531 (55)
9.09 (50) 103 (12) 284 (37)
9.65 (51) 218 (26) 675 (81)
9.91 (47) 155 (18) 261 (32)
10.07 (47) 165 (23) 239 (34)
10.78 (47) 182 (23) 683 (80)
11.36 (45) 188 (25) 862 (102) 0.101 (29)
11.55 (42) 248 (30) 207 (24)
12.25 (41) 281 (36) 196 (23)
12.37 (43) 161 (17) 795 (83)
12.39 (41) 269 (52) 179 (24)
12.90 (41) 157 (21) 880 (104) 0.200 (42)
13.69 (39) 327 (41) 165 (20)
13.82 (39) 147 (16) 940 (95) 0.355 (73)
14.31 (37) 134 (16) 355 (46) 166 (25) 909 (109) 0.435 (59)
15.02 (36) 353 (83) 136 (19)
15.17 (37) 133 (15) 949 (95) 0.502 (64)
15.62 (35) 367 (53) 138 (19)
15.63 (36) 114 (14) 911 (107) 0.632 (94)
16.17 (34) 380 (47)
16.44 (35) 117 (12) 0.018 (4) 901 (91) 0.750 (83)
16.87 (34) 93 (11) 0.067 (36) 851 (100) 0.70 (11)
17.37 (33) 109 (17)
17.38 (32) 374 (55) 111 (14)
17.64 (33) 103 (11) 0.253 (28) 816 (82) 0.92(10)
17.89 (32) 382 (54) 103 (13)
18.05 (33) 91 (11) 0.645 (89) 817 (98) 1.09 (17)
18.78 (32) 102 (12) 1.44 (15) 790 (82) 1.32 (18)
19.01 (30) 366 (66) 91.6 (122)
19.17 (31) 84 (11) 2.28 (28) 730 (88) 1.27 (18)
19.49 (30) 350 (59) 89.7 (105)
19.49 (29) 316 (79)
19.88 (30) 97 (12) 3.72 (38) 694 (71) 1.47 (21)
Table 2: Measured reaction cross sections (mb) for deuterons incident on the Cu nuclei. The mean deuteron energy and resolution due to the thickness and straggling of each foil are shown. Statistical uncertainties are given in parentheses for the cross sections in units of the last digit.

ii.2 Calculation of cross sections and their errors

The gamma-rays from the irradiated foils were measured repeatedly by two calibrated HPGe detectors of 23 and 50% efficiency and of FWHM 1.8 keV at 1.3 MeV. To provide reliable corrections for the decay, the beam-current recorder and -ray spectrometer were synchronized in time. Activated isotopes were identified (see Table 1) using nuclear decay data from Ref. chu99 (). The measurements with different cooling times lasted up to 100 days after irradiation. By analyzing the spectra, the resulting activities at the end of irradiation were obtained. The uncertainty of 3% includes statistical errors and the uncertainty of the detector-efficiency calibration.

In the case of short-lived isotope measurements, the irradiated Cu foils were immediately measured by the HPGe detector with 50% efficiency. To reduce the dead time rate caused by the strong annihilation peak accompanying -decay, the observed Cu foil was situated within two iron slides of 1 mm thickness and a lead plate of 10 mm thickness was placed between the measured foil and the HPGe detector. The detector efficiency was recalibrated according to the experimental conditions using a calibrated Eu radioactive source with an uncertainty of detector efficiency of 5%.

The experimental cross sections, given in Table 2, are shown in Fig. 1 and compared with previously measured data jlg63 (); cbf70 (); ho71 (); st06 (); ko07 (); fwp66 (); st01 (); mn06 (); nb63 (). Their systematic errors are composed of current uncertainty (10%), uncertainty of foil thickness (2%) and uncertainty of detector efficiency determination (2% and 5%, respectively). The mean statistical error in activity determination was 2%. Uncertainty of initial energy determination was 1%, energy spread of incident beam up to 1.8%. Only energy thicknesses are shown in Fig. 1.

CuCu. As the natural copper has two stable isotopes, the generation of Cu by irradiation of natural copper may proceed via three contribution reactions: Cu (with the threshold E=0 MeV), Cu (E=3.767 MeV), and Cu (E=12.512 MeV). Therefore, even for deuteron energies below 20 MeV, we have to take into account all contributions and to report the measured data to the natural copper as shown in Fig. 1(a).

CuCu is the only possible reaction generating Cu isotope by deuteron irradiation on natural copper. These data are shown in Fig. 1(b).

CuZn. There is only one possible way to generate Zn in the energy region up to 20 MeV, the experimental excitation function is shown in Fig. 1(c).

CuZn. The Zn isotope can originate in the Cu reaction, and also in the Cu reaction. The radioactive capture reaction cross sections are known to be very small (of the order of a few hundred b or less). Hence, the Cu reaction would not be expected to contribute appreciably to the measured yield of Zn [see Fig. 1(d)].

CuZn is the only possible reaction to generate Zn in energy region up 20 MeV. The cross sections are shown in Fig. 1(e).

CuNi reaction is the only possible way for generation of the Ni. Our cross section data (see Fig. 1(f)) are the first experimental values except the one value around the deuteron energy of 19 MeV.

Overall, the present experimental data are in satisfactory agreement with the previous measurements jlg63 (); cbf70 (); ho71 (); st06 (); ko07 (); fwp66 (); st01 (); mn06 (); nb63 () within one standard deviation except for the oldest data of Ref. jlg63 () and several data of Ref. cbf70 ().

Iii Energy–dependent optical potential

The description of the deuteron-nucleus interaction represents an important test for both the quality of reaction mechanism models and the evaluation of nuclear data. The simultaneous analysis of the deuteron elastic scattering and induced activation should really involve a consistent input of nuclear model calculations bem09 (); ma10a (); ma10b (), a prime interest for the optical model potential (OMP) parameters being motivated by their further use in the analysis of all deuteron interaction cross sections.

Figure 1: (Color online) Comparison of previous measured data jlg63 (); cbf70 (); ho71 (); st06 (); ko07 (); fwp66 (); st01 (); mn06 (); nb63 () and within this work (full circles), the evaluated data within the TENDL-2010 library TENDL () (dotted curves), and calculated results obtained with TALYS-1.2 code using either the whole default input (dash-dotted) or the replacement of default deuteron OMP by that of the present work (dashed), for the deuteron interaction with Cu.
         Potential depths Geometry parameters
                (MeV)                  (fm)
V=88.5+0.88Z/A-0.26E r=1.17
a=0.734, E14.5
    =0.709+0.0017E, E14.5
W=-0.014+0.0948E r=1.325
a=0.810
W=13.6,               E12 r=1.325
     =15.27-0.142E, 12E35 a=0.770, E12
     =10.3,               E35     =0.583+0.0156E, 12E14.5
    =0.810, E14.5
V=7.33-0.029E r=1.07
a=0.66
Table 3: The parameters of the deuteron optical potential for the Cu target nuclei. A star used as superscript follows the parameters which were changed with respect to the optical potential of Daehnick et al. dah ().
Figure 2: (Color online) Comparison of (left) measured EXFOR_el () deuteron elastic-scattering angular distributions for Cu and calculated values obtained by using the OMP parameters given in Table 3 (solid curves), the global OMP dah () (dot-dashed curves), and TALYS TALYS () default option (dashed curves), and (right) measured EXFOR-TCS () reaction cross sections for deuterons incident on Cu and calculated values obtained by using the same above-mentioned potentials as well as the evaluated data within the TENDL-2010 library TENDL () (dotted curve). Comparison of particular parameters given in Table 3 (solid curves) and of Daehnick et al. dah () OMP (dot-dashed lines) are also shown in the lower part of the right hand side.

Unfortunately, the few measurements of angular distributions of elastic scattered deuterons on Cu EXFOR_el () do not allow an extended OMP analysis. However, while previous OMP analyses on Li ma05 (); ma06a (), Al ma09 (); bem09 (), Fe ma08 (), Co and Nb ma10c () show that no global OMP describes sufficiently well the elastic scattering data in the energy range up to 20 MeV, but the few parameters adjustment (Table 3) of the Daehnick et al. dah (); RIPL3 () OMP led to a good description of the data for the Cu target nuclei. The comparison of the experimental elastic-scattering angular distributions for Cu EXFOR_el () and the calculated values obtained by using the presently adjusted OMP parameters, the global optical potential dah (), and the widely-used TALYS code TALYS () default option based on the Watanabe folding approach wat58 () (dashed curves) are shown in Fig. 2. At the same time the measured reaction cross sections for deuterons incident on the Cu isotopes and natural Cu EXFOR-TCS () are compared in Fig. 2 with the calculated values obtained by using the same potentials as well as the evaluated data within the TENDL-2010 library TENDL (). One may note that the last two calculated excitation functions underestimate the measured values by at least 20%. Finally, the present real-potential diffusibility, imaginary surface-potential depth and diffusibility, and imaginary volume-potential depth are compared with the same OMP parameters of Daehnick et al. dah (). The elastic-scattering cross section calculations have been performed using the computer code SCAT2 SCAT2 ().

The particular importance of the deuteron OMP for the activation cross section calculations can be seen in Fig. 1 through the comparison between the experimental data and the calculated results obtained using both the present deuteron OMP and the corresponding TALYS default option, as well as the TENDL-2010 library TENDL () data. There are thus compared the calculated cross sections obtained using the default input of TALYS, i.e. the Watanabe folding approach wat58 () for the deuteron OMP, with the results following the replacement of this OMP by the parameter set given in Table 3. The differences are obvious while it can also be seen that this replacement still does not lead to a satisfactory description of the experimental activation data. Improvements of the theoretical analysis by taking into account all reaction mechanisms involved in the interaction process are thus additionally needed.

Iv Deuteron breakup

iv.1 Phenomenological approach

The interaction of deuterons with the target nuclei proceeds largely through direct reaction (DR) processes, for deuteron energies below and around the Coulomb barrier, while with increasing incident energy reaction mechanisms like pre-equilibrium emission (PE) or evaporation from the fully equilibrated compound nucleus (CN) also become important. On the other hand, the breakup mechanism is responsible for the enhancement of a large variety of reactions along the whole incident-energy range and thus its contribution to the activation cross sections has to be explicitly taken into account bem09 (); ma10a (); ma10b ().

The physical picture of the deuteron breakup in the Coulomb and nuclear fields of the target nucleus considers two distinct chains, namely the elastic breakup (EB) in which the target nucleus remains in its ground state and none of the deuteron constituents interacts with it, and the inelastic breakup or breakup fusion (BF), where one of these deuteron constituents interacts with the target nucleus while the remaining one is detected. An empirical parametrization of the total proton-emission breakup fraction =/ and the elastic-breakup fraction =/ have previously been obtained ma09 () on the basis of experimental systematics pamp78 (); wu79 (); klein81 (); mats82 (); must87 (). Thus, proton-emission spectra and angular distributions from deuteron-induced reactions on nuclei from Al to Pb at incident energies from 15 to 80 MeV have been studied in this respect. However, an energy range of only 15-30 MeV has been available for the empirical elastic-breakup fraction / systematics klein81 (); must87 (). Their dependence on the charge (Z), atomic number (A) of the target nucleus, and deuteron incident energy (E) was found to be ma09 ():

(1)
(2)

A comparison with the total proton- and neutron-emission breakup cross section parametrization of Kalbach kalb03 ():

(3)

shows that the former parametrization ma09 () considers equal breakup fractions for proton and neutron emission, but also gives all breakup components, i.e. the proton-emission breakup total, elastic, and inelastic fraction =-. The energy dependence of the total, elastic, and inelastic proton-emission breakup cross sections following Ref. ma09 () as well as the total proton-emission breakup cross sections kalb03 () for the deuteron interactions with the Cu nuclei are shown in Fig. 3. It turns out that, for deuteron incident energies above 8 MeV, the predictions for the total proton-emission breakup cross sections given by both parameterizations are rather close. However, at the lowest energies the total proton-emission breakup cross section provided by the latter parametrization kalb03 () become larger than the deuteron total reaction cross section.

Figure 3: (Color online) Energy dependence of the total (solid curve), elastic (dash-dotted) and inelastic (dot-dashed) proton-emission breakup cross sections given by Ref. ma09 () and total proton-emission breakup cross sections of Ref. kalb03 () (dotted), for the deuteron interactions with Cu. The corresponding total reaction cross section is shown by dash-dot-dotted curve.

Concerning the energy dependence of the inelastic- and elastic-breakup components, the interest of the deuteron activation cross sections for incident energies up to 60 MeV has motivated an additional check of the elastic-breakup parameterization ma09 () extension beyond the energies formerly considered for the derivation of its actual form. Actually, as it is shown in Fig. 4 for the Cu target nucleus, the elastic-breakup cross sections given by the empirical parameterization ma09 () decrease with the incident energy beyond the energy range within which it was established. On the other hand, this trend is opposite to that of the total-breakup cross section. Thus, in the absence of any available experimental deuteron elastic-breakup cross section at incident energies above 30 MeV, the correctness of an eventual extrapolation should be checked by comparison of the related predictions with results of an advanced theory such as the Continuum-Discretized Coupled-Channels (CDCC) method kamimura86 (); aust87 ().

iv.2 Phenomenological EB versus CDCC formalism

A detailed description of the CDCC formalism is available elsewhere kamimura86 (); aust87 (); piya99 (); moro06 (); moro09b (); moro09c (), and hence only a brief description of the method is given in the following.

The breakup component is treated within the CDCC formalism as an inelastic excitation of the projectile due to the nuclear and Coulomb interactions with the target nucleus. Consideration of this excitation is performed through the coupling of the projectile unbound excited states in the solution of the scattering problem by means of the coupled channels approach. The deuteron scattering process is analyzed within a three-body model, comprising the two-body projectile and the target, by the model Hamiltonian aust87 ():

(4)

Here is the interaction between the neutron and proton kamimura86 (), assumed to have a Gaussian shape

(5)

where =72.15 MeV and =1.484 fm , were determined from the fit of the deuteron binding energy. The vector is the proton-neutron relative coordinate, is the coordinate of the center of mass of the - pair relative to the target nucleus. and are the proton-target and neutron-target interactions, respectively, usually taken as the central nuclear part of the proton and neutron phenomenological OMPs at half the deuteron incident energy, . Adjusted Koning-Delaroche KD03 () neutron and proton global OMPs, in order to obtain a suitable description of the deuteron elastic-scattering, have been used maCDCC10 (). The operators and are the kinetic energies associated with and .

A finite set of coupled equations is obtained by the introduction of the discretization procedure in which the continuum spectrum, truncated at a maximum excitation energy () and divided into a set of energy (or relative momentum) intervals, is represented by a finite and discrete set of square-integrable functions. Each bin, is represented by a single square-integrable function, calculated by averaging the scattering states for the - relative motion within the bin width. Moreover, the - relative angular momentum is also restricted by considering only a limited number of partial waves, in order to deal with a finite set of coupled equations. Finally, the three-body scattering wave function is expanded over the internal states of the deuteron as follows:

(6)

where is the ground-state wave function and () are the averaged (within each bin) continuum wave functions. The radial functions describe the projectile-target relative motion for the elastic and breakup components. Continuum states with orbital angular momentum , 1 and 2 for the - relative motion were considered. The proton and neutron intrinsic spins were ignored for simplicity within calculations that were performed with the coupled-channels code FRESCO thompson88 ().

Figure 4: (Color online) Energy dependence of the phenomenological ma09 () (dashed curve) and CDCC (solid line) elastic-breakup cross sections for deuteron interactions with the Cu nucleus maCDCC10 (). The solid circle corresponds to Kleinfeller systematics klein81 () while there is also shown the total proton-emission breakup cross section (dotted curve).

The energy dependence of the elastic-breakup cross sections provided by the excitation of the continuum spectrum, in the case of the deuteron interaction with Cu target nucleus, is compared with the prediction of empirical systematics ma09 () in Fig. 4. The elastic-breakup cross sections corresponding to the Kleinfeller et el. systematics (Table 3 of Ref. klein81 ()) are also shown. The agreement of the CDCC elastic-breakup cross sections and the latter systematics can be considered as validation of the present advanced model approach. Moreover, the comparison shown in Fig. 4 points out that the CDCC calculations lead to elastic-breakup cross sections which follow the total-breakup cross section behavior as well as that of the reaction cross section shown in Fig. 3. Therefore the present analysis makes clear that the empirical parameterization extension for the elastic-breakup cross sections beyond the energies considered in this respect should be done with caution maCDCC10 (). The CDCC method thus provides useful initial guidance for the assessment of these extrapolation accuracies and may help to improve the existing phenomenological approaches. However, additional experimental deuteron interaction data, like elastic-scattering angular distributions and inclusive neutron and proton spectra, are needed in order to validate the parameters involved in the CDCC and complete the systematics of the elastic- and total-breakup cross sections over enlarged energy and target mass domains.

iv.3 Inelastic-breakup enhancement of the deuteron activation cross sections

Overall, the deuteron total-breakup cross section should be subtracted from the total reaction cross section that is shared among different statistical–emission channels. On the other hand, the inelastic-breakup processes, where one of deuteron constituents interacts with the target leading to a secondary composite nucleus, bring contributions to different reaction channels. The secondary–chance emission of particles from the original d-target interaction is therefore especially enhanced. Thus, the absorbed proton or neutron following the breakup emission of a neutron or proton, respectively, contributes to the enhancement of the corresponding and reaction cross sections. In order to calculate this breakup enhancement for, e.g., the reaction cross sections, firstly the inelastic-breakup cross sections were obtained in the present work by subtracting also the CDCC elastic-breakup cross sections from the phenomenological total-breakup cross sections given by Eq. (1). Next, they have been bem09 (); ma10a (); ma10b (); es10 () multiplied by the ratios / corresponding to the above-mentioned reactions of the absorbed proton with the target nucleus, where is the proton reaction cross section and stands for or outgoing channels bem09 (). These ratios have been expressed as a function of the deuteron incident energy using the Kalbach kalb07 () formula for the center-of-mass system centroid energy of the deuteron-breakup peak energies of the emitted constituents:

(7)

In a similar way have been obtained also the inelastic-breakup contributions to the and activation cross section due to the neutrons absorbed in further interactions with the target nucleus, i.e. by the , and reactions, respectively. The only difference has consisted in replacing the above-mentioned ratios / by the ratios /, where the non-elastic cross section plays the same role for neutrons as for protons.

Figure 5: (Color online) (a) The centroid of assumed Gaussian line shape kalb07 () for deuteron breakup-peak energies of emitted neutrons (solid) and protons (dash-dotted), and the corresponding values (dashed) calculated for deuterons interacting with Cu. (b) The convolution of the cross section ratio / for the target nucleus Cu (dash-dotted curve) with the Gaussian line shape of the deuteron-breakup peak energies of the corresponding emitted protons, for deuterons with energies of 8, 20 and 30 MeV (solid curves, with the incident energy noted above their maxima), and the convolution results at each deuteron energy (dashed curves).

However, the assumed Gaussian line shape of the deuteron-breakup peak energies of the emitted constituents, that are also showed in Fig. 5(a) for neutrons, have quite large widths. Since the broad approximation of this method adopted previously bem09 () for estimation of the breakup enhancement, a better estimation is considered in the present work. It consists in a convolution of either the ratio / or / with the Gaussian line shape of the deuteron-breakup peak energies of the corresponding emitted constituent, for a given deuteron incident energy. The cases of deuterons with energies of 8, 20 and 30 MeV are shown in Fig. 5(b) together with the cross section ratio /. There are also shown the convolution results at each of these energies, while their area corresponds to the inelastic-breakup enhancement of the reaction cross sections at these energies. These results are more physical, with a realistic incident-energy dependence except only for the case involving the higher-emission energy side of the Gaussian line shape of the deuteron-breakup peak energies. This happens for, e.g., deuterons with energies lower than 8 MeV, shown for the reaction case in Fig. 5(b). Since this side of the Gaussian line shape could be narrower kalb07 (), different widths for the two halves of the Gaussian distribution should be eventually adopted, while otherwise some overestimation may result from using a single width. However, the corresponding reaction cross sections at these energies are just above the reaction threshold so that we have taken into account the inelastic-breakup enhancement of the reaction cross sections only above these energies.

V One-nucleon transfer reactions

Apart from the breakup contributions to deuteron interactions, the direct reaction mechanisms like stripping and pick-up have to be properly considered in order to describe the low energy side of the , and excitation functions ma09 (); bem09 (); ma10a (); ma10b (); es10 (); ma10c (). In the present work the DR contribution to the and reaction reaction cross sections, through population of the low-lying discrete levels of Cu residual nuclei, was calculated using the code FRESCO thompson88 () based on the Coupled–Reaction Channels (CRC) method. The post form distorted-wave transition amplitude with finite-range interaction has been chosen.

v.1 The one-nucleon stripping

The reaction has been in a large extent of critical importance for the study of nuclear structure. Actually, the spectroscopic factors extracted from the analysis of experimental angular distributions of the corresponding emitted protons did contribute to the validation of the nuclear shell model, considering that the neutron from the deuteron is transferred to a single-particle state of the residual nucleus. Consequently, the rich systematics of the achieved experimental spectroscopic factors makes possible the calculation of almost total stripping cross–section contribution to the deuteron activation cross section.

The above-mentioned deuteron phenomenological OMP parameter set (Table 3) has been used for the incident channel, while the Koning–Delaroche KD03 () OMP global parameters have been used for protons interactions with the residual nuclei. The - interaction in the deuteron has been described with the potential given by Eq. (5) and the neutron bound states were generated in a Woods–Saxon real potential with the global values of a reduced radius of 1.25 fm and diffuseness of 0.65 fm, while its depth has been adjusted to reproduce the nucleon binding energies in the residual nuclei.

The present calculations of the single-neutron stripping reaction cross section have involved transitions to 104 final states of the odd-odd residual nucleus Cu and to 81 final states of the similar residual nucleus Cu. The spectroscopic factors that were obtained experimentally from proton angular-distribution measurements for these states up to 5 MeV, as given in Table II of Ref. park63 (), Table I of Ref. park65 (), and NDS108 (); NDS111 (), have been considered in this respect. One may note that a lower number of final states, i.e. 63 for Cu and 52 for Cu, extending up to 3 MeV, were used within a preliminary stage of this work ma10a (), which made necessary an additional assumption concerning the DR contribution from the states at higher energies. The present increase of the final states taken into account for the DR contribution to the reaction cross sections makes a similar assumption no longer necessary. In spite of the corresponding results being rather close to the former ones ma10a (), an increased accuracy is now obtained for this activation component, even better than 5%.

The resulted stripping components of the reaction excitation functions are essential for the description of the experimental data shown in Fig. 6. This statement is valid also concerning the maxima of these excitation functions at deuteron incident energies 8 MeV.

v.2 The one-nucleon pick-up

The excitation function corresponding to Cu nucleus production from deuterons incident on a natural copper target includes contributions from both stripping Cu and pick-up Cu direct reaction mechanisms. Actually, the lowest energy side of a excitation function, between its threshold and those of the and reactions, can be described exclusively by the pick-up reactions as it is shown, e.g., in Fig. 3 of Ref. ma10c ().

Therefore, we have used in the present work the above-mentioned deuteron phenomenological OMP to describe the incident channel of the reaction, in a similar way to the stripping calculation, while the Becchetti and Greenlees RIPL3 (); BG () OMP has been used for the emitted tritons.

The - interaction in triton has been described with a He potential 3He-pot () of Woods-Saxon shape:

(8)

where the parameters =77.71 MeV, =1.008 fm and =0.75 fm were determined by a fit of the 5.50 MeV He binding energy (relatively close to 6.3 MeV corresponding to H). The transfered–neutron bound states were also generated in a Woods-Saxon real potential, with global reduced radius of 1.25 fm, diffuseness of 0.65 fm, and the depth adjusted to the nucleon binding energies in the residual nuclei. The experimental spectroscopic factors obtained by analysis of triton angular distributions related to the population of 14 discrete levels of the residual nucleus Cu NDS108 () have been used for calculation of the pick-up transition amplitude.

The contribution thus obtained of the Cu reaction to the Cu production excitation function, corrected for the isotopic ratio Cu/Cu, is shown in Fig. 6(a). As expected ma10c (), the activation cross sections is the essential contribution among the processes induced by deuterons on the Cu isotope, within the natural copper target, at incident energies between 7-20 MeV. The statistical emission through the and reactions, also shown in Fig. 6(a), become significant at higher energies.

Vi Statistical particle emission

The reaction mechanisms such as pre-equilibrium emission (PE) or evaporation from the fully equilibrated compound nucleus (CN), become important when the incident energy is increased above the Coulomb barrier, when the interaction of deuterons with the target nuclei proceeds largely by DR processes. The related cross sections have been analyzed in this work by using the default model parameters (except for the deuteron OMP in Table 3) of the widely-used computer code TALYS as well as a local consistent parameter set developed in calculations with the PE+CN code STAPRE-H ma95 () taking into account also the breakup and DR results discussed above.

The local analysis results obviously have a higher accuracy while the global predictions may be useful for an understanding of unexpected differences between measured and calculated cross sections. The main assumptions and parameters involved in this work for the sets of global and local calculations have recently been described elsewhere va08 (), only some points specific to the mass range A60 are given here. A further note should concern the fact that similar input parameter sets and calculations have been used to obtain the breakup-enhancement due to one of deuteron constituents interacting with the target nucleus and leading to a secondary composite nucleus, with final contributions to different reaction channels as discussed in Sec. IV.

The deuteron phenomenological optical model parameter set given in Table 3 has been used for the incident channel. The nucleon optical potential of Koning and Delaroche KD03 (), used by default in the TALYS code, has obviously been the first option. However, a basic point revealed by these authors is that their global potential does not reproduce the minimum around the neutron energy of 1–2 MeV for the total neutron cross sections of the 60 nuclei. Following also their comment on the constant geometry parameters which may be responsible for this aspect, we have applied the SPRT method jpd76 () for determination of the OMP parameters over a wide neutron energy range through analysis of the - and -wave neutron strength functions, the potential scattering radius and the energy dependence of the total cross section . The recent RIPL-3 recommendations RIPL3 () for the low–energy neutron scattering properties and the available measured data have been used in this respect, and we found that it is necessary to consider the energy dependence of the real potential geometry at lower energies given in Ref. va08 ().

These potentials were also used for the calculation of the collective inelastic scattering cross sections by means of the direct–interaction distorted–wave Born approximation (DWBA) method and a local version of the computer code DWUCK4 pdk84 (). The weak coupling model was adopted for the odd nuclei Mn and Cu using the collective state parameters of Kalbach ck00 (). Typical ratios of the direct inelastic scattering to the total reaction cross sections in the energy range from few to 60 MeV decrease from 11 to 5%, for the Mn nucleus, and from 8 to 3% for the Cu isotopes.

The OMP of Koning and Delaroche was also considered for the calculation of proton transmission coefficients on the residual nuclei, i.e. the isotopes of Cu and Ni, while a previous trial of this potential concerned the proton reaction cross sections rfc96 (). Actually our local analysis involved the isotopes of Mn, Fe, Co, Ni, Cu and Zn, for lower energies important in statistical emission from excited nuclei. In order to obtain the agreement with the corresponding data we have found it necessary to replace the constant real-potential diffusivity by the energy–dependent form =0.463+0.01 up to 20 MeV for Ni, where the energy is in MeV and the diffusivity is in fm. A final validation of both the original OMP and the additional energy–dependent has been obtained by analysis of the available ) and reaction data up to 12 MeV on Ni isotopes while the other statistical model parameters are the same as in the rest of the present work.

The optical potential which is used in this work for calculation of the -particle transmission coefficients was established previously va94 () for emitted -particles, and supported recently by semi–microscopic analysis for 90 nuclei ma06b (). On the other hand, by comparison of the present calculations and measured data EXFOR () for the target nuclei Cu we found that the real well diffuseness of the above–mentioned global OMP should be changed to 0.67 fm. This reduction is rather similar to that found necessary for the target nuclei Co, and Ni vs04 (). Moreover, a final remark concerns the fact that the same OMP parameter sets were employed within both the PE generalized ma95 () Geometry-Dependent Hybrid (GDH) model mb83 (), and the CN statistical model.

The nuclear level densities were derived on the basis of the back-shifted Fermi gas (BSFG) formula hv88 (), for the excitation energies below the neutron-binding energy, with small adjustments of the parameters and va02 () obtained by a fit of more recent experimental low-lying discrete levels ensdf () and -wave nucleon resonance spacings RIPL3 (). Above the neutron binding we took into account the washing out of shell effects within the approach of Ignatyuk et al. avi75 () and Junghans et al. arj98 (), and using the method of Koning and Chadwick ajk97 () for fixing the appropriate shell correction energy. A transition range from the BSFG formula description to the higher energy approach has been chosen between the neutron binding energy and the excitation energy of 15 MeV, mainly in order to have a smooth connection. On the other hand, the spin distribution has been determined by a variable ratio of the nuclear moment of inertia to its rigid-body value, between 0.5 for ground states, 0.75 at the neutron binding energy, and 1 around the excitation energy of 15 MeV. Concerning the particle-hole state density which for the PE description plays the same role as the nuclear-level density for statistical model calculations, a composite formula ma98 () was used within the GDH model with no free parameters except for the -particle state density = MeV eg81 ().

The modified energy–dependent Breit–Wigner (EDBW) model dgg79 (); mav87 () was used for the electric dipole -ray strength functions of main importance for calculation of the -ray transmission coefficients. The corresponding values have been checked within the calculations of capture cross sections of Mn and Cu isotopes in the neutron energy range from keV to 3–4 MeV, by using the OMP and nuclear level density parameters described above and global estimations chj77 () of the -ray strength functions for multipoles 3. Thus we found that the strength functions corresponding to the experimental RIPL3 () average radiative widths provide an accurate description of the capture data for the Cu isotopes. Finally, the accuracy of the -ray strength functions adopted in this work is also shown by the above–mentioned analysis of the reaction cross sections.

Formally, no free parameter is involved for the PE description within the corresponding generalized GDH model except for -particle emission, the above-mentioned s.p.l.-density and the pre-formation probability eg81 () with a value of 0.2 used in the present work. However, a particular comment concerns the initial configuration of excited particles () and holes (), for deuteron-induced reactions in the present case. Similar careful studies klein81 (); must87 (); pamp78 (); hiw87 () pointed out that - or - may be a suitable choice for this configuration. Our calculations show that the latter one gives the best agreement between the measured and calculated reaction cross sections.

Figure 6: (Color online) Comparison of measured data already shown in Fig. 1 and present analysis results (solid) taking into account the deuteron inelastic breakup (dashed), the DR (dash-dotted for reactions and short dash-dotted for reaction), and the PE+CN (dotted and short-dotted for reaction) mechanism contributions to the deuteron interaction with Cu target nuclei.

Vii Results and discussion

The comparison of the measured and calculated reaction cross sections of Cu is shown in Fig. 6, including the present experimental data already shown in Fig. 1, and the global and local analysis results. For the local analysis both components of the final activation are shown, i.e. the DR cross sections provided by the code FRESCO and the PE+CN contributions supplied by STAPRE-H. The latter is alone rather close to the TALYS predictions. The local approach has led to much better agreement with the present reaction data bem08 (); es10 () especially due to the stripping DR contribution.

In order to obtain a complete description of the reaction cross sections, we have started by taking into account also the neutrons which, following the breakup proton emission, are absorbed in further interactions with the target nucleus. The cross section ma08 () has been considered in this respect (Fig. 5) as well as the corresponding fraction leading to the above-mentioned reactions. These fractions have been obtained by using the ratios of the most recently evaluated mbc06 () and reaction cross sections, respectively, to the neutron reaction cross sections provided by the neutron global OMP KD03 (). A similar procedure has been followed in order to obtain the contribution to the and reaction cross sections due to the protons which, following the breakup neutron emission, are absorbed in further interactions with the target nucleus and described by the cross section . The only difference in this case concerns the reaction cross sections in the incident energy range up to 30 MeV, which have been obtained by PE+CN calculations using the computer code STAPRE-H and the consistent local parameter set described above. All intermediary and ultimate reaction cross sections shown in Fig. 6(c-e) indicate that they may contribute up to 50% of the activation cross sections for deuteron incident energies of 25 MeV.

The contribution due to the breakup proton, added to the PE+CN components provided by STAPRE-H, describe rather well the measured cross sections of the reaction as shown in Fig. 6(f). Similarly, the breakup neutron emission plays the same role for the reaction as shown in Fig. 6(c,d). Their weight is obviously increasing with the incident energy since all reactions involved, following the deuteron breakup, within the second step of these processes have negative Q-values.

Finally, all activation data of deuteron-induced reactions on Cu have been properly described, making obvious the usefulness of the concurrent description of all reaction channels as well as the simultaneous analysis of the deuteron elastic scattering and induced activation. A particular underprediction has concerned however the CuCu reaction cross sections, only their energy dependence being well described. A first comment may concern in this respect the fact that, although the TALYS and TENDL calculations do include a breakup component in all and reaction channels, the systematical relations for its strength does not show enough predictive power in this particular case. On the other hand, also the lower number of the known spectroscopic factors corresponding to the discrete states of the odd-odd residual nucleus Cu, taken into account for the DR contributions, may explain this underprediction.

Viii Summary

The cross section values for deuteron-induced reactions on natural Cu were determined for the reactions CuCu, CuCu, CuZn, CuZn, CuZn and CuNi at deuteron energies up to 20 MeV. Resulting cross section data are in good agreement with the major part of previous reported experiments.

Following a previous extended analysis of elastic-scattering, breakup and direct-reactions of deuterons on Cu, for energies from 3 to 60 MeV ma10a (), the pre-equilibrium and statistical emissions have been considered in the same energy range. The related cross sections have been analyzed by using the default model parameters (except for the deuteron OMP in Table 3) of the widely-used computer code TALYS as well as a local consistent parameter set developed in calculations with the PE+CN code STAPRE-H taking into account also the breakup and DR results formerly discussed. The local approach has led to much better agreement with the present reaction data especially due to the model calculation of the stripping DR contribution.

Consideration of the deuteron breakup plays a key role for the reaction channels adding a second emitted particle to the first one. Thus, in order to obtain a complete description of the , , , and reaction cross sections, we have taken into account also the neutrons which, following the breakup proton emission, are absorbed in further interactions with the target nucleus. Finally, all deuteron-induced reactions on Cu, including the present data measured at 20 MeV deuteron energy, have been properly described due to a simultaneous analysis of the elastic-scattering and reaction data. A similar analysis will be further considered for a systematical evaluation of the deuteron activation of other medium-mass nuclei.

Acknowledgments

The authors are indebted to the operating crew of the U-120M cyclotron for their ready assistance. This work was partly supported by the MTI CR under contract No. 2A-1TP1/101, by the European Communities within the framework of the European Fusion Development Agreement under Contracts of Association between EURATOM and Forschungszentrum Karlsruhe, IPP.CR, and UKAEA, the Karlsruher Institüt für Technologie (KIT) Order No. 320/20459037/INR-NK, and the CNCSIS-Bucharest under Contract PN-II-ID-PCE-2008-2-448.

References

  • (1) P. Bém, L. Bittmann, V. Burjan, U. Fischer, M. Götz, M. Honusek, V. Kroha, J. Novák, S. Simakov, and E. Šimečková, in: Proc. Int. Conf. on Nuclear Data for Science and Technology, Nice, 2007, edited by O. Bersillon et al. (EDP Sciences, Paris, 2008), p. 1003.
  • (2) M. Avrigeanu, W. von Oertzen, R. A. Forrest, A. C. Obreja, F. L. Roman, and V. Avrigeanu, Fusion Eng. Design, 84, 418(2009).
  • (3) P. Bém, E. Šimečková, M. Honusek, U. Fischer, S. P. Simakov, R. A. Forrest, M. Avrigeanu, A. C. Obreja, F. L. Roman, and V. Avrigeanu, Phys. Rev. C 79, 044610(2009).
  • (4) M. Avrigeanu and V. Avrigeanu, EPJ Web of Conferences 2, 01004 (2010).
  • (5) M. Avrigeanu and V. Avrigeanu, J. Phys: Conf. Ser. 205, 012014 (2010).
  • (6) E. Šimečková, P. Bém, M. Götz, M. Honusek, J. Mrázek, J. Novák, M. Štefánik, L. Závorka, M. Avrigeanu and V. Avrigeanu, EPJ Web of Conferences 8, 07002 (2010).
  • (7) J. F. Ziegler, J. P. Biersack, and M. D. Ziegler, SRIM-The Stopping and Range of Ions in Matter, SRIM code, http://www.srim.org .
  • (8) S. Y. F. Chu, L. P. Ekström, and R. B. Firestone, The Lund/LBNL Nuclear Data, Search Version 2.0, February 1999, http://nucleardata.nuclear.lu.se/nucleardata/toi/.
  • (9) J. L. Gilly, G. A. Henriet, M. Preciosa Alves, and P. C. Capron, Phys. Rev. 131, 1727 (1963).
  • (10) C. B. Fulmer and I. R. Williams, Nucl. Phys. A155, 40 (1970).
  • (11) H. Okamura and S. Tamagawa, Nucl. Phys. A169, 401 (1971).
  • (12) S. Takács, F. Tarkanyi, B. Kiraly, A. Hermanne, and M. Sonck, Nucl. Instr. and Meth. B 251, 56 (2006).
  • (13) K. Ochiai, M. Nakao, N. Kubota, S. Sato, M. Yamauchi, N. H. Ishioka, T. Nishitani, and C. Konno, as Ref. bem08 (), p. 1011.
  • (14) F. W. Pement and R. L. Wolke, Nucl. Phys. A86, 429 (1966).
  • (15) S. Takács, F. Tarkanyi, M. Sonck, A. Hermanne, and S. Sudar, Nucl. Instr. and Meth. B 174, 235 (2001).
  • (16) M. Nakao, J. Hori, K. Ochiai, N. Kubota, S. Sato, M. Yamauchi, N. S. Ishioka, and T. Nishitani, Nucl. Instr. and Meth. A 562, 785 (2006).
  • (17) N. Baron and B. L. Cohen, Phys. Rev. 129, 2636 (1963).
  • (18) A. J. Koning and D. Rochman, TENDL-2010: TALYS-Based Evaluated Nuclear Data Library (December 8, 2010), http://www.talys.eu/tendl-2010/.
  • (19) Experimental Nuclear Reaction Data (EXFOR); www-nds.iaea.or.at/exfor; L.L.Lee Jr, J.P.Schiffer, EXFOR C1024 entry; E.Newman et al., EXFOR C1067 entry; S.A.Hjorth et al., EXFOR C1075 entry; R. K. Jolly et al., EXFOR C1023 entry; G. Igo et al., EXFOR D0239 entry; R.Jahr et al., EXFOR D0241 entry; J.L.Yntema et al., EXFOR C1056 entry; S.Mayo et al., EXFOR D0223 entry; L.V.Dubar et al., EXFOR F0579 entry; K. Bearpark et al., EXFOR D0314 entry.
  • (20) M. Avrigeanu, W. von Oertzen, U. Fischer, and V. Avrigeanu, Nucl. Phys. A 759, 327 (2005).
  • (21) M. Avrigeanu, W. von Oertzen, H. Leeb, F. L. Roman, and V. Avrigeanu, in Proc. 11th Int. Conf. on Nuclear Reaction Mechanisms, 12-16 June 2006, Varenna, Italy (Ricerca Scientifica ed Educazione Permanente, Milano, 2006), p. 193.
  • (22) M. Avrigeanu, H. Leeb, W. von Oertzen, F. L. Roman, and V. Avrigeanu, as Ref. bem08 (), p. 2192.
  • (23) M. Avrigeanu and V. Avrigeanu, in: Proc. Int. Conf. on Nuclear Data for Science and Technology, Jeju, Koreea, 2010 (in press).
  • (24) W. W. Daehnick, J. D. Childs, and Z. Vrcelj, Phys. Rev. C 21, 2253 (1980).
  • (25) R. Capote et al., Nucl. Data Sheets 110, 3107(2009); http://www-nds.iaea.org/RIPL-3/ .
  • (26) A. J. Koning, S. Hilaire, and M. C. Duijvestijn, TALYS-1.0, as Ref. bem08 (), p. 211; version TALYS-1.2, December 2009; http://www.talys.eu/home/ .
  • (27) S. Watanabe, Nucl. Phys. 8, 484 (1958).
  • (28) S.Mayo et al., EXFOR D0223 entry; L.V.Dubar et al., EXFOR F0579 entry; K. Bearpark et al., EXFOR D0314 entry.
  • (29) O. Bersillon, Code SCAT2, Note CEA-N-2227, 1992.
  • (30) EXFOR Nuclear Reaction Data, http://www-nds.iaea.or.at/exfor, http://www.nndc.bnl.gov/nndc/exfor .
  • (31) J. Pampus, J. Bisplinghoff, J. Ernst, T. Mayer-Kuckuk, J. Rama Rao, G. Baur, F. Rosel, and D. Trautmann, Nucl. Phys. A311, 141 (1978).
  • (32) J. R. Wu, C. C. Chang, and H. D. Holmgren, Phys. Rev. C 19, 370 (1979).
  • (33) J. Kleinfeller, J. Bisplinghoff, J. Ernst, T. Mayer-Kuckuk, G. Baur, B. Hoffmann, R. Shyam, F. Rosel, and D. Trautmann, Nucl. Phys. A 370, 205 (1981).
  • (34) N. Matsuoka, M. Kondo, A. Shimizu, T. Saito, S. Nagamachi, H. Sakaguchi, A. Goto, and F. Ohtani, Nucl. Phys. A345, 1 (1980).
  • (35) M. G. Mustafa, T. Tamura, and T. Udagawa, Phys. Rev. C 35, 2077 (1987).
  • (36) C. Kalbach Walker, TUNL Progress Report XLII (2002-2003) p. 82-83, Triangle University Nuclear Laboratory; www.tunl.duke.edu/publications/tunlprogress/2003/ .
  • (37) M. Kawai, M. Kamimura, and K. Takesako, Prog. Theor. Phys. Suppl. 184, 118 (1969).
  • (38) N. Austern, Y. Iseri, M. Kamimura, M. Kawai, G. Rawitscher, and M. Yahiro, Phys. Rep. 154, 125 (1987).
  • (39) R. A. D. Piyadasa, M. Kawai, M. Kamimura, and M. Yahiro, Phys. Rev. C 60, 044611 (1999).
  • (40) A. M. Moro and F. M. Nunes, Nucl. Phys. A767, 138 (2006).
  • (41) A. M. Moro, J. M. Arias, J. Gómez-Camacho, and F. Pérez-Bernal, Phys. Rev. C 80, 054605 (2009).
  • (42) A. M. Moro, F. M. Nunes, and R. C. Johnson, Phys. Rev. C 80, 064606 (2009).
  • (43) A. J. Koning and J. P. Delaroche, Nucl. Phys. A713, 231 (2003).
  • (44) M. Avrigeanu and A. M. Moro, Phys. Rev. C 82, 037601 (2010).
  • (45) I. J. Thompson, Comput. Phys. Rep. 7, 167 (1988); v. FRES 2.3 (2007).
  • (46) C. Kalbach Walker, in: TUNL Progress Report, vol. XLVI (2007), p. 78, www.tunl.duke.edu/publications/tunlprogress/2007/tunlxlvi.pdf .
  • (47) Y. S. Park and W.W. Daehnick, Phys. Rev. 181, 1082 (1969).
  • (48) W. W. Daehnick and Y.S. Park, Phys. Rev. 180, 1062 (1969).
  • (49) Balraj Singh, Nuclear Data Sheets 108, 197 (2007).
  • (50) F. Browne and J.K Tuli, Nuclear Data Sheets 111, 1093 (2007).
  • (51) F. D. Becchetti Jr and G. W. Greenlees, Annual Report, J.H. Wiliams Laboratory, University of Minesota, 1969.
  • (52) Y. Iseri, M. Yahiro and M. Kamimura, Prog. Theor. Phys. Suppl. 89, 84 (1986).
  • (53) M. Avrigeanu and V. Avrigeanu, IPNE Report NP-86-1995, Bucharest, 1995, and Refs. therein; News NEA Data Bank 17, 22 (1995).
  • (54) J. P. Delaroche, Ch. Lagrange, and J. Salvy, IAEA-190 (IAEA, Vienna, 1976), vol. 1, p. 251.
  • (55) M. Avrigeanu, S. Chuvaev, A. A. Filatenkov, R. A. Forrest, M. Herman, A. J. Koning, A. J. M. Plompen, F. L. Roman, and V. Avrigeanu, Nucl. Phys. A806, 15 (2008).
  • (56) P. D. Kunz, DWUCK4 user manual, OECD/NEA Data Bank, Issy-les-Moulineaux, France, 1984; www.nea.fr/abs/html/nesc9872.html .
  • (57) C. Kalbach, Phys. Rev. C 62, 44608 (2000).
  • (58) R. F. Carlson, At. Data Nucl. Data Tables 63, 93 (1996).
  • (59) V. Avrigeanu, P.E. Hodgson, and M. Avrigeanu, Phys. Rev. C 49, 2136 (1994).
  • (60) M. Avrigeanu, W. von Oertzen, and V. Avrigeanu, Nucl. Phys. A 764, 246 (2006).
  • (61) V. Semkova, V. Avrigeanu, T. Glodariu, A.J. Koning, A.J.M. Plompen, D.L. Smith, and S. Sudar, Nucl. Phys. A 730 (2004) 255.
  • (62) M. Blann and H. K. Vonach, Phys. Rev. C 28, 1475 (1983).
  • (63) H. Vonach, M. Uhl, B. Strohmaier, B.W. Smith, E.G. Bilpuch, and G. E. Mitchell, Phys. Rev. C 38, 2541 (1988).
  • (64) V. Avrigeanu, T. Glodariu, A. J. M. Plompen, and H. Weigmann, J. Nucl. Sci. Tech. Suppl. 2, 746 (2002).
  • (65) Evaluated Nuclear Structure Data File (ENSDF), http://www.nndc.bnl.gov/ensdf/index.jsp .
  • (66) A. V. Ignatyuk, G. N. Smirenkin, and A. S. Tishin, Yad. Fiz. 21 (1975) 485; Sov. J. Nucl. Phys. 21, 255 (1976).
  • (67) A. R. Junghans, M. de Jong, H.-G. Clerc, A. V. Ignatyuk, G.A. Kudyaev, and K.-H. Schmidt, Nucl. Phys. A 629, 635 (1998).
  • (68) A. J. Koning and M. B. Chadwick, Phys. Rev. C 56, 970 (1997).
  • (69) M. Avrigeanu and V. Avrigeanu, Comp. Phys. Comm. 112, 191 (1998); A.Harangozo, I.Stetcu, M.Avrigeanu, and V.Avrigeanu, Phys. Rev. C 58, 295 (1998).
  • (70) E. Gadioli and E. Gadioli-Erba, Z. Phys. A 299, 1 (1981).
  • (71) D. G. Gardner and F. S. Dietrich, Report UCRL-82998, LLNL-Livermore, 1979.
  • (72) M. Avrigeanu, V. Avrigeanu, G. Cata, and M. Ivascu, Rev. Roum. Phys. 32, 837 (1987).
  • (73) C. H. Johnson, Phys. Rev. C 16, (1977).
  • (74) H. I. West, Jr., R. G. Lanier, and M. G. Mustafa, Phys. Rev. C 35, 2067 (1987).
  • (75) M. B. Chadwick, P. Obložinský, M. Herman, N. M. Greene, R. D. McKnight, D. L. Smith et al., Nucl. Data Sheets 107, 2931 (2006).
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