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thanks: Present address: Department of Science, Anne Arundel Community College, Arnold, MD 21012thanks: Present address: Research Center for Accelerator and Radioisotope Science, Tohoku University, Sendai 980-8578, Japanthanks: Present address: Kansai Institute for Photon Science, National Institutes for Quantum Science and Technology, Kyoto 619-0215, Japanthanks: Present address: Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37830

Optical model potentials for deuteron scattering off 24Mg, 28Si, 58Ni, 90Zr, 116Sn, and 208Pb at \sim100 MeV/nucleon

D. Patel Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556    D. C. Cuong Institute for Nuclear Science and Technology, VINATOM, 179 Hoang Quoc Viet, Hanoi 122772, Vietnam    K.  B. Howard Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556    U. Garg Corresponding author; email: [email protected] Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556    Dao T. Khoa Institute for Nuclear Science and Technology, VINATOM, 179 Hoang Quoc Viet, Hanoi 122772, Vietnam    H. Akimune Department of Physics, Konan University, Kobe 568-8501, Japan    G. P. A. Berg Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556    M. Fujiwara Research Center for Nuclear Physics, Osaka University, Osaka 567-0047, Japan    M. N. Harakeh ESRIG, University of Groningen, 9747 AA Groningen, The Netherlands    M. Itoh Research Center for Accelerator and Radioisotope Science, Tohoku University, Sendai 980-8578, Japan    C. Iwamoto Research Center for Nuclear Physics, Osaka University, Osaka 567-0047, Japan    T. Kawabata Department of Physics, Kyoto University, Kyoto 606-8502, Japan Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan    K. Kawase Research Center for Nuclear Physics, Osaka University, Osaka 567-0047, Japan    J. T. Matta Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556    T. Murakami Department of Physics, Kyoto University, Kyoto 606-8502, Japan    M. Yosoi Research Center for Nuclear Physics, Osaka University, Osaka 567-0047, Japan
Abstract

Angular distributions of the elastic and inelastic deuteron-nucleus scattering off 24Mg, 28Si, 58Ni, 90Zr, 116Sn, and 208Pb have been measured at a beam energy of 98 MeV/nucleon, with the goal of constraining the deuteron optical potential in this kinematical regime and to extract the reduced transition probabilities for the ground-state transitions to low-lying excited states of these nuclei. Two potential models were used in the analysis of the measured (d,d)(d,d) and (d,d)(d,d^{\prime}) data within the optical model and the distorted-wave Born approximation: the phenomenological optical model potential associated with the collective model of nuclear scattering, and the semi-microscopic double-folding model of the deuteron-nucleus potential based on a realistic density-dependent M3Y interaction. The deuteron optical potential and inelastic (d,d)(d,d^{\prime}) scattering form factors were calculated using these two potential models, allowing for a direct comparison between the potential models as well as the validation of the deduced EλE\lambda transition rates.

I Introduction

With the increasing availability of radioactive ion beams of reasonable intensities, there has been enhanced recent interest in the investigation of giant resonances (GR), which are highly collective oscillations of atomic nuclei. In particular, the isoscalar giant monopole resonance (ISGMR) in nuclei far from the stability line has the potential to make significant strides in our understanding of nuclear incompressibility, KK_{\infty}, and especially the asymmetry term, KτK_{\tau} [1]. Such measurements have to be performed in inverse kinematics, with deuterium and helium gases being the best targets available so far. While inelastic scattering of α\alpha particles has been the mainstay of such studies for a long time now [1], there has not been much work with deuterons since the mid-70’s primarily because of various experimental constraints [2, 3]. On the other hand, most of the measurements of GR with radioactive ion beams so far have employed active-target time projection chambers (AT-TPC) with deuterium as the component gas [4, 5, 6, 7]. Because of paucity of GR data with deuterons, it was important to validate in known cases the results obtained in (d,d)(d,d^{\prime}) measurements via direct comparison with results of inelastic α\alpha scattering. Such a detailed investigation was carried out by measuring small-angle inelastic deuteron scattering off 116Sn and 208Pb, and it was established that the extracted ISGMR strength distributions, using a multipole decomposition analysis similar to that done for inelastic α\alpha scattering, agree very well with those deduced from the (α,α)(\alpha,\alpha^{\prime}) data [8].

Such analyses hinge upon obtaining good-quality optical model (OM) parameters from elastic scattering data. The OM potential is widely used to generate wave functions for elastic scattering. These wave functions serve, in turn, as the door waves, widely known as the distorted waves, for the analysis of other direct reaction channels within the distorted-wave Born approximation (DWBA) or coupled-channel formalism. The inelastic scattering leading to the excitation of collective states of the target nucleus is essential for the determination of the underlying nuclear structure properties from the measured angular distributions. The nuclear interaction potential is, however, inherently complicated. Therefore, the phenomenological optical potential (OP) of a simple functional form is often employed in the OM and DWBA calculations to describe direct nuclear reactions and to extract nuclear properties from the angular distribution data. It represents a simple “effective” interaction used in the collective model of nuclear scattering [9] to describe both the elastic and inelastic scattering channels.

For elastic deuteron-nucleus scattering, the existing OM studies of the deuteron OP are mainly based on the phenomenological potential model using the Woods-Saxon (WS) functional form as described, for example, in Ref. [10]. This simple OP was successfully used to describe the elastic as well as inelastic angular distributions of deuteron scattering off heavy nuclei (A \gtrsim 40), based on the collective model of nuclear scattering [9]. However, the collective model approach seems to overestimate the (one-step) transition probabilities from the ground state to the low-lying excited states of some light nuclei. For example, as noted in Ref. [11], the OM parameter set that gives the best fit of the elastic angular distribution requires 40% lower value of the deformation parameter β2\beta_{2}, as compared to the adopted value, to reproduce the experimentally observed 21+{}^{+}_{1} angular distribution in the nucleus 16O.

In this work, we report on the elastic and inelastic deuteron-nucleus scattering measurements at the beam energy of 98 MeV/nucleon for several targets, ranging from light- to medium- and heavy-mass nuclei. The measured (d,d)(d,d) and (d,d)(d,d^{\prime}) scattering data have been analyzed within the OM and DWBA, respectively, using both the WS phenomenological potential model as well as a semi-microscopic deuteron-nucleus potential obtained in the double-folding model [12, 13, 14]. The extracted OM parameters are expected to find use in analyzing the giant resonance data with radioactive ion beams.

The experiments were performed at the ring cyclotron facility of the Research Center for Nuclear Physics (RCNP), Osaka University, Japan. The Ed=196E_{d}=196 MeV deuteron beam was scattered off six highly enriched (more than 90%) self-supporting targets listed in Table 1. Elastic and inelastic deuteron-nucleus scattering measurements were made over an angular range of θlab3.532\theta_{\rm lab}\sim 3.5^{\circ}-32^{\circ}. Each experimental angular opening (2\sim 2^{\circ}-wide) was subdivided into three parts for the analysis, each corresponding to a solid angle of 0.42 msr.

Table 1: Target specifications
Target Thickness Target Thickness
(mg/cm2) (mg/cm2)
24Mg 50.0 90Zr 4.2
28Si 58.5 116Sn 10.0
58Ni 1.5 208Pb 10.0

The scattered particles were momentum analyzed by the magnetic spectrometer Grand Raiden and focused onto the focal-plane detector system [17] consisting of two multi-wire drift chambers (MWDC) and two plastic scintillators [18]. The time-of-flight and energy-loss techniques were used for the identification of the scattered particles. Grand Raiden was used in the double-focusing mode in order to identify and eliminate practically all instrumental background from the final spectra [8]. Particle tracks were reconstructed using the ray-tracing technique described in Refs. [17, 19]. This, in turn, allowed for the reconstruction of the scattering angle. The experimental angular resolution was \sim 0.15, including the nominal broadening of the scattering angle due to the emittance of the beam and the multiple Coulomb scattering effects. Further details of the experimental and data analysis procedures have been provided in Ref. [8, 20].

II DWBA analysis based on the phenomenological OM potential

The two available global deuteron-nucleus optical potentials were developed by Daehnick et al. [10] and Bojowald et al. [21] in the 1980s using the phenomenological WS form for both the real and imaginary OP, covering the mass range of 27 \leq A \leq 238 and energy range of Ed10E_{d}\sim 10 MeV–90 MeV. The deuteron carries one unit of spin (𝒔=𝟏\mbox{\boldmath$s$}=\mbox{\boldmath$1$}) in its ground state, and this requires the inclusion of a real spin-orbit term VsV_{\ell s} into the OP. For the imaginary OP, in addition to the volume absorption WW, an imaginary surface term WDW_{D} is also included to account for the surface absorption which is significant due to the deuteron breakup [22, 23]. Thus, the total OP is determined explicitly as

U(r)=V(r)+iW(r)+iWD(r)+Vs(r)(𝒔)+VC(r),U(r)=V(r)+iW(r)+iW_{D}(r)+V_{\ell s}(r)(\mbox{\boldmath$\ell$}\cdot\mbox{\boldmath$s$})+V_{C}(r), (1)
whereV(r)\displaystyle\mbox{where}\ V(r) =\displaystyle= Vf(r,rV,aV),\displaystyle-Vf(r,r_{V},a_{V}), (2)
W(r)\displaystyle W(r) =\displaystyle= Wf(r,rW,aW),\displaystyle-Wf(r,r_{W},a_{W}), (3)
WD(r)\displaystyle W_{D}(r) =\displaystyle= 4aDWDddrf(r,rD,aD),\displaystyle 4a_{D}W_{D}{\frac{d}{dr}}f(r,r_{D},a_{D}), (4)
Vs(r)\displaystyle V_{\ell s}(r) =\displaystyle= Vs[mπc]21rddrf(r,rs,as),\displaystyle V_{\ell s}\left[\frac{\hbar}{m_{\pi}c}\right]^{2}\frac{1}{r}\frac{d}{dr}f(r,r_{\ell s},a_{\ell s}), (5)

and VC(r)V_{C}(r) is the Coulomb potential of a uniformly charged sphere of radius RC=1.3A1/3R_{C}=1.3~{}A^{1/3} fm. The functional form f is chosen in the WS form for all the terms

f(r,ri,ai)=[1+exp(rriA1/3ai)]1.f(r,r_{i},a_{i})=\left[1+\exp\left(\frac{r-r_{i}A^{1/3}}{a_{i}}\right)\right]^{-1}. (6)

The phenomenological OM potential given by Eqs. (1)-(6) is used in the OM analysis of the measured elastic (d,d)(d,d) scattering data, and to generate the distorted waves for the DWBA description of the inelastic (d,d)(d,d^{\prime}) scattering data. The associated OM parameters were obtained from a χ2\chi^{2}-minimization fit to the elastic (d,d)(d,d) data using the code ECIS97 [24], and they are given explicitly in Table 2. The global deuteron OPs [10, 21] were used for the parameter initialization in the χ2\chi^{2} search.

Table 2: Best-fit parameters of the phenomenological OP (1)-(6). Because of spin convention, the VsV_{\ell s} value must be divided by 2 when used in the numerical input of the code ECIS97 [24]. The errors were deduced from the weight of each parameter in the covariant multi-parameter χ2\chi^{2}-search, with rVr_{V} and VsV_{\ell s} kept fixed during the search.

Target 208Pb 116Sn 90Zr 58Ni 28Si 24Mg
VV (MeV) 46.54±0.0146.54\pm 0.01 44.33±0.0144.33\pm 0.01 42.95±0.1342.95\pm 0.13 39.07±0.1439.07\pm 0.14 35.58±0.1335.58\pm 0.13 31.92±0.1331.92\pm 0.13
rVr_{V} (fm) 1.18 1.18 1.18 1.18 1.18 1.18
aVa_{V} (fm) 0.938±0.0010.938\pm 0.001 0.911±0.0010.911\pm 0.001 0.997±0.0130.997\pm 0.013 0.914±0.0040.914\pm 0.004 0.911±0.0130.911\pm 0.013 0.977±0.0040.977\pm 0.004
WW (MeV) 20.59±0.0120.59\pm 0.01 20.87±0.0320.87\pm 0.03 20.20±0.2020.20\pm 0.20 21.41±0.2021.41\pm 0.20 22.67±0.1322.67\pm 0.13 24.39±0.1424.39\pm 0.14
rWr_{W} (fm) 1.160±0.0011.160\pm 0.001 1.070±0.0011.070\pm 0.001 1.060±0.0131.060\pm 0.013 1.100±0.0191.100\pm 0.019 0.850±0.0010.850\pm 0.001 1.000±0.0121.000\pm 0.012
aWa_{W} (fm) 0.361±0.0020.361\pm 0.002 0.670±0.0020.670\pm 0.002 0.538±0.0120.538\pm 0.012 0.456±0.0040.456\pm 0.004 0.420±0.0050.420\pm 0.005 0.501±0.0030.501\pm 0.003
WDW_{D} (MeV) 7.00±0.017.00\pm 0.01 7.00±0.017.00\pm 0.01 7.90±0.197.90\pm 0.19 7.60±0.197.60\pm 0.19 7.95±0.047.95\pm 0.04 7.50±0.147.50\pm 0.14
rDr_{D} (fm) 1.230±0.0011.230\pm 0.001 1.110±0.0011.110\pm 0.001 1.100±0.0191.100\pm 0.019 1.050±0.0201.050\pm 0.020 1.000±0.0041.000\pm 0.004 1.022±0.0051.022\pm 0.005
aDa_{D} (fm) 0.790±0.0010.790\pm 0.001 1.080±0.0011.080\pm 0.001 0.997±0.0060.997\pm 0.006 1.030±0.0151.030\pm 0.015 0.980±0.0010.980\pm 0.001 0.920±0.0030.920\pm 0.003
VsV_{\ell s} (MeV) 4.22 4.22 4.22 4.22 4.22 4.22
rsr_{\ell s} (fm) 1.150±0.0011.150\pm 0.001 1.130±0.0011.130\pm 0.001 1.200±0.0011.200\pm 0.001 1.190±0.0171.190\pm 0.017 1.130±0.0151.130\pm 0.015 1.163±0.0031.163\pm 0.003
asa_{\ell s} (fm) 1.230±0.0011.230\pm 0.001 1.110±0.0131.110\pm 0.013 0.985±0.0020.985\pm 0.002 1.110±0.0121.110\pm 0.012 1.110±0.0201.110\pm 0.020 1.164±0.0131.164\pm 0.013

The OM results obtained using the best-fit OP parameter set are shown as dashed lines in Figs. 1 and 2, in comparison with elastic (d,d)(d,d) scattering data measured at Ed=196E_{d}=196 MeV for the targets under study.

Refer to caption
Figure 1: Elastic (d,d)(d,d) scattering data measured at Ed=196E_{d}=196 MeV (in ratio to the corresponding Rutherford cross sections) for 24Mg, 28Si, and 58Ni targets (solid points). The dashed and solid lines are the OM results given by the phenomenological OP (1)-(6) and hybrid folded OP (13)-(18), respectively.
Refer to caption
Figure 2: The same as Fig. 1 but for 90Zr, 116Sn, and 208Pb targets.

The DWBA analysis of inelastic deuteron-nucleus scattering data is restricted to the direct one-step excitation of a collective state of the target, neglecting the contributions of indirect two- or three-step transitions and the channel coupling effects. The (d,d)(d,d^{\prime}) scattering cross section is calculated using the following DWBA inelastic scattering amplitude [25]:

TDWBA=[χ(𝒌,𝒓)]dA|VdA|dAχ+(𝒌,𝒓)d3rd3r,T_{\rm DWBA}=\int\left[\chi^{-}(\mbox{\boldmath$k$}^{\prime},\mbox{\boldmath$r$}^{\prime})\right]^{*}\langle dA^{\prime}|V_{d-A}|dA\rangle\chi^{+}(\mbox{\boldmath$k$},\mbox{\boldmath$r$})d^{3}rd^{3}r^{\prime}, (7)

where the distorted waves χ±\chi^{\pm} are generated by the OP (1)-(6). The transition matrix element of the deuteron-nucleus interaction dA|VdA|dA\langle dA^{\prime}|V_{d-A}|dA\rangle is dubbed as the inelastic scattering form factor (FF). A widely adopted method is to obtain the nuclear inelastic scattering FF by radially deforming nuclear part of the OP, based on the collective vibrational (or rotational) model of nuclear scattering [9]. For the (d,d)(d,d^{\prime}) scattering to a 2λ2^{\lambda}-pole collective excited state of target, the inelastic scattering FF is determined as

Fλ(r)\displaystyle F_{\lambda}(r) =\displaystyle= FN(λ)(r)+Fs(λ)(r)(𝒔)+FC(λ)(r),\displaystyle F^{(\lambda)}_{N}(r)+F^{(\lambda)}_{\ell s}(r)(\mbox{\boldmath$\ell$}\cdot\mbox{\boldmath$s$})+F^{(\lambda)}_{C}(r), (8)
FN(λ)(r)\displaystyle F^{(\lambda)}_{N}(r) =\displaystyle= δλ(N)ddr[V(r)+iW(r)+iWD(r)],\displaystyle\delta^{(N)}_{\lambda}\frac{d}{dr}[V(r)+iW(r)+iW_{D}(r)], (9)
Fs(λ)(r)\displaystyle F^{(\lambda)}_{\ell s}(r) =\displaystyle= δλ(N)ddrVs(r).\displaystyle\delta^{(N)}_{\lambda}\frac{d}{dr}V_{\ell s}(r). (10)

Prescription (9)-(10) is known as the deformed optical potential (DOP) method to generate the inelastic nuclear scattering FF. The spin-orbit contribution (10) to the total (d,d)(d,d^{\prime}) cross section is minor, but it helps to better reproduce the observed oscillation pattern of inelastic (d,d)(d,d^{\prime}) cross section for medium mass targets. For an isoscalar excitation, the nuclear deformation length δλ(N)\delta^{(N)}_{\lambda} is usually assumed to be the same as the proton deformation length δλ(p)\delta^{(p)}_{\lambda}, determined from the reduced transition rate B(Eλ)B(E\lambda\uparrow) [25] as

δλ(p)=4πB(Eλ)/e23ZRAλ1,RA=1.3A1/3fm.\delta^{(p)}_{\lambda}=\frac{4\pi\sqrt{B(E\lambda\uparrow)/e^{2}}}{3ZR_{A}^{\lambda-1}},\ R_{A}=1.3A^{1/3}\ \mbox{fm}. (11)

The Coulomb inelastic FF in Eq. (8) can be approximately obtained in a “model independent” form [25]:

FC(λ)(r)=4πB(Eλ)e(2λ+1)rλ+1.F^{(\lambda)}_{C}(r)=\frac{4\pi\sqrt{B(E\lambda\uparrow)}\ e}{(2\lambda+1)r^{\lambda+1}}. (12)

Thus, the OP parameters (1)-(6) and the reduced transition rate B(Eλ)B(E\lambda\uparrow) of the target excitation are the main inputs for the DWBA analysis of inelastic (d,d)(d,d^{\prime}) scattering using the collective model of nuclear scattering [9] associated with the phenomenological OP). The DWBA calculation of the (d,d)(d,d^{\prime}) scattering cross section has been done using two choices of the B(Eλ)B(E\lambda):

i) B(Eλ)B(E\lambda\uparrow) is fixed to the experimentally adopted transition rates [26, 27, 28], denoted as B(Eλ)adoptedB(E\lambda)_{\rm adopted} in Table 3;

ii) B(Eλ)B(E\lambda\uparrow) is deduced from the best DWBA fit of the calculated (d,d)(d,d^{\prime}) cross section to the (d,d)(d,d^{\prime}) scattering data and denoted as B(Eλ)DOPB(E\lambda)_{\rm DOP} or B(Eλ)DFMB(E\lambda)_{\rm DFM} in Table 3.

Table 3: Experimentally adopted values for the reduced electric transition rates B(E2)B(E2\uparrow) [26, 27], B(E3)B(E3\uparrow) [28], and the best-fit transition rates B(Eλ)DOPB(E\lambda)_{\rm DOP} and B(Eλ)DFMB(E\lambda)_{\rm DFM} deduced from the DWBA analysis of the (d,d)(d,d^{\prime}) data using the inelastic FF based on the phenomenological OP and that based on the hybrid folded deuteron-nucleus potential, respectively. The errors were estimated from those of the measured angular distributions.
Target ExE_{x} λπ\lambda^{\pi} B(Eλ)adoptedB(E\lambda)_{\rm adopted} B(Eλ)DOPB(E\lambda)_{\rm DOP} B(Eλ)DFMB(E\lambda)_{\rm DFM}
(MeV) (e2e^{2} bλ) (e2e^{2} bλ) (e2e^{2} bλ)
24Mg 1.368 2+2^{+} 0.0432 (11) 0.0284 (14) 0.0410 (21)
28Si 1.779 2+2^{+} 0.0326 (12) 0.0196 (10) 0.0326 (16)
58Ni 1.454 2+2^{+} 0.0695 (20) 0.0695 (35) 0.0695 (35)
90Zr 2.186 2+2^{+} 0.061 (4) 0.0641 (32) 0.0641 (32)
2.748 33^{-} 0.098 (5)a 0.0510 (37) 0.0640 (32)
0.037 - 0.079 b
116Sn 1.293 2+2^{+} 0.209 (6) 0.241 (12) 0.240 (12)
2.266 33^{-} 0.132 (18) c 0.142 (7) 0.160 (8)
0.112 - 0.202 b
208Pb 2.610 33^{-} 0.611 (9) c 0.611 (31) 0.642 (32)
0.419 - 0.836 b

aadopted from (e,e)(e,e^{\prime}) data

b from inelastic nucleon- and light-ion scattering data

c adopted from Coulomb excitation data

Refer to caption
Figure 3: The inelastic (d,d)(d,d^{\prime}) scattering data measured at Ed=196E_{d}=196 MeV (solid points) for the excitation of 21+{}^{+}_{1} states of 24Mg, 28Si, 58Ni targets, and 31{}^{-}_{1} state of 208Pb target. The DWBA results given by the collective model FF (8)-(12) based on the adopted B(Eλ)adoptedB(E\lambda)_{\rm adopted} and best-fit B(Eλ)DOPB(E\lambda)_{\rm DOP} values (see Table 3) are shown as dashed and solid lines, respectively.

The DWBA description of inelastic (d,d)(d,d^{\prime}) scattering data measured for the excitation of 21+{}^{+}_{1} states of 24Mg, 28Si, 58Ni targets, and 31{}^{-}_{1} state of 208Pb target given by the collective-model inelastic FF (8)-(12) is shown in Fig. 3. As can be seen, the 31{}^{-}_{1} angular distribution measured for 208Pb target is reproduced well with the adopted B(E3)adoptedB(E3)_{\rm adopted} value [28]. However, the DWBA description of the measured 21+{}^{+}_{1} cross section using the adopted B(E2)B(E2) value, B(E2)adoptedB(E2)_{\rm adopted}, seems to get worse for light 24Mg and 28Si nuclei, where the calculated (d,d)(d,d^{\prime}) cross section overestimates data at small angles, and then becomes non-oscillatory for angles above \sim 25. The best DWBA fit to inelastic (d,d)(d,d^{\prime}) data given by the collective-model FF requires B(E2)DOPB(E2)_{\rm DOP} value of around 40% lower than B(E2)adoptedB(E2)_{\rm adopted} value. This likely indicates a deficiency of the collective model of nuclear scattering [9] based on the phenomenological OP (1)-(6) for light-mass nuclei, as also found earlier for 16O in Ref. [11].

Refer to caption
Figure 4: Inelastic 116Sn(d,d)(d,d^{\prime}) scattering data (solid points) measured at Ed=196E_{d}=196 MeV for the excitation of the 21+{}^{+}_{1} and 31{}^{-}_{1} states of 116Sn target. The DWBA results given by the collective model FF (8)-(12) based on the adopted B(Eλ)adoptedB(E\lambda)_{\rm adopted} and best-fit B(Eλ)DOPB(E\lambda)_{\rm DOP} values (see Table 3) are shown as dashed and solid lines, respectively.
Refer to caption
Figure 5: The same as Fig. 4 but for inelastic 90Zr(d,d)(d,d^{\prime}) scattering data.

The DWBA has been proven to be a reliable approximation for the direct reaction studies at energies around or above 100 MeV/nucleon. Therefore, a good agreement of the (d,d)(d,d^{\prime}) cross section calculated in the DWBA with (d,d)(d,d^{\prime}) data measured for 21+{}^{+}_{1} and 31{}^{-}_{1} states of target must be a prerequisite for the validation of the phenomenological OP (1)-(6). In the present work, the DWBA analysis of inelastic deuteron scattering off 90Zr and 116Sn targets was chosen as test ground for the phenomenological deuteron-nucleus OP. The DWBA results obtained for 116Sn and 90Zr targets are shown in Figs. 4 and 5, respectively. At variance with light targets, the DWBA cross sections given by the collective model inelastic FF based on the best-fit OP and adopted B(E2)adoptedB(E2)_{\rm adopted} values [26, 27] agree well with the measured 21+{}^{+}_{1} angular distribution for both 90Zr and 116Sn targets. The best DWBA fit yields B(E2)DOPB(E2)_{\rm DOP} values around 5% and 15% larger than B(E2)adoptedB(E2)_{\rm adopted} values for 90Zr and 116Sn, respectively (see Table 3).

The situation is different, on the other hand, for the 31{}^{-}_{1} angular distributions measured for these targets. While the DWBA calculation using the collective model inelastic FF based on the adopted B(E3)adoptedB(E3)_{\rm adopted} value [28] describes well the (d,d)(d,d^{\prime}) data measured for the 31{}^{-}_{1} state of 116Sn, the same prescription overestimates the 31{}^{-}_{1} angular distribution measured for the 90Zr target over the whole angular range. Given B(E3)adopted0.098e2B(E3)_{\rm adopted}\approx 0.098\ e^{2}b3 adopted from (e,e)(e,e^{\prime}) data, and the empirical B(E3)B(E3) values of 0.037 to 0.079 e2e^{2}b3 deduced from inelastic nucleon- and light-ion scattering data (see Table V in Ref. [28]), such a disagreement with the 31{}^{-}_{1} angular distribution for 90Zr would not be unexpected. Indeed, the best DWBA fit to the measured 31{}^{-}_{1} cross sections yields a lower value of B(E3)DOP0.051e2B(E3)_{\rm DOP}\approx 0.051\ e^{2}b3.

III DWBA analysis based on the folded deuteron-nucleus potential

The microscopic description of the nucleus-nucleus interaction is usually based on a chosen effective pairwise nucleon-nucleon (NN) interaction vv between projectile nucleon and bound nucleon of target. The density dependence of vv presumably takes into account the three-nucleon interaction and higher-order NN correlations. Among such models, the double-folding model (DFM) has been used widely to calculate the α\alpha-nucleus and heavy-ion OP [12, 13, 14]. The established success of the DFM in describing the observed elastic scattering for many nucleus-nucleus systems indicates that it produces the dominant part of the nucleus-nucleus OP. Within the DFM, the deuteron-nucleus scattering potential can be formally determined [14] as

UF=dA|VdA|dA=𝒜idjAjAij|vNN|ij,U_{F}=\langle dA^{\prime}|V_{d-A}|dA\rangle=\mathcal{A}\sum_{i\in d}\sum_{j\in A}\sum_{j^{\prime}\in A^{\prime}}\langle ij^{\prime}|v_{\rm NN}|ij\rangle, (13)

where the diagonal (A=AA^{\prime}=A ) and nondiagonal (AAA^{\prime}\neq A) matrix elements describe elastic and inelastic deuteron-nucleus scattering, respectively. The antisymmetrization 𝒜\mathcal{A} accounts for all single-nucleon exchanges between deuteron and target, giving rise to a nonlocal exchange term of the potential (13)

UF=idjAjA[ij|vD|ij+ij|vEX|ji],U_{F}=\sum_{i\in d}\sum_{j\in A}\sum_{j^{\prime}\in A^{\prime}}[\langle ij^{\prime}|v_{\rm D}|ij\rangle+\langle ij^{\prime}|v_{\rm EX}|ji\rangle], (14)

where vD(EX)v_{\rm D(EX)} is the direct (exchange) part of vv. Given the nonlocal exchange potential, one has to solve an integro-differential OM equation involving a nonlocal kernel of the deuteron-nucleus OP, which has not been done so far due the complexity of the nonlocal DFM computation. In fact, the exact solution of the OM equation with the nonlocal folded OP was obtained only for elastic nucleon scattering (see, e.g., Ref. [16] and references therein). Like previous DFM calculations [29, 14], we have used in the present work the well-proven local approximation for the exchange potential, based on the WKB approximation for the change in the deuteron-nucleus relative motion wave function induced by the exchange of spatial coordinates of each interacting nucleon pair (see more details in Ref. [15]). In this case, both the direct and exchange terms of the deuteron-nucleus potential (14) are evaluated [14] by folding the deuteron and target densities of with the chosen effective NN interaction vv. The accuracy of such a WKB approximation was shown again in a recent OM study of elastic nucleon-nucleus scattering [16]. With a localized exchange potential, not only the OM calculation is much simpler, but also the comparison with the (local) phenomenological OP (1)-(6) is more direct which is essential for the present study.

Effective density-dependent NN interaction and nuclear densities

The CDM3Y6 density-dependent version of the M3Y interaction [29] is used in the present DFM calculation of the deuteron-nucleus potential (13)-(14). The real density dependence of the CDM3Y6 interaction was adjusted by a realistic HF description of nuclear matter, with nuclear incompressibility K252K\approx 252 MeV [29]. The imaginary density dependence of the CDM3Y6 interaction was introduced in Ref. [30] to reproduce the Brueckner–Hartree–Fock results for nucleon OP in nuclear matter by Jeukenne, Lejeune and Mahaux (the JLM potential) [31]. This (complex) density-dependent CDM3Y6 interaction was successfully used in the DFM calculation of the α+208\alpha+^{208}Pb OP and inelastic scattering FF [30] for the multipole decomposition analysis of (α,α)(\alpha,\alpha^{\prime}) data measured for isoscalar giant resonances of 208Pb at 97 MeV/nucleon [32]. We note that prior to the present work, the only DFM calculation of the deuteron-nucleus OP was done 42 years ago by Cook [33] using the density independent M3Y interaction.

Beside the effective NN interaction, the nuclear densities of projectile and target are essential inputs for the DFM calculation. In the present work, we have chosen the deuteron density given by the exact solution of the two-body problem using the Argonne V18 interaction as the free NN interaction [34]. For the DFM calculation of the diagonal (A=AA^{\prime}=A ) elastic deuteron-nucleus potential, the Fermi distribution has been adopted for the ground-state (g.s.) densities of target nuclei:

ρ0(r)=ρ0/[1+exp((rc)/a)],\rho_{0}(r)=\rho_{0}/[1+\exp((r-c)/a)], (15)

with the parameters ρ0,c\rho_{0},\ c and aa listed in Table 4.

Table 4: Parameters of the Fermi distribution (15).
Nuclear density distribution
Target 24Mg 28Si 58Ni 90Zr 116Sn 208Pb
ρ0\rho_{0} (fm-3) 0.170 0.167 0.176 0.165 0.154 0.157
cc (fm) 2.995 3.160 4.080 4.900 5.490 6.670
aa (fm) 0.478 0.523 0.515 0.515 0.515 0.545
Reference [35] [35] [36] [37] [37] [37]
Charge density distribution
Target 24Mg 28Si 58Ni 90Zr 116Sn 208Pb
ρ0\rho_{0}(fm-3) 0.0785 0.0841 0.0826 0.0726 0.0688 0.0628
cc (fm) 3.045 3.154 4.177 4.908 5.417 6.647
aa (fm) 0.523 0.523 0.523 0.523 0.523 0.523
Reference [38] [38] [38] [38] [38] [38]

The main input for the DFM calculation of the nondiagonal (AAA^{\prime}\neq A) deuteron-nucleus potential (the folded inelastic scattering FF) is the nuclear transition density of the target excitation. The DFM method (13)-(14) is also used to calculate the Coulomb inelastic FF microscopically by folding the deuteron charge density and charge transition density of the target excitation with the Coulomb force acting between two protons [14]. For the 2λ-pole excitations under study, we adopt the so-called Bohr-Mottelson prescription [39] for the nuclear- and charge transition densities

ρλ(r)=δλdρ0(r)drandρcharge(λ)(r)=δλdρcharge(0)(r)dr,\rho_{\lambda}(r)=-\delta_{\lambda}\frac{d\rho_{0}(r)}{dr}\ \mbox{and}\ \rho^{(\lambda)}_{\rm charge}(r)=-\delta_{\lambda}\frac{d\rho^{(0)}_{\rm charge}(r)}{dr}, (16)

where the g.s. charge density ρcharge(0)(r)\rho^{(0)}_{\rm charge}(r) is determined using the same Fermi distribution (15) with parameters listed in Table 4. The deformation length δλ\delta_{\lambda} is determined from the transition rate B(Eλ)B(E\lambda\uparrow) of the target excitation using the following relation

B(Eλ)=e2|Mλ|2,whereMλ=0rλ+2ρcharge(λ)(r)𝑑r.B(E\lambda)=e^{2}|M_{\lambda}|^{2},\ \mbox{where}\ M_{\lambda}=\int_{0}^{\infty}r^{\lambda+2}\rho^{(\lambda)}_{\rm charge}(r)~{}dr. (17)

At variance with the DOP prescription (11), the deformation length δλ\delta_{\lambda} in Eq. (17) is the scaling factor of the nuclear transition density (16) used in the folding calculation (14) of inelastic scattering FF, which is constrained by the considered B(Eλ)B(E\lambda) transition rate.

Folded deuteron OP and inelastic scattering FF

The deuteron breakup has been shown to affect significantly the deuteron OP at the surface [22, 23], and a WS surface term WD(r)W_{D}(r) has been added to the imaginary folded OP because the DFM does not take into account the dynamic polarization of the OP by the breakup effect. A slight renormalization of the strength of both the real and imaginary folded OP is also allowed in the OM analysis of elastic (d,d)(d,d) data, and the total OP is determined in the hybrid manner as

U(r)=UF(0)(r)+iWD(r)+Vs(r)(𝒔)+VC(r),U(r)=U^{(0)}_{F}(r)+iW_{D}(r)+V_{\ell s}(r)(\mbox{\boldmath$\ell$}\cdot\mbox{\boldmath$s$})+V_{C}(r), (18)

where UF(0)(r)=NVVF(0)(r)+iNWWF(0)(r)U^{(0)}_{F}(r)=N_{V}V^{(0)}_{F}(r)+iN_{W}W^{(0)}_{F}(r) is the diagonal folded deuteron-nucleus potential (14). The surface and spin-orbit terms of the OP (18) are determined in the same way as in Eqs. (4)-(5). The OM results obtained with the hybrid folded deuteron OP (18) are shown as solid lines in Figs. 1 and 2, with the best-fit NV(W)N_{V(W)} coefficients, parameters of the surface and spin-orbit terms of the OP listed in Table 5.

Table 5: Best-fit NV(W)N_{V(W)} coefficients, parameters of the surface and spin-orbit terms of the hybrid folded deuteron OP (18). Because of spin convention, the VsV_{\ell s} value must be divided by 2 when used in the numerical input of the code ECIS97 [24]. The errors were deduced from the weight of each parameter in the covariant multi-parameter χ2\chi^{2}-search, with WD,aD,VsW_{D},\ a_{D},\ V_{\ell s}, and asa_{\ell s} kept fixed during the search.
Target 208Pb 116Sn 90Zr 58Ni 28Si 24Mg
NVN_{V} 0.98±0.010.98\pm 0.01 0.94±0.010.94\pm 0.01 0.98±0.010.98\pm 0.01 0.98±0.010.98\pm 0.01 0.95±0.010.95\pm 0.01 0.95±0.010.95\pm 0.01
NWN_{W} 1.01±0.021.01\pm 0.02 1.04±0.021.04\pm 0.02 1.00±0.011.00\pm 0.01 1.03±0.031.03\pm 0.03 1.09±0.031.09\pm 0.03 1.00±0.031.00\pm 0.03
WDW_{D} (MeV) 7.60 7.60 7.60 7.60 7.60 7.60
rDr_{D} (fm) 0.70±0.090.70\pm 0.09 0.70±0.040.70\pm 0.04 0.55±0.030.55\pm 0.03 0.92±0.040.92\pm 0.04 0.54±0.070.54\pm 0.07 0.75±0.080.75\pm 0.08
aDa_{D} (fm) 0.65 0.65 0.65 0.65 0.65 0.65
VsV_{\ell s} (MeV) 4.22 4.22 4.22 4.22 4.22 4.22
rsr_{\ell s} (fm) 1.03±0.011.03\pm 0.01 1.00±0.021.00\pm 0.02 1.03±0.021.03\pm 0.02 1.05±0.011.05\pm 0.01 1.03±0.021.03\pm 0.02 0.82±0.020.82\pm 0.02
asa_{\ell s} (fm) 0.85 0.85 0.85 0.85 0.85 0.85

With the surface absorption taken into account by WD(r)W_{D}(r) term of the imaginary deuteron OP (18), the impact of the deuteron breakup on the complex folded deuteron-nucleus OP seems to be small, with the obtained NV(W)N_{V(W)} coefficients being quite close to unity (see Table 5).

The total inelastic (d,d)(d,d^{\prime}) scattering FF is also determined in the hybrid manner as

Fλ(r)=UF(λ)(r)+FWD(λ)(r)+Fs(λ)(r)(𝒔)+FC(λ)(r),F_{\lambda}(r)=U^{(\lambda)}_{F}(r)+F^{(\lambda)}_{W_{D}}(r)+F^{(\lambda)}_{\ell s}(r)(\mbox{\boldmath$\ell$}\cdot\mbox{\boldmath$s$})+F^{(\lambda)}_{C}(r), (19)

where the folded nuclear UF(λ)(r)=VF(λ)(r)+iWF(λ)(r)U^{(\lambda)}_{F}(r)=V^{(\lambda)}_{F}(r)+iW^{(\lambda)}_{F}(r) and Coulomb FC(λ)(r)F^{(\lambda)}_{C}(r) terms of the inelastic scattering FF are kept unchanged (as given by the DFM calculation) in the DWBA analysis of (d,d)(d,d^{\prime}) data. The surface and spin-orbit terms of the FF (19) are determined by the DOP method (9)-(10), using the same deformation length δλ\delta_{\lambda} as that used for the nuclear- and charge transition densities (16). The DWBA results obtained with the hybrid folded inelastic FF (19) for (d,d)(d,d^{\prime}) scattering on 24Mg, 28Si, 58Ni, and 208Pb targets are shown in Fig. 6. Unlike the DWBA description of the 21+{}^{+}_{1} cross sections measured for light 24Mg and 28Si targets given by the collective model FF (9)-(12) shown in Fig. 3, the hybrid folded FF (19) reproduces these same (d,d)(d,d^{\prime}) data very well using the B(E2)adoptedB(E2)_{\rm adopted} values. The oscillation pattern of the 21+{}^{+}_{1} cross section observed for these targets is also better reproduced by the hybrid folded FF compared to the collective model FF, and the best-fit B(E2)DFMB(E2)_{\rm DFM} value agrees nicely with the B(E2)adoptedB(E2)_{\rm adopted} value as shown in Table 3.

Refer to caption
Figure 6: The same as in Fig. 3 but obtained with the hybrid folded inelastic FF (19). The DWBA results based on the adopted B(Eλ)adoptedB(E\lambda)_{\rm adopted} and best-fit B(Eλ)DFMB(E\lambda)_{\rm DFM} values (see Table 3) are shown as dashed and solid lines, respectively.

It should be noted here that the deformation parameter β2\beta_{2} is obtained in one case from the OP geometry using the DOP method (9)-(10), while in the other case it is obtained (16) from the geometry of the g.s. density. A more accurate comparison could be made based on the deformation length β2R\beta_{2}R obtained from both geometries or even better to compare the full integral of both the folded inelastic FF and collective model FF determined with the respective deformation parameters.

The DWBA descriptions of the 21+2^{+}_{1} and 313^{-}_{1} angular distributions given by the hybrid folded inelastic FF (19) for 116Sn and 90Zr targets are shown in Figs. 7 and 8, respectively. One can see that the collective-model and hybrid folded inelastic scattering FF’s give nearly equivalent DWBA descriptions of (d,d)(d,d^{\prime}) data measured for the 21+2^{+}_{1} excitation of these nuclei. The best-fit B(E2)DOPB(E2)_{\rm DOP} and B(E2)DFMB(E2)_{\rm DFM} values obtained for 90Zr and 116Sn targets are larger than the adopted values by around 5% and 15%, respectively (see Table 3).

Refer to caption
Figure 7: The same as in Fig. 4, but obtained with the hybrid folded inelastic FF (19). The DWBA results based on the adopted B(Eλ)adoptedB(E\lambda)_{\rm adopted} and best-fit B(Eλ)DFMB(E\lambda)_{\rm DFM} values (see Table 3) are shown as dashed and solid lines, respectively.
Refer to caption
Figure 8: The same as in Fig. 5, but obtained with the hybrid folded inelastic FF (19). The DWBA results based on the B(Eλ)adoptedB(E\lambda)_{\rm adopted} and best-fit B(Eλ)DFMB(E\lambda)_{\rm DFM} values (see Table 3) are shown as dashed and solid lines, respectively.

Like the DWBA results given by the collective-model FF shown in Figs. 4 and 5, the DWBA results given by the hybrid folded FF (19) based on the B(E3)adoptedB(E3)_{\rm adopted} value [28] reasonably reproduce the (d,d)(d,d^{\prime}) data measured for the 31{}^{-}_{1} state of 116Sn, but overestimate the data measured for the 31{}^{-}_{1} state of 90Zr over the entire angular range. The best-fit B(E3)DFMB(E3)_{\rm DFM} value is around 35% smaller than B(E3)adoptedB(E3)_{\rm adopted} value from (e,e)(e,e^{\prime}) data, but in a good agreement with the empirical B(E3)B(E3) values deduced from inelastic nucleon- and light-ion scattering data [28].

We note further that the best-fit B(E3)DOPB(E3)_{\rm DOP} value obtained for the 31{}^{-}_{1} state of 90Zr using the collective-model FF is about 20% lower than the best-fit B(E3)DFMB(E3)_{\rm DFM} value. A similar trend was also found for 313^{-}_{1} states of 116Sn and 208Pb (see Table 3) which shows that the DOP method consistently gives a lower B(E3)B(E3) value compared to that given by the DFM approach, as discussed previously in Ref. [40]. However, the DOP method seems to better reproduce B(E3)adoptedB(E3)_{\rm adopted} value from the Coulomb excitation data [28].

Summary

Elastic and inelastic deuteron scattering have been measured off 24Mg, 28Si, 58Ni, 90Zr, 116Sn, and 208Pb at an energy of 98 MeV/nucleon. The measured (d,d)(d,d) and (d,d)(d,d^{\prime}) angular distributions were analyzed within the OM and DWBA using the phenomenological deuteron OP associated with the collective model of nuclear scattering, and the hybrid potential model for the deuteron OP and inelastic FF based on the microscopic DFM calculation. The E2E2 and E3E3 transition rates of the 21+2^{+}_{1} and 313^{-}_{1} excitations of these target nuclei have been deduced from the best DWBA fits to the (d,d)(d,d^{\prime}) scattering data, which agree reasonably with the adopted B(Eλ)B(E\lambda) values [26, 28].

The results of the OM analysis of elastic (d,d)(d,d) data using the hybrid folded OP show that the deuteron breakup does not affect significantly the volume part of the deuteron OP given by the DFM calculation. However, the breakup effect seems to imply an enhanced absorption at the surface, which can be taken into account effectively by a surface WS potential added to the imaginary deuteron OP.

While both potential models describe equally well the (d,d)(d,d) and (d,d)(d,d^{\prime}) angular distributions measured for medium- and heavy-mass target nuclei, the DWBA calculation using the collective-model inelastic FF (DOP) gives a poorer description of the 21+2^{+}_{1} angular distribution measured for the light-mass 24Mg and 28Si nuclei, in comparison with the DWBA description of the same data using the semi-microscopic folded inelastic FF (DFM).

The DWBA analysis of the 313^{-}_{1} angular distribution measured for 90Zr target indicates that B(E3)adoptedB(E3)_{\rm adopted} value from (e,e)(e,e^{\prime}) data [28] is too high, and the DWBA results given by the two potential models agree well with (d,d)(d,d^{\prime}) scattering data, with the best-fit B(E3)B(E3) values close to those deduced from inelastic nucleon- and light-ion scattering data.

A hindrance of the E3E3 transition rate determined by the collective-model inelastic FF compared to that determined by the inelastic folded FF was also found, which illustrates the inconsistency between the DWBA description of nuclear excitation with λ3\lambda\gtrsim 3 based on the DOP approach and that based on the DFM approach discussed earlier by Beene et al. [40].

Acknowledgment

We acknowledge the efforts of the RCNP staff in providing high-quality deuteron beams required for these measurements, and thank A. Okamoto (Konan), T. Sako (Kyoto) and K. Schlax (Notre Dame) for their assistance with the experiment. This work has been supported in part by the National Science Foundation (Grants No. PHY-1068192, No. PHY-2011890, and No. PHY-2310059). Two of us (D.C.C. and D.T.K.) were supported by the National Foundation for Science and Technology Development of Vietnam (NAFOSTED Project No. 103.04-2021.74).

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