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Structure of C13{}^{13}\mathrm{C} in the Cluster Shell Model

A H Santana Valdés1    R Bijker2 Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Apartado Postal 70-543, 04510 Cd. de México, México 1adrian.santana@correo.nucleares.unam.mx, 2bijker@nucleares.unam.mx
Abstract

We study the structure of 13C in the framework of the Cluster Shell Model. A comparison of the available experimental data with our model is made. Some predictions for level ordering and form factors are presented.

1 Introduction

Recent measurements of rotational excitations in 12C have renewed interest in the cluster structure of light nuclei, particularly α\alpha conjugate nuclei as clusters of kk α\alpha-particles. The interest in these structures dates as back as 1937, with the works of [1, 2, 3, 4]. The intricate patterns in which protons and neutrons are arranged give rise to a multitude of special properties, many of them of great implications, from nuclear physics to astrophysics, where the best example of this is the Hoyle state. Clustering in nuclei is complex, and the underlying physics is not yet fully understood, being a major challenge for researchers. Over the years 12C has been the object of study of several models, including Antisymmetric Molecular Dynamics[5], Fermion Molecular Dynamics[6], BEC-like cluster model[7], lattice EFT[8] and the Algebraic Cluster Model[9], all of them implementing or obtaining the cluster structure as a result. A more comprehensive review of many different models and their assumptions about clustering in nuclei can be found in [10, 11, 12].

Yet for its neighbors, a query arises when one questions to what extent the cluster structure persists with adding extra nucleons. This proceeding addresses part of this question, showing precursory results of longitudinal form factors for 12C and 13C and transverse form factors for 13C in the framework of the Cluster Shell Model (CSM), where 13C is seen as a 12C core plus an extra neutron. 13C can then be considered as a system with 𝒟3h{\cal D}^{\prime}_{3h} symmetry, consisting of three α\alpha-particles in a triangular configuration plus an additional neutron moving in the deformed field generated by the cluster. The matrix elements of the form factor operators are then calculated, where a dominance of the core cluster structure is found for longitudinal form factors, exhibiting a very similar qq dependence between 12C and 13C, corroborated by experimental data. Finally, we show some preliminary results for transverse form factors.

2 Cluster Shell Model

The Cluster Shell Model was introduced in [13, 14, 15] to describe nuclei composed of kk α\alpha-particles plus additional nucleons, denoted as kα+xk\alpha+x nuclei. It is similar in spirit to the Nilsson model [16]; the main difference lies in that the odd nucleon moves in the deformed field generated by the cluster core.

2.1 Cluster Potential

To obtain the single-particle energy levels, we define

H=T+V(r)+Vso(r)+12(1+τ3)VC(r),\displaystyle H\;=\;T+V(\vec{r})+V_{\rm so}(\vec{r})+\frac{1}{2}(1+\tau_{3})V_{\rm C}(\vec{r})~{}, (1)

i.e. the sum of the kinetic energy, a central potential obtained by convoluting the density

ρ(r)=\displaystyle\rho(\vec{r})= (απ)3/2i=1kexp[α(rri)2]\displaystyle\left(\frac{\alpha}{\pi}\right)^{3/2}\sum_{i=1}^{k}\exp\left[-\alpha\left(\vec{r}-\vec{r}_{i}\right)^{2}\right]
=\displaystyle= (απ)3/2eα(r2+β2) 4πλμiλ(2αβr)Yλμ(θ,ϕ)i=1kYλμ(θi,ϕi),\displaystyle\left(\frac{\alpha}{\pi}\right)^{3/2}\mbox{e}^{-\alpha(r^{2}+\beta^{2})}\,4\pi\,\sum_{\lambda\mu}i_{\lambda}(2\alpha\beta r)\,Y_{\lambda\mu}(\theta,\phi)\sum_{i=1}^{k}Y_{\lambda\mu}^{\ast}(\theta_{i},\phi_{i})~{}, (2)

with the interaction between the α\alpha-particle and the nucleon, a spin-orbit interaction, and a Coulomb potential for an odd proton. In equation 1, ri=(ri,θi,ϕi)\vec{r}_{i}=(r_{i},\theta_{i},\phi_{i}) represent the coordinates of the α\alpha-particles with respect to the center-of-mass of the cluster structure. The case of 13C belongs to k=3k=3 with an equilateral triangular configuration, whose coordinates are given by (β,π2,0)(\beta,\frac{\pi}{2},0), (β,π2,2π3)(\beta,\frac{\pi}{2},\frac{2\pi}{3}) and (β,π2,4π3)(\beta,\frac{\pi}{2},\frac{4\pi}{3}). The deformation parameter (from spherical symmetry) is β\beta, which is the distance of each of the alpha particles to the center of mass of the cluster structure. The resulting potentials are

V(r)\displaystyle V\left(\vec{r}\right) =V0λμfλ(r)Yλμ(θ,ϕ)i=1kYλμ(θi,ϕi),\displaystyle=-V_{0}\sum_{\lambda\mu}f_{\lambda}\left(r\right)Y_{\lambda\mu}\left(\theta,\phi\right)\sum_{i=1}^{k}Y_{\lambda\mu}^{*}\left(\theta_{i},\phi_{i}\right), (3)
Vso(r)\displaystyle V_{so}\left(\vec{r}\right) =V0,so12[1rV(r)r(sl)+(sl)1rV(r)r],\displaystyle=V_{0,so}\frac{1}{2}\left[\frac{1}{r}\frac{\partial V\left(\vec{r}\right)}{\partial r}\left(\vec{s}\cdot\vec{l}\right)+\left(\vec{s}\cdot\vec{l}\right)\frac{1}{r}\frac{\partial V\left(\vec{r}\right)}{\partial r}\right], (4)
fλ(r)\displaystyle f_{\lambda}\left(r\right) =eα(r2+β2)4πiλ(2αβr).\displaystyle=e^{-\alpha\left(r^{2}+\beta^{2}\right)}4\pi i_{\lambda}\left(2\alpha\beta r\right). (5)

2.2 𝒟3h{\cal D}^{\prime}_{3h} symmetry

Refer to caption
Figure 1: Schematic view of all principal axis and rotation operators for 𝒟3h{\cal D}^{\prime}_{3h} symmetry.

To construct a complete wave function we need to understand in more detail the 𝒟3h{\cal D}^{\prime}_{3h} symmetry. The objective is to construct a symmetry-adapted basis for 𝒟3h{\cal D}^{\prime}_{3h} symmetry instead of a spherical basis[17, 18]. In the case of triangular symmetry the eigenstates of equation 1 can be classified according to the doubly degenerate spinor representations of the double point group 𝒟3h{\cal D}^{\prime}_{3h} [19, 20]: Ω=E1/2\Omega=E_{1/2}, E5/2E_{5/2} and E3/2E_{3/2}, or in the notation of Ref. [17] Ω=E1/2(+)\Omega=E_{1/2}^{(+)}, E1/2()E_{1/2}^{(-)} and E3/2E_{3/2}, respectively. From similar work in molecular physics, to differentiate between the degenerate states, one finds all rotations of the structure of study; the case in question is shown in figure 1. Then improper rotations are used (in this case the S6S_{6}) to identify the intrinsic states of the doubly degenerate spinor representations. The resulting labels are γ=±5/2\gamma=\pm 5/2 for Ω=E5/2\Omega=E_{5/2}, γ=±1/2\gamma=\pm 1/2 for E1/2E_{1/2} and γ=±3/2\gamma=\pm 3/2 for E3/2E_{3/2}. The Hamiltonian of the CSM is solved in the body-fixed system, using the harmonic oscillator basis |nljm|nljm\rangle.

ϕΩγ=\displaystyle\phi_{\Omega\gamma}= nljmCnljmΩγ|nljm\displaystyle\sum_{nljm}C^{\Omega\gamma}_{nljm}\left|nljm\right> (6)

The rotational states can be labeled by the angular momentum II, parity PP, and its projection KK on the symmetry axis, |IPK|I^{P}K\rangle. Both II and KK are half integers. Then the allowed values of KPK^{P} for each one of the spinor representations, along with their γ\gamma labels are given by [17, 18]

Ω=E1/2,γ=±12:KP=±12+,52,±72,Ω=E5/2,γ=±52:KP=12,±52+,72+,Ω=E3/2,γ=±32:KP=±32+,32,92+,\displaystyle\begin{array}[]{lcl}\Omega=E_{1/2},\;\gamma=\pm\frac{1}{2}&:&K^{P}=\pm\frac{1}{2}^{+},\mp\frac{5}{2}^{-},\pm\frac{7}{2}^{-},\ldots\\ \Omega=E_{5/2},\;\gamma=\pm\frac{5}{2}&:&K^{P}=\mp\frac{1}{2}^{-},\pm\frac{5}{2}^{+},\mp\frac{7}{2}^{+},\ldots\\ \Omega=E_{3/2},\;\gamma=\pm\frac{3}{2}&:&K^{P}=\pm\frac{3}{2}^{+},\mp\frac{3}{2}^{-},\mp\frac{9}{2}^{+},\ldots\end{array} (10)

with I=|K|I=|K|, |K|+1|K|+1, \ldots. A schematic view can be seen in figure 2. The complete wave function is defined then by [18]

|Ωγ;IPMK=2I+116π2ψv(1+𝒮i1𝒮e)ϕΩγDMKI(ω)\displaystyle\left|\Omega\gamma;I^{P}MK\right>=\sqrt{\frac{2I+1}{16\pi^{2}}}\psi_{v}\left(1+{\cal S}_{i}^{-1}{\cal S}_{e}\right)\phi_{\Omega\gamma}D_{MK}^{I}(\omega) (11)

where ψv\psi_{v} is the vibrational wave function, ϕΩγ\phi_{\Omega\gamma} the intrinsic wave function and DMKI(ω)D_{MK}^{I}(\omega) the rotational wave function. The wave function is invariant under the transformation 𝒮i1𝒮e{\cal S}_{i}^{-1}{\cal S}_{e} where the operator 𝒮{\cal S} is the product of a rotation about π\pi followed by a parity transformation [18]. The operator 𝒮i1{\cal S}_{i}^{-1} acts on the intrinsic wave function and 𝒮e{\cal S}_{e} on the rotational wave function.

2.3 Splitting of single-particle levels

Previous work on the splitting of single-particle levels is shown in [13, 21]. The splitting of the single-particle energy levels is seen in figure 3. Two simple observations that are illustrated in the figure are that at a value of β=0\beta=0 the spherical symmetry is recovered, and at max value, we have 3-fold degeneracy of the spherical symmetry. In other words, at the max value we obtain the view of a particle in a field formed by three separate (not bound in a nucleus) alpha particles, which is unlike the Nilsson model where in the case of max deformation one obtains the splitting for an ”infinite cigar”. From the elastic form factors, one obtains the value for β\beta and then comes back to figures 3 and 2 and obtains the base rotational band proposed for 13C. Foreshadowing the subsequent section, the value obtained for β\beta is 1.71 fm, which in turn gives the ground state rotational band as Ω=E5/2\Omega=E_{5/2}, and the ground state with IP=12I^{P}=\frac{1}{2}^{-}.

Refer to caption
Figure 2: Schematic view of rotational structure with 𝒟3h{\cal D}^{\prime}_{3h}, proposed for 13C. Imagine obtained from [22].
Refer to caption
Figure 3: Single-particle energy level splitting from solving equation 1. The values used for equations 3 and 4 are V0V_{0}=32 MeV, α\alpha=0.0511 fm-2 and V0,soV_{0,so}=17 MeV fm-2.

3 Form Factors and comparison to experimental data

Using equation 11 we can now calculate the form factors for 13C and compare them with available experimental data. We use the standard form factors operators, of which a full explanation is found in [23].

3.1 Longitudinal form factors

The charge distribution is taken to be section 2.1, plus a point-like distribution for the extra nucleon

ρ(r)=(Ze)c3(απ)3/2i=13exp[α(rri)2]+e~δ(rrsp),\displaystyle\rho(\vec{r})=\frac{(Ze)_{\rm c}}{3}\left(\frac{\alpha}{\pi}\right)^{3/2}\sum_{i=1}^{3}\exp\left[-\alpha\left(\vec{r}-\vec{r}_{i}\right)^{2}\right]+\tilde{e}\delta(\vec{r}-\vec{r}_{\rm sp}), (12)

(Ze)c(Ze)_{\rm c} is the electric charge of the 3α3\alpha core nucleus, and e~\tilde{e} the effective charge of the extra nucleon, which for the case of 13C is taken to be zero. Making a Fourier transformation of equation 12, and then summing over final and averaged over initial states, we obtain the multipoles of the longitudinal (Coulomb) form factor;

FCλ(q;Ωγ,IKΩγ,IK)\displaystyle F_{C\lambda}\left(q;\Omega^{\prime}\gamma^{\prime},I^{\prime}K^{\prime}\rightarrow\Omega\gamma,IK\right) =4π(Ze)oddI,K,λ,KK|I,KδΩΩδγγGvvc(q),\displaystyle=\frac{\sqrt{4\pi}}{\left(Ze\right)_{\mathrm{odd}}}\langle I^{\prime},K^{\prime},\lambda,K-K^{\prime}\left|I,K\right\rangle\delta_{\Omega\Omega^{\prime}}\delta_{\gamma\gamma^{\prime}}G_{vv^{\prime}}^{\mathrm{c}}\left(q\right), (13)

where (Ze)odd(Ze)_{\rm odd} denotes the electric charge of the odd nucleus. For the vibrationally elastic case with v=v=0v=v^{\prime}=0 the collective part is given by

G00c(q;λ,KK)\displaystyle G^{\rm c}_{00}(q;\lambda,K-K^{\prime}) =(Ze)cjλ(qβ)eq2/4αYλ,KK(π2,0)δKK,3κ\displaystyle=(Ze)_{\rm c}\,j_{\lambda}(q\beta)\,\mbox{e}^{-q^{2}/4\alpha}\,Y_{\lambda,K-K^{\prime}}(\frac{\pi}{2},0)\,\delta_{K-K^{\prime},3\kappa} (14)

A final remark arises when calculating form factors with diagonal intrinsic states. In that case, branching ratios are found between different form factors with the same multipole.

|FCλ(q;Ωγ,IKΩγ,I1K1)|2|FCλ(q;Ωγ,IKΩγ,I2K2)|2=I,K,λ,K1K|I1,K12I,K,λ,K2K|I2,K22.\displaystyle\frac{\left|F_{C\lambda}(q;\Omega\gamma,I^{\prime}K^{\prime}\rightarrow\Omega\gamma,I_{1}K_{1})\right|^{2}}{\left|F_{C\lambda}(q;\Omega\gamma,I^{\prime}K^{\prime}\rightarrow\Omega\gamma,I_{2}K_{2})\right|^{2}}=\frac{\left<I^{\prime},K^{\prime},\lambda,K_{1}-K^{\prime}|I_{1},K_{1}\right>^{2}}{\left<I^{\prime},K^{\prime},\lambda,K_{2}-K^{\prime}|I_{2},K_{2}\right>^{2}}. (15)

Finally one sees that the single particle element for Coulomb form factors doesn’t give any contribution to the total value, thus we expect that for both 12C and 13C to have the same q dependence. The results are illustrated in figures 4 and 5.

Refer to caption
Figure 4: Comparison of elastic form factor between 12C (left) and 13C(right). Both graphs include available experimental data for both 12C[24] and 13C[25].
Refer to caption
Figure 5: Comparison of C2 form factor between 12C (left) and 13C(right). Both graphs include available experimental data for both 12C[26, 27] and 13C[28].

3.2 Transverse form factors

Just as previously done for the Coulomb form factors, the transverse form factors are obtained from a Fourier transform of the current J\vec{J} and magnetization operator μ\vec{\mu}, with a little more algebra involved to obtain the final expressions. The main assumption we do from the CSM is that the only contributor to both is the extra nucleon

J\displaystyle\vec{J} =0\displaystyle=0 (16)
μ\displaystyle\vec{\mu} =δ(rix)μiσ(i)2Mi,\displaystyle=\delta\left(\vec{r_{i}}-\vec{x}\right)\mu_{i}\frac{\vec{\sigma}\left(i\right)}{2M_{i}}, (17)

where μi\mu_{i} is the magnetic moment (in nuclear magnetons) of the nucleon involved, in this case for the free neutron is μn=1.91\mu_{n}=-1.91 and MiM_{i} is the mass. The multipoles for the transverse form factor are then given by

FEλ/Mλ(q;Ωγ,IK\displaystyle F_{E\lambda/M\lambda}(q;\Omega^{\prime}\gamma^{\prime},I^{\prime}K^{\prime} =I,K,λ,KK|I,KδvvGΩγ,Ωγsp(q)\displaystyle=\left<I^{\prime},K^{\prime},\lambda,K-K^{\prime}|I,K\right>\delta_{vv^{\prime}}G_{\Omega\gamma,\Omega^{\prime}\gamma^{\prime}}^{{\rm sp}}(q)
+P(1)I+KI,K,λ,KK|I,KδvvHΩγ,Ωγsp(q),\displaystyle+P(-1)^{I+K}\left<I^{\prime},K^{\prime},\lambda,-K-K^{\prime}|I,-K\right>\delta_{vv^{\prime}}H_{\Omega\gamma,\Omega^{\prime}\gamma^{\prime}}^{{\rm sp}}(q), (18)

where GΩγ,Ωγsp(q)G_{\Omega\gamma,\Omega^{\prime}\gamma^{\prime}}^{{\rm sp}}(q) and HΩγ,Ωγsp(q)H_{\Omega\gamma,\Omega^{\prime}\gamma^{\prime}}^{{\rm sp}}(q) will have the form

GΩγ,Ωγsp(q)\displaystyle G^{\rm sp}_{\Omega\gamma,\Omega^{\prime}\gamma^{\prime}}(q) =nljmnljmCnljmΩγCnljmΩγnljm|T^λμζ(q,r)|nljm\displaystyle=\sum_{nljm}\sum_{n^{\prime}l^{\prime}j^{\prime}m^{\prime}}C^{\Omega\gamma}_{nljm}C^{\Omega^{\prime}\gamma^{\prime}}_{n^{\prime}l^{\prime}j^{\prime}m^{\prime}}\left<nljm\left|\hat{T}_{\lambda\mu}^{\zeta}\left(q,\vec{r}\,\right)\right|n^{\prime}l^{\prime}j^{\prime}m^{\prime}\right> (19a)
HΩγ,Ωγsp(q)\displaystyle H^{\rm sp}_{\Omega\gamma,\Omega^{\prime}\gamma^{\prime}}(q) =nljmnljmCnljmΩγCnljmΩγ(1)n+j+mnlj,m|T^λμζ(q,r)|nljm\displaystyle=\sum_{nljm}\sum_{n^{\prime}l^{\prime}j^{\prime}m^{\prime}}C^{\Omega\gamma}_{nljm}C^{\Omega^{\prime}\gamma^{\prime}}_{n^{\prime}l^{\prime}j^{\prime}m^{\prime}}(-1)^{n+j+m}\left<nlj,-m\left|\hat{T}_{\lambda\mu}^{\zeta}\left(q,\vec{r}\,\right)\right|n^{\prime}l^{\prime}j^{\prime}m^{\prime}\right> (19b)

and T^λμζ(q,r)\hat{T}_{\lambda\mu}^{\zeta}\left(q,\vec{r}\,\right) are the electric/magnectic transverse form factor operators

T^λμE(q,r)\displaystyle\hat{T}_{\lambda\mu}^{E}\left(q,\vec{r}\,\right) =qμi2MNMλ,λμ(ri)σ(i)\displaystyle=q\frac{\mu_{i}}{2M_{N}}\vec{M}_{\lambda,\lambda}^{\mu}(\vec{r_{i}})\cdot\vec{\sigma}(i)
T^λμM(q,r)\displaystyle\hat{T}_{\lambda\mu}^{M}\left(q,\vec{r}\,\right) =iqμi2MN(λ2λ+1Mλ,λ+1μ(ri)+λ+12λ+1Mλ,λ1μ(ri))σ(i)\displaystyle=iq\frac{\mu_{i}}{2M_{N}}\left(-\sqrt{\frac{\lambda}{2\lambda+1}}\vec{M}_{\lambda,\lambda+1}^{\mu}(\vec{r_{i}})+\sqrt{\frac{\lambda+1}{2\lambda+1}}\vec{M}_{\lambda,\lambda-1}^{\mu}(\vec{r_{i}})\right)\cdot\vec{\sigma}(i)
Mλ1,λ2μ(r)\displaystyle\vec{M}_{\lambda_{1},\lambda_{2}}^{\mu}\left(\vec{r}\,\right) =jλ2(qr)Yλ1λ21μ(θ,ϕ).\displaystyle=j_{\lambda_{2}}(qr)\vec{Y}_{\lambda_{1}\lambda_{2}1}^{\mu}(\theta,\phi). (20)

The results are showed in figure 6.

Refer to caption
Figure 6: Comparison of M1 elastic form factor between experimental data [28] and CSM calculation.

4 Summary and Conclusions

From calculations, it is seen that for longitudinal form factors in the base rotational band of 13C, the cluster core structure is dominant. In those cases, we expected that Coulomb form factors for both 12C and 13C have the same qq dependence. From figures 4 and 5 we see that the experimental data seems to support that idea, differing only slightly in some aspects. Also, it shows for 13C that longitudinal form factors follow a branching ratio rule like the one in equation 15. This is of great importance since it indicates that some properties of the cluster structure in 12C are still present in 13C.

Unfortunately, such a positive outcome was not the case for the transverse form factors. From figure 6 we are not able to reproduce available experimental data. Only global functional properties are reproduced of [28]. It is most likely that our assumptions in equations 16 and 17 are incorrect and must then include a contribution of the cluster core. A possible solution may be found in [29], but it would have to be adapted for the CSM.

To reiterate, the CSM as is now is a good approximation to calculate longitudinal form factors for 13C, reproducing accurately the available experimental data. Meanwhile, in the case of transverse form factors, the model is still lacking, due most likely to not considering the contribution of the cluster structure to the transverse form factors.

\ack

This work was supported in part by research grants IN101320, IG101423 from PAPIIT-DGAPA and 784896 from CONACYT.

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