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Systematic study for relation between nuclear structure and reaction in 10Be nucleus

T. Furumoto [email protected] College of Education, Yokohama National University, Yokohama 240-8501, Japan    T. Suhara Matsue College of Technology, Matsue 690-8518, Japan    N. Itagaki Department of Physics, Osaka Metropolitan University, Osaka, 558-8585, Japan Nambu Yoichiro Institute of Theoretical and Experimental Physics (NITEP), Osaka Metropolitan University, Osaka 558-8585, Japan
Abstract

We systematically investigate the relation between the nuclear structure and reaction in the 10Be nucleus using a theoretical framework. The structure of the 10Be nucleus is constructed with a cluster model based on a microscopic viewpoint. In this paper, the 10Be nucleus with different structures is prepared by manipulating the parameters of an effective nucleon-nucleon interaction. The nuclear structure and expectation values of physical quantities are drastically changed by the modification. We summarize such changes and show the effects on the elastic and inelastic scatterings for the proton and 12C targets in the microscopic coupled-channel calculation. Especially, we recently reported the visualization of dineutron correlation in 10Be on proton inelastic scattering in [Phys. Rev. C104, 034613 (2021)]. In this preceding work, we found that the changing the degree of dineutron correlation in 10Be leads to drastic changes of the inelastic cross section for the 2+2{}_{2}^{+} state. The development (or breaking) of the dineutron correlation is governed by the strength of the spin-orbit interaction of the structure calculation. However, in the previous work, some of the realistic physical points were missing, for example, the binding energy. Therefore, we reconstruct the 10Be nucleus by adjusting the effective nucleon-nucleon interaction to obtain the reasonable binding energy of the ground state. With this improvement, we again discuss the dineutron correlation in the 10Be nucleus. We reconfirm the way to measure the degree of the development (or breaking) of dineutron cluster structure; the sensitivity to the inelastic cross section of the ground state to the 2+2{}_{2}^{+} state of 10Be.

I Introduction

For decades, the microscopic description based on the nucleon-nucleon (NNNN) interaction for the nuclear structure and reaction has been developed. These microscopic approaches are successful in describing and understanding the properties of the nuclear structure and reaction quite well. Although the NNNN interaction has been investigated since the discovery of the proton and neutron, its behavior is still not fully understood, especially in the nuclear medium. Therefore, in these microscopic structure and reaction calculations, the effective NNNN interaction with parameters has often been used. There are many microscopic models based on the (effective) NNNN interaction for the nuclear structure Vautherin and Brink (1972); Dechargé and Gogny (1980); Kamimura (1981); Ono et al. (1992); Baye et al. (1994); Itagaki et al. (1995); Navrátil et al. (2000); Otsuka et al. (2001); Nakada (2003); Suhara and Kanada-En’yo (2010); Isaka and Kimura (2015); Tohsaki et al. (2001); Kanada-Enyo et al. (1995); Neff and Feldmeier (2004). The microscopic description has led to the understanding of a great deal of nuclear structure information. Recently, improvements in computational technology have made it possible to perform even more precise nuclear structure calculations. Most microscopic approaches to nuclear reactions are based on the folding model. This has been developed for the nucleon and heavy-ion scatterings Sinha (1975); Brieva and Rook (1977a, b, 1978); Satchler and Love (1979); Kobos et al. (1982); Khoa et al. (1994); Rikus and Geramb (1984); Khoa et al. (1997); Amos et al. (2000); Khoa (2001); Furumoto and Sakuragi (2006); Khoa et al. (2007); Furumoto et al. (2008, 2009, 2010, 2016). It is remarkable that the recent microscopic description of the nuclear structure and reaction is based on the realistic NNNN interaction.

Through these analyses, the connection between the microscopic nuclear structure and reaction models has been attempted. By the connection, microscopic nuclear reaction calculations accurately incorporating nuclear structure information were performed, and many experimental data were successfully reproduced Sakuragi et al. (1986); Takashina et al. (2005); Khoa et al. (2011); Qu et al. (2015, 2017); Kanada-En’yo and Ogata (2019). In addition, the approach with the microscopic nuclear structure and reaction gives interesting predictions Furumoto et al. (2010); Furumoto and Sakuragi (2013); Furumoto et al. (2013, 2021). In such approaches, density is one of the key intermediaries because it is one of the inputs in the microscopic folding model and one of the outputs in the microscopic nuclear structure model. The diagonal and transition densities contain a large amount of nuclear structure information. The microscopic folding model tells us the nuclear structure information in the observable through the density. Therefore, to derive the diagonal and transition densities not only microscopically but also macroscopically is important to connect nuclear structure and reaction. Here, we note that it is possible to observe the structure information in experimental data if the diagonal and transition densities have a sensitivity to the nuclear structure. Therefore, it is important to make the relation among density, nuclear structure, reaction mechanism, and observable clearer.

Here, we demonstrate an example of how the change of the nuclear structure in an artificial way affects the reaction. The change is closely related to the development and breaking of the dineutron correlation as reported in Ref. Itagaki et al. (2002), where we discussed the dineutron correlation and its breaking because of the spin-orbit interaction. The persistence of the dineutron cluster is sensitive to the choice of the strength of the spin-orbit interaction in the structure calculation, even if the binding energy of the neutrons from the threshold is kept constant. Although the dineutron structure is favored when the spin-orbit interaction is weak, the spin-orbit interaction with realistic strength significantly breaks the dineutron structure. In Ref. Furumoto et al. (2021), we found that the inelastic cross section to the 22+{}^{+}_{2} state is drastically dependent on the development and breaking of the dineutron correlation. With the advancement of microscopic approaches, such a reliable and interesting analysis is now feasible. Here, we again summarize the basic properties of 10Be. The 10Be nucleus is considered as a typical neutron-rich nucleus with a cluster structure, and in this nucleus, two valence neutrons perform molecular-orbital motions around two α\alpha clusters Seya et al. (1981); Itagaki and Okabe (2000); Itagaki et al. (2000, 2002). With regard to its 0+ states, the 01+{}^{+}_{1} and 03+{}^{+}_{3} states are characterized by the π\pi orbit of the valence neutrons around α\alphaα\alpha. On the other hand, the 02+{}^{+}_{2} state has a large α\alphaα\alpha distance, which is characterized by the σ\sigma orbit. Above these 0+ states, rotational bands are formed. For example, the 21+{}^{+}_{1} state is a member of the K=0K=0 band together with the ground 0+0^{+} state, and the 22+{}^{+}_{2} state is the band head state of the K=2K=2 side-band.

In this study, we perform the systematic calculation to reveal the relation between the nuclear structure and reaction of the 10Be nucleus. The present 10Be nucleus is constructed under the assumption of the four-body (α\alpha + α\alpha + n + n) cluster model. The stochastic multi-configuration mixing method enables to the description of many exotic cluster structures Ichikawa et al. (2011); Muta et al. (2011). We focus on the low-lying (0+1{}_{1}^{+}, 2+1{}_{1}^{+}, and 2+2{}_{2}^{+}) states. In the microscopic cluster model, we modify the various parameters for the effective NNNN interaction. The energies, nuclear size, and expectation values of 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (one-body operator) and 𝑺2\langle\bm{S}^{2}\rangle (two-body operator) are calculated to investigate the dependence of the parameters for the NNNN interaction. The transition strengths with multipolarity λ=2\lambda=2 are listed for the proton, neutron, isoscalar (IS), and isovector (IV) parts, respectively. To apply the microscopic nuclear reaction model, we obtain the diagonal and transition densities from the total wave function. Specifically, the microscopic coupled channel (MCC) calculation is performed to describe 10Be elastic and inelastic scatterings by a proton and 12C targets at E/A=E/A= 59.4 and 200 MeV. The present MCC calculation well reproduces the experimental data for the 0+1{}_{1}^{+} and 2+1{}_{1}^{+} states at E/A=E/A= 59.4 MeV. Although no experimental data are available for the 2+2{}_{2}^{+} state, the inelastic cross section is demonstrated in the present MCC calculation. The effect of the change of the parameters in the microscopic structure calculation is discussed on the elastic and inelastic scattering cross sections derived from the MCC calculation. In addition, we reconstruct the 10Be nucleus by adjusting the binding energy, which was ignored in the previous systematic calculation. With this improvement, we again discuss the possibility of observing the degree of the development and breaking of the dineutron correlation in 10Be through the 2+2{}_{2}^{+} inelastic cross section.

This paper is organized as follows. In Sec. II, we briefly introduce the present structure and reaction models. In Sec. III, we listed the results of the microscopic cluster model with the modified parameters. We also show the results of the elastic and inelastic cross sections with the modified nuclear structure information. We will discuss the effect of the value of the parameters in the nuclear structure calculation. In addition, we show the results of the reconstructed 10Be nucleus by reproducing the binding energy by simultaneously adjusting the spin-orbit strength and the Majorana parameter. The development and breaking of the dineutron correlation in 10Be are again discussed. Lastly, we summarize this paper in Sec. IV.

II Formalism

We first construct the 10Be nucleus within the 4-body (α\alpha + α\alpha + n + n) cluster model. With the diagonal and transition densities obtained from the microscopic cluster calculation, the 10Be + p and 10Be + 12C elastic and inelastic scatterings are given by the microscopic coupled channel (MCC) calculation as the same manners in Refs. Furumoto et al. (2013, 2021). To avoid repetition, we give just the main points in this section. The details of the structure and reaction calculations are provided in Refs. Furumoto et al. (2013, 2018); Furumoto and Takashina (2021); Furumoto et al. (2021).

II.1 Microscopic cluster model

The 10Be nucleus is constructed by the stochastic multiconfiguration mixing method based on the microscopic cluster model Ichikawa et al. (2011); Muta et al. (2011). The calculation method is almost the same as Ref. Furumoto et al. (2021). Therefore, we use a simplified notation in this paper.

The total wave function Φ\Phi is expressed by the superposition of the basis states Ψ\Psi as follows:

Φ=iciΨi.\Phi=\sum_{i}c_{i}\Psi_{i}. (1)

After the parity and angular momentum projections, the eigenstates of the Hamiltonian are obtained by diagonalizing the Hamiltonian matrix. Additionally, the coefficients, cic_{i}, for the linear combination of Slater determinants are obtained. We adopt 500 basis states to obtain the total wave function. We confirmed that sufficient convergence was achieved with 500 basis states. In fact, for the 4-body cluster system, even 400 basis states are known to provide sufficient convergence as shown in Ref. Furumoto et al. (2013).

In the above process, we introduce various α\alpha + α\alpha + n + n configurations for the basis states to describe the 10Be nucleus as follows:

Ψi=𝒜[ϕα(𝒓14,𝑹1)ϕα(𝒓58,𝑹2)ϕn(𝒓9,𝑹3)ϕn(𝒓10,𝑹4)]i,\Psi_{i}={\cal A}\big{[}\phi_{\alpha}(\bm{r}_{1-4},\bm{R}_{1})\phi_{\alpha}(\bm{r}_{5-8},\bm{R}_{2})\phi_{n}(\bm{r}_{9},\bm{R}_{3})\phi_{n}(\bm{r}_{10},\bm{R}_{4})\big{]}_{i}, (2)

where 𝒜\cal A is the antisymmetrizer and ϕα\phi_{\alpha} and ϕn\phi_{n} are the wave functions of α\alpha and neutron, respectively. The wave functions of the jj-th nucleon, whose spatial coordinate is 𝒓j\bm{r}_{j}, is described as a locally shifted Gaussian centered at 𝑹\bm{R}, exp[ν(𝒓j𝑹)2]\exp[-\nu(\bm{r}_{j}-\bm{R})^{2}]. Here, the positions of the Gaussian-centered parameter 𝑹\bm{R} are randomly generated. The ν\nu parameter is ν=\nu= 1/(2×\times1.462) fm-2, which is widely used and satisfies the binding energy of the α\alpha particle.

The Hamiltonian is given as follows. The two-body interaction includes the central, spin-orbit, and Coulomb parts. The Volkov No.2 effective potential is applied to the central part Volkov (1965), as,

V(central)(r)\displaystyle V^{\rm(central)}(r) =\displaystyle= (WMPσPτ+BPσHPτ)\displaystyle(W-MP^{\sigma}P^{\tau}+BP^{\sigma}-HP^{\tau}) (3)
×(V1exp(r2/c12)+V2exp(r2/c22)),\displaystyle\times(V_{1}\exp(-r^{2}/c_{1}^{2})+V_{2}\exp(-r^{2}/c_{2}^{2})),

where c1=c_{1}= 1.01 fm, c2=1.8c_{2}=1.8 fm, V1=V_{1}= 61.14 MeV, V2=60.65V_{2}=-60.65 MeV, and W=1MW=1-M. Here, we often use the parameter setting as M=0.60M=0.60 and B=H=0.08B=H=0.08 Furumoto et al. (2013, 2018, 2021), which reproduces the α\alpha-α\alpha scattering phase shift. Meanwhile, the different values for the parameters MM and B=HB=H are employed in the investigations of various nuclei Varga and Cseh (1993); Ito et al. (2004); Kanada-En’yo (2007); Suhara and Kanada-En’yo (2010). Therefore, we examine in the range of 0.52, 0.54, 0.56, 0.58, 0.60, 0.62, and 0.64 for MM and 0, 0.04, 0.08, 0.12, 0.16, and 0.20 for B=HB=H.

Here, we introduce the spin-orbit term of the G3RS potential Tamagaki (1968); Yamaguchi et al. (1979),

V(spinorbit)(r)=VLS(ed1r2ed2r2)P(3O)𝑳𝑺,V^{\rm(spin-orbit)}(r)=V_{\rm LS}(e^{-d_{1}r^{2}}-e^{-d_{2}r^{2}})P(^{3}O)\bm{L}\cdot{\bm{S}}, (4)

where d1=5.0d_{1}=5.0 fm-2 and d2=2.778d_{2}=2.778 fm-2. The operator 𝑳\bm{L} represents the relative angular momentum, and 𝑺\bm{S} represents the spin (𝑺1+𝑺2\bm{S}_{1}+\bm{S}_{2}). P(3O)P(^{3}O) is the projection operator onto the triplet odd state. As in Ref. Furumoto et al. (2021), the strength of the spin-orbit interaction, VLSV_{\rm LS}, is also treated as a parameter in this paper. This value is often fixed around 2000 MeV to reproduce the data of the 10Be nucleus. In this paper, we show the results with VLSV_{\rm LS} = 0, 500, 1000, 1500, 2000, 2500, 3000, 3500, and 4000 MeV.

To connect the nuclear structure and reaction calculations, we prepare the diagonal and transition densities in the same manner as in Ref. Baye et al. (1994).

II.2 MCC model

After calculating the diagonal and transition densities, we perform the nuclear reaction calculation. We apply the calculated densities to MCC calculations with the complex GG-matrix interaction MPa Yamamoto et al. (2014, 2016). The MPa interaction has been successfully applied for nuclear reactions Furumoto et al. (2016); Qu et al. (2017); Furumoto et al. (2019); Furumoto and Takashina (2021). The detailed MCC calculation procedure for the folding potential is described in Refs. Khoa et al. (2002); Furumoto et al. (2008); Furumoto and Takashina (2021); Furumoto et al. (2021). Then, we briefly introduce the single and double-folding model calculations.

The single-folding model potential is simply described as

Uαβ(SF)(R;E/A)=ρIαIβ(r)v(𝒔,ρ;E/A)𝑑𝒓,U^{(SF)}_{\alpha\to\beta}(R;E/A)=\int{\rho_{I_{\alpha}\to I_{\beta}}(r)v(\bm{s},\rho;E/A)d\bm{r}}, (5)

where RR is the radial distance between the incident 10Be nucleus and the target proton. α\alpha and β\beta mean channel number of the initial and final states. IαI_{\alpha} and IβI_{\beta} are spins of the initial and final states, respectively. E/AE/A is the incident energy per nucleon. ρIαIβ\rho_{I_{\alpha}\to I_{\beta}} is the diagonal (α=β\alpha=\beta) and transition (αβ\alpha\neq\beta) densities; ss is the radial distance between a nucleon in the projectile nucleus and the target proton, and 𝒔=𝒓𝑹\bm{s}=\bm{r}-\bm{R}. We note that the description of Eq. (5) is simplified; in the actual calculation, the proton and neutron densities are separately folded with the proton-proton and proton-neutron interactions, respectively. The Coulomb potential is also obtained by folding the nucleon-nucleon Coulomb interaction and proton density. The knock-on exchange part and the spin-orbit part are obtained in the same manner as in Refs. Furumoto and Takashina (2021); Furumoto et al. (2021).

The double-folding model potential is also provided as

Uαβ(DF)(R;E/A)=ρIαIβ(𝒓)ρIαIβ(𝒓)v(𝒔,ρ;E/A)𝑑𝒓𝑑𝒓,U^{(DF)}_{\alpha\to\beta}(R;E/A)=\int{\rho_{I_{\alpha}\to I_{\beta}}(\bm{r})\rho^{\prime}_{I^{\prime}_{\alpha}\to I^{\prime}_{\beta}}(\bm{r}^{\prime})v(\bm{s},\rho;E/A)d\bm{r}d\bm{r}^{\prime}}, (6)

where IαI^{\prime}_{\alpha} and IβI^{\prime}_{\beta} are spins of initial and final states for the target nucleus, respectively. ρIαIβ\rho^{\prime}_{I^{\prime}_{\alpha}\to I^{\prime}_{\beta}} is the diagonal (α=β\alpha=\beta) and transition (αβ\alpha\neq\beta) densities for the target nucleus. Here, 𝒔=𝒓𝒓𝑹\bm{s}=\bm{r}-\bm{r}^{\prime}-\bm{R}. The frozen density approximation is applied to ρ\rho in vv. The frozen density approximation is the standard prescription to describe the nucleus-nucleus system and its efficiency is verified in Refs. Furumoto et al. (2009, 2016). The knock-on exchange part is obtained in the same manner as Refs. Furumoto and Sakuragi (2013); Furumoto et al. (2013).

When the single and double folding potentials are applied to the nuclear reaction, we modify the strength of the imaginary part of the potential. Since the complex GG-matrix is constructed with the infinite nuclear matter, the strength of the imaginary part is often adjusted for the finite nucleus because these level densities are quite different. Therefore, we consider the incident-energy-dependent renormalization factor, NW=0.5+(E/A)/1000N_{W}=0.5+(E/A)/1000 Furumoto et al. (2019), for the imaginary part of the folding model potential. We note that any additional parameter is not needed to calculate the 10Be scatterings by the proton and 12C targets. With the potentials, the scattering matrix is obtained from the folded potentials by solving the CC equation based on the Stormer method. Relativistic kinematics is used in the calculation. The cross sections are calculated with the scattering amplitude derived from the scattering matrix as shown in Ref. Satchler (1983).

III Results

The calculated results will be introduced and discussed in this section. We first show the dependence of the parameters (VLSV_{\rm LS}, MM, and B(=H)B(=H)) for the binding energy, radius, and expectation values of 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle and 𝑺2\langle\bm{S}^{2}\rangle of the 01+{}^{+}_{1}, 21+{}^{+}_{1}, and 22+{}^{+}_{2} states, respectively. Here, 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle is the expectation value of the one-body operator and the sum of the spin-orbit operator of the nucleons, whereas 𝑺2\langle\bm{S}^{2}\rangle is the two-body operator, which is the square of the sum of the one-body spin operator over the nucleons. In the investigation of the dependence of the parameters (VLSV_{\rm LS}, MM, and B(=H)B(=H)), we regard the standard values of VLS=V_{\rm LS}= 2000 MeV, M=M= 0.60, and B=H=B=H= 0.08 as criterion. The quadrupole transition strength between each states is also introduced. In addition, we discuss the effect of the change in the nuclear structure on the elastic and inelastic cross sections.

When we calculate the 10Be + 12C system, we apply the 12C density obtained by 3α\alpha-RGM Kamimura (1981) to the MCC calculation. The 01+{}^{+}_{1}, 21+{}^{+}_{1}, and 02+{}^{+}_{2} states of the 12C nucleus are included because the excitation states are well known to have a strong channel coupling effect.

After that, we discuss the relation between the dineutron correlation and the inelastic cross section at the realistic physical point. Concretely, we show the additional results in which the MM and VLSV_{\rm LS} parameters are simultaneously adjusted without changing the binding energy of the ground state as in Ref. Itagaki et al. (2002). In order to evaluate the effect of the dineutron correlation on the structure and reaction, we prepare the pure dineutron basis and compare with more realistic one.

III.1 Systematic calculation with microscopic cluster model

Here we show the dependence of the structure on the parameters (VLSV_{\rm LS}, MM, and B(=H)B(=H)). The parameters give various binding energies, radii, and expectation values of 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle and 𝑺2\langle\bm{S}^{2}\rangle for the 01+{}^{+}_{1}, 21+{}^{+}_{1}, and 22+{}^{+}_{2} states. This systematic analysis clarifies the role of each parameter (VLSV_{\rm LS}, MM, and BB (=H)(=H)) in 10Be. In addition, the quadrupole transition strengths between each state are examined. The transition strengths are also changed together with the property of the nuclear structure. We will discuss the effect of the property of the nuclear structure on the elastic and inelastic cross sections.

III.1.1 Dependence of VLSV_{LS}

Here, we show the dependence of VLSV_{\rm LS} in the Hamiltonian of the nuclear structure calculation on the obtained nuclear structure and reaction. The results are essentially the same as in Ref. Furumoto et al. (2021). However, we show the calculation results as a table instead of a figure in this paper.

Table 1: Binding energies (BE), point-proton radius (rpr_{p}), point-neutron radius (rnr_{n}), point-nucleon-matter radius (rmr_{m}), expectation values of 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle and 𝑺2\langle\bm{S}^{2}\rangle for the neutron, and transition strengths (BB(E2), the neutron part (BB(E2)n), BB(IS2), and BB(IV2)) for VLSV_{\rm LS} = 0–4000 MeV.
VLSV_{\rm LS} (MeV) 0 500 1000 1500 2000 2500 3000 3500 4000
BE (01+{}^{+}_{1}) (MeV) -59.29 -59.54 -60.27 -61.43 -62.97 -64.88 -67.17 -69.81 -72.80
BE (21+{}^{+}_{1}) (MeV) -57.14 -57.23 -57.57 -58.37 -59.78 -61.66 -63.93 -66.57 -69.52
BE (22+{}^{+}_{2}) (MeV) -55.52 -55.79 -56.44 -57.14 -57.72 -58.32 -59.00 -59.80 -60.72
rpr_{p} (01+{}^{+}_{1}) (fm) 2.548 2.535 2.498 2.448 2.393 2.338 2.286 2.238 2.197
rpr_{p} (21+{}^{+}_{1}) (fm) 2.521 2.518 2.503 2.451 2.380 2.317 2.261 2.214 2.175
rpr_{p} (22+{}^{+}_{2}) (fm) 2.546 2.526 2.489 2.476 2.474 2.465 2.450 2.432 2.413
rnr_{n} (01+{}^{+}_{1}) (fm) 2.815 2.797 2.746 2.677 2.598 2.517 2.440 2.371 2.310
rnr_{n} (21+{}^{+}_{1}) (fm) 2.791 2.787 2.765 2.693 2.597 2.508 2.430 2.365 2.311
rnr_{n} (22+{}^{+}_{2}) (fm) 2.812 2.791 2.749 2.737 2.737 2.726 2.709 2.688 2.665
rmr_{m} (01+{}^{+}_{1}) (fm) 2.712 2.695 2.650 2.588 2.518 2.447 2.380 2.319 2.266
rmr_{m} (21+{}^{+}_{1}) (fm) 2.686 2.682 2.663 2.599 2.512 2.433 2.364 2.306 2.258
rmr_{m} (22+{}^{+}_{2}) (fm) 2.709 2.688 2.648 2.636 2.635 2.625 2.609 2.589 2.567
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (01+{}^{+}_{1}) -0.0002832 0.3766 0.6783 0.8871 1.025 1.118 1.182 1.226 1.257
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (21+{}^{+}_{1}) -0.0007262 0.09012 0.2824 0.6649 0.9164 1.038 1.114 1.167 1.203
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (22+{}^{+}_{2}) -0.002162 0.3583 0.4459 0.2394 0.1156 0.09424 0.09968 0.1135 0.1317
𝑺2\langle\bm{S}^{2}\rangle (01+{}^{+}_{1}) 0.001527 0.06294 0.2080 0.3717 0.5181 0.6376 0.7311 0.8028 0.8574
𝑺2\langle\bm{S}^{2}\rangle (21+{}^{+}_{1}) 0.002947 0.02264 0.1166 0.3520 0.5470 0.6632 0.7441 0.8049 0.8514
𝑺2\langle\bm{S}^{2}\rangle (22+{}^{+}_{2}) 0.002436 0.1035 0.2126 0.1503 0.09792 0.1056 0.1363 0.1785 0.2284
BB(E2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 2.952 3.615 6.473 11.14 11.82 10.61 9.222 8.005 7.006
BB((E2)n: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 18.12 18.47 19.47 17.46 12.72 9.508 7.411 5.944 4.883
BB(IS2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 35.69 38.42 48.39 56.49 49.06 40.20 33.17 27.75 23.59
BB(IV2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 6.442 5.740 3.491 0.7058 0.01631 0.03004 0.09894 0.1531 0.1911
BB(E2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 16.14 14.56 9.867 3.228 0.6455 0.1297 0.01963 0.0001363 0.006089
BB((E2)n: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 5.861 4.443 1.108 0.4739 2.640 3.521 3.620 3.448 3.216
BB(IS2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 41.46 35.09 17.59 1.228 0.6747 2.299 3.106 3.404 3.502
BB(IV2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 2.549 2.917 4.363 6.175 5.897 5.002 4.173 3.491 2.943
BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (e2e^{2} fm4) 12.75 15.30 22.45 15.92 4.390 1.114 0.2748 0.05108 0.001385
BB((E2)n: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 0.5122 1.971 12.25 25.59 17.21 10.17 6.362 4.169 2.807
BB(IS2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 18.37 28.25 67.87 81.88 38.98 18.01 9.281 5.143 2.933
BB(IV2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 8.149 6.288 1.531 1.142 4.213 4.551 3.992 3.297 2.684

Table 1 shows the calculated binding energies (BE). The experimental data are -65.07, -61.70, and -59.11 MeV for 01+{}^{+}_{1}, 21+{}^{+}_{1}, and 22+{}^{+}_{2}, respectively. By changing the strength VLSV_{\rm LS} in the range 0–4000 MeV, the binding energies are drastically changed. A large VLSV_{\rm LS} value results in strong binding energy. On the other hand, a small VLSV_{\rm LS} value results in weak binding energy. The calculated values were almost identical to the experimental data around 2500 MeV. However, we have taken 2000 MeV as a criterion for VLSV_{\rm LS}, because the effect of the α+t+t\alpha+t+t cluster structure is not included in this paper. The effect of the α\alpha cluster breaking and recombination gives a deeper binding energy Itagaki et al. (2008).

Table 1 also shows the calculated root mean squared radii for the point proton (rpr_{p}), point neutron (rnr_{n}), and point nucleon matter (rmr_{m}) of the 01+{}^{+}_{1}, 21+{}^{+}_{1}, and 22+{}^{+}_{2} states. The experimental values of the proton and matter radii of the 10Be ground state are 2.357 ±\pm 0.018 fm N ortersh auser et al. (2009) and 2.39 ±\pm 0.02 fm Tanihata et al. (1985), respectively. The calculated radii are very close to the experimental data around VLSV_{\rm LS} = 2500 MeV. The increase in the strength of the spin-orbit interaction is responsible for the small size of the point nucleon-matter, neutron, and proton because of the strong binding. The size of the 01+{}^{+}_{1} and 21+{}^{+}_{1} states show consistent behaviors, especially with the strong binding. On the other hand, the 22+{}^{+}_{2} state, which is larger than the 01+{}^{+}_{1} and 21+{}^{+}_{1} states except for very small VLSV_{\rm LS} values, exhibits much gentler shrinkage behavior with increasing binding energy. This result implies that the structure of the 22+{}^{+}_{2} state is quite different from that of the ground and 21+{}^{+}_{1} states when strong spin-orbit interaction is applied. Indeed, the 22+{}^{+}_{2} state with K=2K=2 corresponds to the excitation of one neutron from the spin-orbit favored orbit to the unfavored one according to the simple molecular-orbital picture.

In order to gain more precise information, we present the expectation values of 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle and 𝑺2\langle\bm{S}^{2}\rangle for the neutron in Table 1. The expectation values of the proton part are 0 because all protons are in the α\alpha clusters. The 01+{}^{+}_{1} and 21+{}^{+}_{1} states clearly exhibit similar growth of the expectation value with changing the strength of the spin-orbit interaction. Thus, the 01+0^{+}_{1} and 21+2^{+}_{1} states have similar inner structures and undergo similar changes with increasing strength of the spin-orbit interaction. The expectation value of the 22+{}^{+}_{2} state shows a different trend, unlike the behavior of the 01+0^{+}_{1} and 21+2^{+}_{1} states. This finding implies that the inner structure of the 22+{}^{+}_{2} state is different from the structures of the 01+{}^{+}_{1} and 21+{}^{+}_{1} states when the strong spin-orbit interaction is applied.

Next, we see the quadrupole transition strengths between each state. Table 1 also shows the quadrupole transition strengths (BB(E2), the neutron part BB((E2)n), BB(IS2), and BB(IV2)) from the 21+{}^{+}_{1} state to the 01+{}^{+}_{1} state, from the 22+{}^{+}_{2} state to the 01+{}^{+}_{1} state, and from the 22+{}^{+}_{2} state to the 21+{}^{+}_{1} state. Although the radii and expectation values of the 01+{}^{+}_{1} and 21+{}^{+}_{1} states show similar tendencies, the change in the transition strengths of BB(E2) and BB((E2)n) from the 21+{}^{+}_{1} state to the 01+{}^{+}_{1} state is not simple. Under weak spin-orbit interaction, the strengths of the proton and neutron parts are quite different. With increasing the VLSV_{\rm LS} value, the transition strength of the proton part becomes large. For VLSV_{\rm LS} = 2000–4000 MeV, both the proton and neutron parts decrease together. This behavior is caused by the sign reversal of the transition density for the neutron part as mentioned in Ref. Furumoto et al. (2021). From another perspective, we see IS and IV transition strengths. The obtained IS transition strengths from 21+{}^{+}_{1} to 01+{}^{+}_{1} stay in the range of 20–60 fm4. The IV transition strengths from 21+{}^{+}_{1} to 01+{}^{+}_{1} get gradually small as VLSV_{\rm LS} grows. On the other hand, the IS transition strengths from 22+{}^{+}_{2} to 01+{}^{+}_{1} are drastically changed by the VLSV_{\rm LS} value. This effect on the cross section will be discussed later. Here, we also discuss the transition strength from the 22+{}^{+}_{2} state to the 21+{}^{+}_{1} state. The BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value becomes smaller when the strength of the VLSV_{\rm LS} value becomes larger. In Ref. Itagaki et al. (2002), it is mentioned that the increase of the BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value with the decrease of the VLSV_{\rm LS} value supports a triaxial α\alpha + α\alpha + dineutron clustering configuration. However, the BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) values with VLSV_{\rm LS} = 0 and 500 MeV are smaller than that with 1000 MeV. This is considered to be caused by the further development of the dineutron cluster. Namely, the coupling pattern of the angular momentum among the two α\alpha clusters and the dineutron cluster is different in the 21+{}^{+}_{1} and 22+{}^{+}_{2} states. Concretely, when the small VLSV_{\rm LS} value is adopted, it is considered that the two α\alpha clusters with the relative angular momentum L=0L=0 are synthesized with the dineutron around them with L=2L=2 in the 21+{}^{+}_{1} state. On the other hand, the two α\alpha clusters with the relative angular momentum L=2L=2 are synthesized with the dineutron moving around them with L=0L=0 in the 22+{}^{+}_{2} state. The decrease of the BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value and the increase of the BB(IV2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value corroborate the situation. We will discuss this situation again in Sec. III.3.

Refer to caption
Figure 1: (a) Elastic cross section, (b) inelastic cross section for the 21+{}^{+}_{1} state, and (c) inelastic cross section for the 22+{}^{+}_{2} state of 10Be + p system at E/A=E/A= 59.4 MeV. The detail for the curves is written in the text. The experimental data are taken from EXF ; Cortina-Gil et al. (1997); Iwasaki et al. (2000).
Refer to caption
Figure 2: Same as Fig. 1 but at E/A=E/A= 200 MeV.
Refer to caption
Figure 3: Same as Fig. 1 but for the 12C target. The experimental data are taken from EXF ; Cortina-Gil et al. (1997).
Refer to caption
Figure 4: Same as Fig. 3 but at E/A=E/A= 200 MeV.

Figure 1 shows the (a) elastic cross section, (b) inelastic cross section for the 21+{}^{+}_{1} state, and (c) inelastic cross section for the 22+{}^{+}_{2} state of the 10Be nucleus by the proton target at E/A=E/A= 59.4 MeV. The two-dot-dashed, dot-dashed, dashed, dotted, bold-solid, bold(red)-dotted, bold(red)-dashed, bold(red)-dot-dashed, and bold(red)-two-dot-dashed curves are obtained with VLSV_{LS} = 0, 500, 1000, 1500, 2000, 2500, 3000, 3500, and 4000 MeV, respectively. The experimental data are well reproduced in a wide range of the VLSV_{\rm LS} values. The change in the size of the ground state with varying VLSV_{\rm LS} slightly affects the elastic cross section. The relation among the binding energy, the nuclear size, and the elastic cross section will be discussed in Sec. III.2 in detail. The visible change in the transition strength from the 21+{}^{+}_{1} state to the 01+{}^{+}_{1} state for the proton and neutron parts results in a slight change in the inelastic cross section. As mentioned above, the BB(IS2) values are obtained within 20–60 fm4. Therefore, the calculated inelastic cross sections are similar to each other. On the other hand, the calculated inelastic cross sections for the 22+{}^{+}_{2} state are greatly dependent on the VLSV_{\rm LS} value adopted in the structure calculation. The drastic change in the inelastic cross section is caused by the difference in the transition strengths, as shown in Table 1. As mentioned in Ref. Furumoto et al. (2021), the behavior of the neutron part, in particular, is important and affects the IS transition strength from the 22+{}^{+}_{2} state to the 01+{}^{+}_{1} state. Here, we mention that the transition strength from the 22+{}^{+}_{2} state to the 21+{}^{+}_{1} state cannot be ignored. Therefore, the multistep reaction effect (01+{}^{+}_{1} \to 21+{}^{+}_{1} \to 22+{}^{+}_{2}) also contributes and makes the inelastic cross section for the 22+{}^{+}_{2} state at E/A=E/A= 59.4 MeV complicated. To avoid the multistep reaction effect, we also calculate the elastic and inelastic cross sections at a higher energy at which the multistep reaction effect is considered to be minor. In fact, we confirmed that the multistep reaction effect arising from the transition from the 21+{}^{+}_{1} state to the 22+{}^{+}_{2} state is minor at 200 MeV. Figure 2 shows the calculated (a) elastic cross section, (b) inelastic cross section for the 21+{}^{+}_{1} state, and (c) inelastic cross section for the 22+{}^{+}_{2} state at E/A=E/A= 200 MeV. The inelastic cross section for the 22+{}^{+}_{2} state is drastically influenced by the choice of the spin-orbit strength for the structure calculation, and this choice affects the inner structure of 10Be. On the other hand, it is difficult to distinguish the effect of the VLSV_{\rm LS} parameter on the elastic cross section and the inelastic cross section for the 21+{}^{+}_{1} state.

We also calculate the elastic and inelastic cross sections for the 10Be + 12C system at E/A=E/A= 59.4 and 200 MeV to investigate the effect of a different target. Figures 3 and 4 show the (a) elastic cross section, (b) inelastic cross section for the 21+{}^{+}_{1} state, and (c) inelastic cross section for the 22+{}^{+}_{2} state of the 10Be + 12C system at E/A=E/A= 59.4 and 200 MeV. The difference in the nuclear size has a minor effect on the elastic cross sections for the 12C target. The inelastic cross sections for the 21+{}^{+}_{1} state for the 12C target have similar behavior to each other. Also, we can see the drastic change of the inelastic cross sections for the 22+{}^{+}_{2} state. Here, we note that the calculated inelastic cross sections for the 22+{}^{+}_{2} state show different behavior in comparison with the proton target, especially for the dotted and bold solid curves. The results are caused by the weak IS transition strength shown in Table 1. In the present calculation for the 12C target, the IV component has no effect on the cross section. Comparing the proton target with 12C, the effect of IS and IV components can be seen.

III.1.2 Dependence of MM

Next, we investigate the dependence of the Majorana (M)(M) parameter. The MM parameter is responsible for describing the nucleon-nucleon exchange effect and is related to the Wigner (WW) parameter as W=1MW=1-M. The values of 0.56–0.63 are widely used in the cluster model calculations. For the 10Be nucleus, 0.56 or 0.60 is usually adopted. Therefore, we investigate the range of MM = 0.52–0.64, which is wider than the usual cases, in this paper.

Table 2: Same as Table 1 but for MM = 0.52–0.64.
MM 0.52 0.54 0.56 0.58 0.60 0.62 0.64
BE (01+{}^{+}_{1}) (MeV) -77.07 -73.08 -69.39 -66.01 -62.97 -60.26 -57.90
BE (21+{}^{+}_{1}) (MeV) -74.22 -70.17 -66.38 -62.91 -59.78 -57.05 -54.73
BE (22+{}^{+}_{2}) (MeV) -69.52 -66.18 -63.11 -60.29 -57.72 -55.40 -53.34
rpr_{p} (01+{}^{+}_{1}) (fm) 2.160 2.205 2.258 2.320 2.393 2.479 2.579
rpr_{p} (21+{}^{+}_{1}) (fm) 2.139 2.180 2.231 2.296 2.380 2.488 2.617
rpr_{p} (22+{}^{+}_{2}) (fm) 2.237 2.286 2.341 2.404 2.474 2.557 2.660
rnr_{n} (01+{}^{+}_{1}) (fm) 2.298 2.357 2.426 2.506 2.598 2.702 2.816
rnr_{n} (21+{}^{+}_{1}) (fm) 2.292 2.346 2.411 2.494 2.597 2.722 2.863
rnr_{n} (22+{}^{+}_{2}) (fm) 2.446 2.509 2.579 2.655 2.737 2.828 2.933
rmr_{m} (01+{}^{+}_{1}) (fm) 2.244 2.297 2.360 2.433 2.518 2.615 2.724
rmr_{m} (21+{}^{+}_{1}) (fm) 2.232 2.281 2.341 2.416 2.512 2.631 2.767
rmr_{m} (22+{}^{+}_{2}) (fm) 2.365 2.423 2.487 2.558 2.635 2.723 2.827
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (01+{}^{+}_{1}) 1.210 1.177 1.136 1.085 1.025 0.9571 0.8816
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (21+{}^{+}_{1}) 1.121 1.091 1.050 0.9938 0.9164 0.8123 0.6919
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (22+{}^{+}_{2}) 0.08979 0.08770 0.08810 0.1038 0.1156 0.1560 0.2073
𝑺2\langle\bm{S}^{2}\rangle (01+{}^{+}_{1}) 0.7115 0.6723 0.6271 0.5755 0.5181 0.4560 0.3915
𝑺2\langle\bm{S}^{2}\rangle (21+{}^{+}_{1}) 0.7017 0.6742 0.6416 0.6011 0.5470 0.4731 0.3835
𝑺2\langle\bm{S}^{2}\rangle (22+{}^{+}_{2}) 0.1009 0.09268 0.08663 0.08654 0.09792 0.1241 0.1542
BB(E2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 6.049 7.000 8.226 9.811 11.82 14.26 17.17
BB((E2)n: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 3.916 4.981 6.557 8.970 12.72 18.35 26.07
BB(IS2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 19.70 23.79 29.47 37.54 49.06 64.96 85.55
BB(IV2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 0.2309 0.1713 0.09447 0.01885 0.01631 0.2579 0.9271
BB(E2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 0.02127 0.04007 0.09132 0.2363 0.6455 1.704 3.907
BB((E2)n: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 2.793 3.039 3.202 3.141 2.640 1.592 0.4369
BB(IS2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 2.327 2.382 2.212 1.654 0.6747 0.001903 1.731
BB(IV2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 3.302 3.777 4.375 5.100 5.897 6.589 6.958
BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (e2e^{2} fm4) 0.09201 0.2346 0.6204 1.666 4.390 10.60 21.48
BB((E2)n: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 4.574 5.816 7.856 11.32 17.21 26.41 38.68
BB(IS2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 5.963 8.387 12.89 21.68 38.98 70.46 117.8
BB(IV2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 3.368 3.715 4.061 4.302 4.213 3.548 2.513

Table 2 shows calculated values of binding energies, radii, expectation values, and quadrupole transition strengths. Not only the VLSV_{\rm LS} parameter but also the MM parameter give drastic changes in the binding energies. With the increase of MM, the repulsive effect becomes larger. Therefore, the large (small) MM value gives weak (strong) binding. However, it is found that MM has a minor effect on the excitation energy of the 21+{}^{+}_{1} state. On the contrary, when the MM parameter is large, the difference of the energies between the 21+{}^{+}_{1} and 22+{}^{+}_{2} states becomes small. The size of the ground and excited states are also influenced by the change in the binding energy. The strong binding gives the small size for the ground and excited states. Therefore, the trend of the dependence of size on the MM parameter is simple. Also, the expectation values show a simple increase or decrease, except for the 𝑺2\langle\bm{S}^{2}\rangle value of 22+{}^{+}_{2} state, which shows minor dependence on the MM value.

Next, we discuss the transition strength. Both of the proton and neutron parts of the transition strengths from the 21+{}^{+}_{1} state to the 01+{}^{+}_{1} state simply increase with the MM parameter. The increase is concerned with the IS component. For the transition strength from the 22+{}^{+}_{2} state to the 01+{}^{+}_{1} state, the proton part increases, but the neutron part decreases with the MM parameter. The increase of the proton part and the decrease of the neutron part give complicated transition strength of the IS and IV components. The IV component of the transition strength from the 22+{}^{+}_{2} state to the 01+{}^{+}_{1} state is always larger than the IS component. This result is also different in comparison with the VLSV_{\rm LS} case. In addition, the transition strength from the 22+{}^{+}_{2} state to the 21+{}^{+}_{1} state gets larger with the MM parameter. This indicates that we cannot ignore the multistep reaction effect on the inelastic cross section caused by the strong transition from the 21+{}^{+}_{1} state to the 22+{}^{+}_{2} state.

Refer to caption
Figure 5: Same as Fig. 1 but for MM = 0.52–0.64. The detail is written in the text.
Refer to caption
Figure 6: Same as Fig. 5 but at E/AE/A = 200 MeV.
Refer to caption
Figure 7: Same as Fig. 5 but for the 12C target.
Refer to caption
Figure 8: Same as Fig. 6 but for the 12C target.

Figures 5 and 6 show the calculated elastic and inelastic cross sections by the proton target with the experimental data. The two-dot-dashed, dot-dashed, dashed, dotted, bold-solid, bold(red)-dotted, and bold(red)-dashed curves are obtained with MM = 0.52, 0.54, 0.56, 0.58, 0.60, 0.62, and 0.64, respectively. The effect of changing the nuclear size is barely visible on the elastic cross section. We will discuss the effect of the binding energy, nuclear size, and elastic cross section again in Sec. III.2. The effect of the change of the transition strength from the 21+{}^{+}_{1} state to the 01+{}^{+}_{1} state is barely visible on the inelastic cross section for the 21+{}^{+}_{1} state. On the contrary, we can see the drastic change of the inelastic cross sections for the 22+{}^{+}_{2} state. In Ref. Furumoto et al. (2021), we expected that the change of the MM parameter would not have much impact on the inelastic cross section. However, it indeed does give the change. Here, we compare the inelastic cross sections for the 22+{}^{+}_{2} state at E/A=E/A= 59.4 with 200 MeV. At 59.4 MeV, the multistep reaction effect caused by the strong transition strength from the 22+{}^{+}_{2} state to the 21+{}^{+}_{1} state gives complicated angular distribution. On the other hand, we can discuss the effect of changing the MM parameter on the inelastic cross section for the 22+{}^{+}_{2} state at 200 MeV because the multistep reaction effect can be ignored at higher incident energy. The effect of changing MM is indeed seen on the inelastic cross section for the 22+{}^{+}_{2} state at 200 MeV as shown in Fig. 6. Although this is smaller compared with the change of the VLSV_{\rm LS} parameter shown in Fig. 2, we cannot ignore the effect. Therefore, we will discuss the contribution of the VLSV_{\rm LS} and MM parameters simultaneously in Sec. III.2.

Figures 7 and 8 show the calculated elastic and inelastic cross sections by the 12C target with the experimental data. Again, the change in the nuclear size has a minor effect on the elastic cross sections for the 12C target. The inelastic cross sections for the 21+{}^{+}_{1} state for the 12C target show similar behavior to that for the proton target. Also, we can see the drastic change of the inelastic cross sections for the 22+{}^{+}_{2} state. However, the behavior of the inelastic cross sections obtained with weak IS transition to the 22+{}^{+}_{2} state is slightly different in comparison with the proton target. This is caused by the small transition strength of the IS component. Again, we note that the IV component has no effect on the present calculation for the 12C target.

III.1.3 Dependence of B,HB,H

Next, we investigate the dependence of the BB and HH parameters. The role of these parameters is to adjust the relative strength of the proton-proton (neutron-neutron) and proton-neutron interactions. The original Volkov interaction has no BB and HH terms. However, not only deuteron but also two neutrons are bound within B=H=0B=H=0. Therefore, the BB and HH are often applied to give a realistic condition with the Volkov interaction.

Table 3: Same as Table 1 but for B=HB=H = 0–0.20.
B=HB=H 0 0.04 0.08 0.12 0.16 0.20
BE (01+{}^{+}_{1}) (MeV) -63.85 -63.39 -62.97 -62.57 -62.20 -61.85
BE (21+{}^{+}_{1}) (MeV) -60.58 -60.17 -59.78 -59.42 -59.09 -58.78
BE (22+{}^{+}_{2}) (MeV) -58.49 -58.10 -57.72 -57.37 -57.03 -56.71
rpr_{p} (01+{}^{+}_{1}) (fm) 2.398 2.396 2.393 2.391 2.390 2.388
rpr_{p} (21+{}^{+}_{1}) (fm) 2.387 2.383 2.380 2.378 2.377 2.376
rpr_{p} (22+{}^{+}_{2}) (fm) 2.470 2.472 2.474 2.477 2.480 2.482
rnr_{n} (01+{}^{+}_{1}) (fm) 2.591 2.594 2.598 2.602 2.606 2.611
rnr_{n} (21+{}^{+}_{1}) (fm) 2.591 2.593 2.597 2.601 2.605 2.611
rnr_{n} (22+{}^{+}_{2}) (fm) 2.715 2.726 2.737 2.749 2.761 2.773
rmr_{m} (01+{}^{+}_{1}) (fm) 2.516 2.517 2.518 2.520 2.522 2.525
rmr_{m} (21+{}^{+}_{1}) (fm) 2.511 2.511 2.512 2.514 2.516 2.520
rmr_{m} (22+{}^{+}_{2}) (fm) 2.620 2.627 2.635 2.643 2.652 2.660
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (01+{}^{+}_{1}) 0.9680 0.9975 1.025 1.052 1.077 1.099
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (21+{}^{+}_{1}) 0.8667 0.8924 0.9164 0.9381 0.9574 0.9739
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (22+{}^{+}_{2}) 0.1217 0.1189 0.1156 0.1121 0.1083 0.1045
𝑺2\langle\bm{S}^{2}\rangle (01+{}^{+}_{1}) 0.4484 0.4827 0.5181 0.5544 0.5913 0.6285
𝑺2\langle\bm{S}^{2}\rangle (21+{}^{+}_{1}) 0.4658 0.5055 0.5470 0.5900 0.6414 0.6791
𝑺2\langle\bm{S}^{2}\rangle (22+{}^{+}_{2}) 0.09248 0.09534 0.09792 0.1002 0.1022 0.1040
BB(E2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 11.98 11.90 11.82 11.76 11.71 11.67
BB((E2)n: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 13.11 12.90 12.72 12.54 12.39 12.25
BB(IS2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 50.15 49.58 49.06 48.60 48.19 47.83
BB(IV2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 0.02527 0.02055 0.01631 0.01262 0.009488 0.006893
BB(E2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 0.7458 0.6949 0.6455 0.5982 0.5534 0.5112
BB((E2)n: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 2.552 2.597 2.640 2.681 2.719 2.754
BB(IS2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 0.5384 0.6051 0.6747 0.7464 0.8191 0.8919
BB(IV2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 6.056 5.978 5.897 5.812 5.726 5.638
BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (e2e^{2} fm4) 4.965 4.677 4.390 4.108 3.834 3.569
BB((E2)n: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 18.18 17.70 17.21 16.70 16.18 15.66
BB(IS2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 42.15 40.57 38.98 37.37 35.77 34.17
BB(IV2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 4.144 4.180 4.213 4.241 4.262 4.275

Table 3 shows calculated values of binding energies, radii, expectation values, and quadrupole transition strengths. Almost all the calculated values show a minor dependence on the change of the BB and HH parameters. The expectation value of 𝑺2\langle\bm{S}^{2}\rangle for the 01+{}^{+}_{1}, 21+{}^{+}_{1} and 21+{}^{+}_{1} states and the transition strength from the 22+{}^{+}_{2} state to the 01+{}^{+}_{1} state are slightly affected. However, their causal relationship is not clear.

Refer to caption
Figure 9: Same as Fig. 1 but with B=HB=H = 0–0.20. The detail is written in the text.
Refer to caption
Figure 10: Same as Fig. 9 but at E/AE/A = 200 MeV.
Refer to caption
Figure 11: Same as Fig. 9 but for the 12C target.
Refer to caption
Figure 12: Same as Fig. 10 but for the 12C target.

Figures 9 and 10 show the calculated elastic and inelastic cross sections for the proton target with the experimental data. The dashed, dotted, bold-solid, bold(red)-dotted, bold(red)-dashed, and bold(red)-dot-dashed curves are obtained with B=HB=H = 0.00, 0.04, 0.08 0.12, 0.16, and 0.20, respectively. Again, the effect of changing the BB and HH values is minor in the elastic and inelastic cross sections. In the low-lying states of 10Be, the BB and HH parameters are found to play a minor role. Nevertheless, “the bound two neutrons” is unphysical, and these parameters allow the elimination of such conditions; the application of the BB and HH parameters is to reproduce a realistic physical situation even if the effect is small. Figures 11 and 12 show the calculated elastic and inelastic cross sections for the 12C target with the experimental data. Again, we cannot see the effect of changing the BB and HH parameters in the elastic and inelastic cross sections for the 12C target. These results imply that it is difficult to see the difference of the BB and HH parameters in the elastic and inelastic cross sections.

III.2 Effect of binding energy of the ground state

In the above subsections, we have only discussed the parameter dependence in nuclear structure calculations. That is, we did not specifically consider realistic physical points (e.g., binding energies, etc.). In this subsection, we adjust the VLSV_{\rm LS} and MM parameters so that the binding energies of different parameter sets are consistently reproduced to each other as in Ref. Itagaki et al. (2002). In this paper, we first fix the VLSV_{\rm LS} value in the range of 0–4000 MeV and adjust the MM parameter to obtain the appropriate binding energy. On the contrary, if the MM parameter is first fixed in the range of 0.52–0.64, the appropriate VLSV_{\rm LS} value could not be obtained for the small MM values of 0.52–0.56, when the constraint of reproducing the binding energy is imposed. The results are summarized in Table 4.

Table 4: Same as Table 1 but for (VLS(MeV),M)(V_{\rm LS}\ {\rm(MeV)},M) = (0, 0.57), (500, 0.57), (1000, 0.58), (1500,0.59), (2000,0.60), (2500,0.61), (3000,0.63), (3500,0.64), and (4000,0.65).
VLSV_{\rm LS} (MeV) 0 500 1000 1500 2000 2500 3000 3500 4000
MM 0.57 0.57 0.58 0.59 0.60 0.61 0.63 0.64 0.65
BE (01+{}^{+}_{1}) (MeV) -62.79 -63.15 -62.79 -62.77 -62.97 -63.34 -62.33 -62.91 -63.61
BE (21+{}^{+}_{1}) (MeV) -60.78 -60.90 -60.05 -59.72 -59.78 -60.07 -58.98 -59.52 -60.18
BE (22+{}^{+}_{2}) (MeV) -59.27 -59.64 -59.04 -58.40 -57.72 -55.67 -54.70 -54.85 -55.08
rpr_{p} (01+{}^{+}_{1}) (fm) 2.433 2.418 2.418 2.408 2.393 2.376 2.398 2.377 2.355
rpr_{p} (21+{}^{+}_{1}) (fm) 2.410 2.407 2.419 2.402 2.380 2.360 2.388 2.364 2.340
rpr_{p} (22+{}^{+}_{2}) (fm) 2.388 2.374 2.397 2.438 2.474 2.504 2.575 2.603 2.635
rnr_{n} (01+{}^{+}_{1}) (fm) 2.681 2.660 2.651 2.628 2.598 2.565 2.580 2.543 2.505
rnr_{n} (21+{}^{+}_{1}) (fm) 2.660 2.655 2.666 2.634 2.597 2.561 2.582 2.543 2.505
rnr_{n} (22+{}^{+}_{2}) (fm) 2.639 2.621 2.645 2.695 2.737 2.770 2.846 2.872 2.898
rmr_{m} (01+{}^{+}_{1}) (fm) 2.585 2.566 2.560 2.542 2.518 2.491 2.509 2.478 2.446
rmr_{m} (21+{}^{+}_{1}) (fm) 2.563 2.559 2.570 2.544 2.512 2.482 2.506 2.473 2.440
rmr_{m} (22+{}^{+}_{2}) (fm) 2.542 2.525 2.549 2.595 2.635 2.667 2.741 2.767 2.796
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (01+{}^{+}_{1}) -0.00007341 0.4572 0.7533 0.9237 1.026 1.091 1.110 1.145 1.172
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (21+{}^{+}_{1}) -0.0006060 0.1090 0.3788 0.7384 0.9164 1.006 1.033 1.078 1.112
𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle (22+{}^{+}_{2}) -0.001788 0.4060 0.4069 0.1962 0.1156 0.09737 0.09827 0.1051 0.1307
𝑺2\langle\bm{S}^{2}\rangle (01+{}^{+}_{1}) 0.001095 0.08877 0.2521 0.4007 0.5181 0.6097 0.6547 0.7160 0.7670
𝑺2\langle\bm{S}^{2}\rangle (21+{}^{+}_{1}) 0.002028 0.02980 0.1667 0.3979 0.5470 0.6399 0.6839 0.7393 0.7844
𝑺2\langle\bm{S}^{2}\rangle (22+{}^{+}_{2}) 0.001607 0.1232 0.1971 0.1250 0.09792 0.1055 0.1232 0.1457 0.1756
BB(E2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 1.817 2.594 6.401 10.67 11.82 11.80 12.84 12.27 11.60
BB((E2)n: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 13.53 13.95 16.05 14.83 12.72 11.31 12.28 11.20 10.25
BB(IS2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 25.26 28.58 42.73 50.67 49.06 46.20 50.24 46.93 43.66
BB(IV2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}) (fm4) 5.429 4.514 2.181 0.3407 0.01631 0.005189 0.006227 0.02422 0.04227
BB(E2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (e2e^{2} fm4) 11.77 10.32 6.559 2.117 0.6455 0.2236 0.1388 0.03778 0.0009486
BB((E2)n: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 3.594 2.303 0.1438 1.022 2.640 3.439 3.758 4.007 4.169
BB(IS2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 28.38 22.38 8.646 0.1970 0.6747 1.909 2.452 3.267 4.044
BB(IV2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}) (fm4) 2.358 2.874 4.760 6.081 5.897 5.417 5.341 4.823 4.295
BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (e2e^{2} fm4) 8.154 11.22 18.98 11.34 4.390 1.851 1.408 0.6334 0.2230
BB((E2)n: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 0.002228 0.9923 13.58 22.47 17.21 12.55 11.63 8.580 6.004
BB(IS2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 8.426 18.89 64.66 65.73 38.98 24.05 21.13 13.88 8.542
BB(IV2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) (fm4) 7.886 5.539 0.4507 1.886 4.213 4.764 4.944 4.551 3.913

Table 4 shows the calculated values of binding energies, radii, expectation values, and quadrupole transition strengths with the VLSV_{\rm LS} and MM values obtained with parameters adjusting the binding energy of the ground state. The binding energies of the ground state are obtained within the deviation of 1 MeV from the set of VLSV_{\rm LS} = 2000 MeV and MM = 0.60. The parameter set is also shown in Table 4. On the other hand, the excitation energies of the 21+{}^{+}_{1} and 22+{}^{+}_{2} states still depend on the set of the VLSV_{\rm LS} and MM values. Here, we notice that the effect of the VLSV_{\rm LS} parameter is dominant for the excitation energy. By adjusting the binding energy of the ground state, the nuclear sizes of the ground state are obtained almost consistently. The expectation values of 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle and 𝑺2\langle\bm{S}^{2}\rangle are drastically dependent on the parameter set; they are strongly dependent on the VLSV_{\rm LS} parameter. Namely, the property of the 10Be nucleus strongly depends on the VLSV_{\rm LS} parameter even if we adjust the binding energies of the ground state.

For the proton part of the transition strength from the 21+{}^{+}_{1} state to the 01+{}^{+}_{1} state, the difference of the VLSV_{\rm LS} and MM values is not clearly seen. On the other hand, the neutron part shows that the change of the VLSV_{\rm LS} parameter has a significant effect. For the transition strength from the 22+{}^{+}_{2} state to the 21+{}^{+}_{1} state, the contribution of the VLSV_{\rm LS} parameter is dominant. Namely, the obtained nuclear structure information is strongly affected by the VLSV_{\rm LS} parameter even if the energies of the ground state are consistently by simultaneously changing the VLSV_{\rm LS} and MM parameters.

Refer to caption
Figure 13: Same as Fig. 1 but with the modification of MM. The detail is written in the text. In addition, the (blue) solid curve is the result obtained with the dineutron basis. The detail of the solid curve is introduced in the next section.
Refer to caption
Figure 14: Same as Fig. 13 but at E/A=E/A= 200 MeV.
Refer to caption
Figure 15: Same as Fig. 13 but for the 12C target.
Refer to caption
Figure 16: Same as Fig. 14 but for the 12C target.

Figures 13 and 14 show the calculated elastic and inelastic cross sections for the proton target with the experimental data. The two-dot-dashed, dot-dashed, dashed, dotted, bold-solid, bold(red)-dotted, bold(red)-dashed, bold(red)-dot-dashed, and bold(red)-two-dot-dashed curves are obtained with (VLS(MeV),M)(V_{\rm LS}\ {\rm(MeV)},M) = (0, 0.57), (500, 0.57), (1000, 0.58), (1500,0.59), (2000, 0.60), (2500, 0.61), (3000, 0.63), (3500, 0.64), and (4000, 0.65), respectively. The meaning of the (blue) solid curves will be explained in the next subsection. As mentioned before, adjusting the binding energy results in a similar nuclear size. We found that this gives similar elastic cross sections. The inelastic cross section for the 21+{}^{+}_{1} state is slightly affected by the adopted set of the VLSV_{\rm LS} and MM parameters. On the other hand, the drastic change can be seen in the inelastic cross section for the 22+{}^{+}_{2} state. In addition, the results are similar to Figs. 1 and 2 which are obtained by changing only the VLSV_{\rm LS} parameter.

Figures 15 and 16 show the calculated elastic and inelastic cross sections for the 12C target with the experimental data. Again, we can see the consistent results of the elastic cross sections owing to a similar nuclear size. In addition, we can see the drastic change of the inelastic cross section for the 22+{}^{+}_{2} state. These results are also similar to Figs. 3 and 4. Namely, the obtained results support the strong contribution of the VLSV_{\rm LS} parameter even if the energy of the ground state is consistently reproduced to each other by varying the VLSV_{\rm LS} and MM parameters simultaneously.

III.3 Reconfirmation of behavior of inelastic cross section dependent on development and breaking of dineutron correlation

Next, we reconfirm the characteristic behavior of the inelastic cross section for the 22+{}^{+}_{2} state depending on the development and breaking of the dineutron correlation. We use the wave function constructed in the previous subsection and investigate the dineutron correlation in 10Be. To describe the dineutron correlation, we prepare the dineutron cluster as

Ψi=𝒜[ϕα(𝒓14,𝑹1)ϕα(𝒓58,𝑹2)ϕ2n(𝒓910,𝑹3)]i,\Psi_{i}={\cal A}\big{[}\phi_{\alpha}(\bm{r}_{1-4},\bm{R}_{1})\phi_{\alpha}(\bm{r}_{5-8},\bm{R}_{2})\phi_{2n}(\bm{r}_{9-10},\bm{R}_{3})\big{]}_{i}, (7)

where the positions of the centers of the wave packets for the two valence neutrons are the same. Here, the valence neutrons have spin up and down. Therefore, the dineutron cluster fully satisfies the condition of the dineutron correlation (S=0S=0 and large spatial overlap). We fix the MM parameter to be 0.54 to reproduce the binding energy of the ground state in the same manner as in the previous subsection.

With the dineutron cluster wave function, the obtained binding energies are -63.46, -61.33, and -60.40 MeV for 01+{}^{+}_{1}, 21+{}^{+}_{1}, and 22+{}^{+}_{2} states, respectively. The calculated radii are 2.318, 2.289, 2.256, 2.445, 2.401, 2.386, 2.395, 2.357, and 2.335 fm for rpr_{p} (01+{}^{+}_{1}), rpr_{p} (21+{}^{+}_{1}), rpr_{p} (22+{}^{+}_{2}), rnr_{n} (01+{}^{+}_{1}), rnr_{n} (21+{}^{+}_{1}), rnr_{n} (22+{}^{+}_{2}), rmr_{m} (01+{}^{+}_{1}), rmr_{m} (21+{}^{+}_{1}), and rmr_{m} (22+{}^{+}_{2}), respectively. The transition strengths are 1.677, 8.898, 18.30, 2.849, 7.940, 1.647, 16.82, 2.354, 7.434, 0.2712, 10.54, and 4.865 (e2e^{2})fm4 for BB(E2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}), BB((E2)n: 21+{}^{+}_{1} \to 01+{}^{+}_{1}), BB(IS2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}), BB(IV2: 21+{}^{+}_{1} \to 01+{}^{+}_{1}), BB(E2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}), BB((E2)n: 22+{}^{+}_{2} \to 01+{}^{+}_{1}), BB(IS2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}), BB(IV2: 22+{}^{+}_{2} \to 01+{}^{+}_{1}), BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}), BB((E2)n: 22+{}^{+}_{2} \to 21+{}^{+}_{1}), BB(IS2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}), and BB(IV2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}), respectively. The excitation energy is similar to the case with the weak VLSV_{\rm LS} parameter rather than the large one. The nuclear size obtained with the pure dineutron cluster is smaller than all results in this paper. It is obvious that the expectation values of 𝑳𝑺\langle\bm{L}\cdot\bm{S}\rangle and 𝑺2\langle\bm{S}^{2}\rangle are zero. The transition strengths are also similar to the weak VLSV_{\rm LS} cases rather than the large one while the nuclear size is small. We note that the BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value is smaller than the results obtained with VLSV_{\rm LS} = 0–1000 MeV shown in Table 1. This small BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value implies the development of the α\alpha + α\alpha + dineutron cluster picture. Again, the coupling pattern of the angular momentum among the two α\alpha clusters and the dineutron cluster is different in the 21+{}^{+}_{1} and 22+{}^{+}_{2} states. Concretely, when the small VLSV_{\rm LS} value is adopted, it is considered that the two α\alpha clusters with the relative angular momentum L=0L=0 are synthesized with the dineutron around them with L=2L=2 in the 21+{}^{+}_{1} state. On the other hand, the two α\alpha clusters with the relative angular momentum L=2L=2 are synthesized with the dineutron moving around them with L=0L=0 in the 22+{}^{+}_{2} state. The decrease of the BB(E2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value and the increase of the BB(IV2: 22+{}^{+}_{2} \to 21+{}^{+}_{1}) value corroborate the situation. In addition, the result of the pure dineutron cluster implies that the developed dineutron cluster can be generated by employing the weak VLSV_{\rm LS} parameter.

Figures 13, 14, 15, and 16 show the result of the pure dineutron cluster state with the (blue) solid curves. The effect of the nuclear size is not clearly seen on the elastic cross section. The results of the pure dineutron cluster state are consistent with those obtained with the weak VLSV_{\rm LS} value, especially for the inelastic cross section of the 22+{}^{+}_{2} state. Again, the development of the dineutron structure by weak VLSV_{\rm LS} parameter is supported.

Table 5: The components of dineutron configurations Cdineutron(Iiπ)C^{\rm dineutron}(I^{\pi}_{i}) defined in Eq. (8). The components are obtained with the wave functions constructed in Secs. III.1.1, III.1.2, and III.2.
VLSV_{\rm LS} (MeV) 0 500 1000 1500 2000 2500 3000 3500 4000
MM=0.60
CdineutronC^{\rm dineutron} (01+{}^{+}_{1}) 0.8516 0.8162 0.7562 0.6952 0.6424 0.5976 0.5577 0.5201 0.4839
CdineutronC^{\rm dineutron} (21+{}^{+}_{1}) 0.8125 0.7955 0.7555 0.6634 0.5763 0.5153 0.4665 0.4252 0.3903
CdineutronC^{\rm dineutron} (22+{}^{+}_{2}) 0.8345 0.7740 0.7074 0.7067 0.7129 0.6994 0.6773 0.6512 0.6229
VLSV_{\rm LS} = 2000 MeV
MM 0.52 0.54 0.56 0.58 0.60 0.62 0.64
CdineutronC^{\rm dineutron} (01+{}^{+}_{1}) 0.5764 0.6003 0.6197 0.6338 0.6424 0.6465 0.6476
CdineutronC^{\rm dineutron} (21+{}^{+}_{1}) 0.4951 0.5187 0.5401 0.5589 0.5763 0.5936 0.6095
CdineutronC^{\rm dineutron} (22+{}^{+}_{2}) 0.7811 0.7761 0.7632 0.7421 0.7129 0.6777 0.6432
VLSV_{\rm LS} (MeV) 0 500 1000 1500 2000 2500 3000 3500 4000
MM 0.57 0.57 0.58 0.59 0.60 0.61 0.63 0.64 0.65
CdineutronC^{\rm dineutron} (01+{}^{+}_{1}) 0.8794 0.8376 0.7603 0.6939 0.6424 0.6020 0.5724 0.5444 0.5195
CdineutronC^{\rm dineutron} (21+{}^{+}_{1}) 0.8524 0.8336 0.7628 0.6540 0.5763 0.5234 0.4906 0.4574 0.4294
CdineutronC^{\rm dineutron} (22+{}^{+}_{2}) 0.8762 0.8016 0.7316 0.7276 0.7129 0.6868 0.6461 0.6192 0.5940

To confirm the development of the dineutron structure by weak VLSV_{\rm LS} parameter, we calculate the component of dineutron cluster, while this component is sensitive to basis states dependent on the random number. Here, we confirmed that the dependence of the basis states does not affect our conclusion. The component of the dineutron cluster for each state is listed in Table 5. Here the dineutron cluster component (Cdineutron(Iiπ)C^{\rm dineutron}(I^{\pi}_{i})) for the state Φ(Iiπ)\Phi(I^{\pi}_{i}) is defined as

Cdineutron(Iiπ)=kΦ(Iiπ)|ψkdineutronψkdineutron|Φ(Iiπ),C^{\rm dineutron}(I^{\pi}_{i})=\sum_{k}\langle\Phi(I^{\pi}_{i})|\psi_{k}^{\rm dineutron}\rangle\langle\psi_{k}^{\rm dineutron}|\Phi(I^{\pi}_{i})\rangle, (8)

where ψkdineutron\psi_{k}^{\rm dineutron} is the kk-th orthonormal state obtained by diagonalizing the Hamiltonian matrix only within the basis states of dineutron clusters introduced in Eq. (7). To clarify on which parameters the dineutron cluster component depends, we show in Table 5 not only the realistic cases but also cases where only the VLSV_{\rm LS} parameter or the MM parameter is changed. The 01+{}^{+}_{1}, 21+{}^{+}_{1}, and 22+{}^{+}_{2} states with the weak VLSV_{\rm LS} value have strong overlaps with the pure dineutron cluster state. With the increase of the VLSV_{\rm LS} value, the dineutron component becomes small. On the other hand, the components of dineutron configurations have a minor dependence on the MM parameter for the 01+{}^{+}_{1} and 21+{}^{+}_{1} states. The dependence of the MM parameter for the 22+{}^{+}_{2} state can be seen, however, the magnitude is smaller than the dependence of the VLSV_{\rm LS} parameter. This supports that the weak VLSV_{\rm LS} parameter gives the development of the dineutron cluster state in the 10Be nucleus.

IV Summary

We summarised the relation between the nuclear structure and reaction with the 10Be nucleus by systematic analysis. The 10Be nucleus is constructed by changing the parameters of the effective NNNN interaction in the microscopic cluster model. The elastic and inelastic cross sections for the proton and 12C targets at E/A=E/A= 59.4 and 200 MeV were calculated with the diagonal and transition densities obtained with various interaction parameters in the MCC calculation. The calculated elastic and inelastic cross sections well reproduce the experimental data.

In the construction of the 10Be nucleus, the strength of the spin-orbit potential (VLSV_{\rm LS}), the nucleon-nucleon exchange effect (MM), and the strength of the proton-proton (neutron-neutron) and proton-neutron interactions (BB and HH) are modified. The VLSV_{\rm LS} parameter has a strong effect on the nuclear structure. The binding energy, nuclear size, expectation value, and transition strength are drastically changed by the VLSV_{\rm LS} value. The elastic and inelastic cross sections are also dependent on the VLSV_{\rm LS} parameter. Especially, the value has an important role in the inelastic cross section of the 22+{}^{+}_{2} state. It is found that the VLSV_{\rm LS} parameter has an important role in the development of the dineutron correlation. The difference of the IV component is slightly seen in the comparison of the proton and 12C targets. The MM parameter also has an effect on the nuclear structure information. The calculated cross sections are also affected by this difference. The multistep reaction effect is also visible at E/A=E/A= 59.4 MeV because the transition strength from the 22+{}^{+}_{2} state to the 21+{}^{+}_{1} state increases with the MM parameter. On the other hand, we see a clear result without the multistep reaction effect at E/A=E/A= 200 MeV. Comparing the results at 200 MeV, the effect of the VLSV_{\rm LS} parameter on the inelastic cross section of the 22+{}^{+}_{2} state is found to be larger than the MM parameter. The BB and HH parameters give a minor effect on the nuclear structure and reaction. It is the VLSV_{\rm LS} parameter that changes the inelastic cross section of the 22+{}^{+}_{2} state most drastically. Since the degree of development of the dineutron correlation is highly dependent on the strength of the spin-orbit interaction, the structure of 10Be changes significantly and the cross section also changes with the VLSV_{\rm LS} parameter.

Next, we adjusted the VLSV_{\rm LS} and MM parameters simultaneously to reproduce the binding energy of the ground state. We prepared different sets of these parameters and compared the obtained structure and the effect on the reaction. As a result, the property of the nuclear structure is found to strongly depend on the VLSV_{\rm LS} parameter rather than the MM parameter. The calculated cross sections are also dependent on the VLSV_{\rm LS} parameter. In addition, we prepared the pure dineutron cluster wave function to investigate the dineutron component in the 10Be nucleus by adjusting the VLSV_{\rm LS} and MM parameters. It is found that the 10Be nucleus with the weak VLSV_{\rm LS} value has a large overlap to the pure dineutron cluster model. Therefore, we again conclude that the development and breaking of the dineutron correlation in 10Be is sensitive to changes in the spin-orbit contribution, thereby resulting in drastic changes in the inelastic scattering for the 22+{}^{+}_{2} state.

Acknowledgements.
This work was supported by Japan Society for the Promotion of Science (JSPS) KAKENHI Grant Numbers JP20K03944, JP21K03543, and JP22K03618. This work was supported by the collaborative research program at Hokkaido University.

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