# Shape of hypernuclei in () deformation plane

###### Abstract

We study the shape of hypernuclei in the full () deformation plane, including both axially symmetric and triaxial quadrupole deformations. To this end, we use the constrained Skyrme Hartree-Fock+BCS method on the three-dimensional Cartesian mesh. The potential energy surface is analyzed for carbon hypernuclei as well as for sd-shell hypernuclei such as Si and Mg. We show that the potential energy surface in the () plane is similar to each other between the hypernuclei and the corresponding core nuclei, although the addition of hyperon makes the energy surface somewhat softer along the direction.

###### pacs:

21.80.+a, 23.20.Lv, 21.30.Fe, 21.60.Jz^{†}

^{†}preprint:

## I Introduction

One of the main interests in hypernuclear physics is to investigate how an addition of particle influences the properties of atomic nuclei. Due to the absence of Pauli’s principle between nucleon and particle, it is believed that a hyperon can be treated as an impurity to probe deep interior of the nuclear medium. With the presence of hyperon as an impurity, some bulk properties of nuclei such as the shape and collective motions may be changed Motoba83 (); Hiyama99 (); Zofka80 (). Indeed, the shrinkage of Li, with respect to Li, has been observed experimentally by measuring the B(E2) value from the state to the state of Li Tanida01 (); Hashimoto06 ().

As the shape of nuclei plays a decisive role in determining their properties such as quadrupole moment and radius, mean-field model calculations have been performed in recent years to investigate the change of nuclear shape due to the addition of a hyperon. Deformed Skyrme-Hartree-Fock(SHF) studies in Ref. Zhou07 () have shown that the deformation parameter of the hypernuclei which they studied is slightly smaller (within the same sign) than that of the corresponding core nuclei, and thus no significant effect of hyperon on nuclear deformation was found. On the other hand, we have performed a relativistic mean field (RMF) study and found that the nuclear deformation of the core nuclei completely disappears for C and Si hypernuclei due to the addition of particle Myaing08 (), although we have obtained similar results to the SHF calculations in Ref. Zhou07 () for many other hypernuclei. In Ref. Schulze10 (), we have compared between the SHF and RMF approaches and have shown that the different results with respect to nuclear deformation between the two approaches is due to the fact that the RMF yields a somewhat stronger polarization effect of hyperon as compared to the SHF approach. We have also shown that the disappearance of the deformation realizes also in the SHF approach if the energy difference between the optimum deformation and the spherical configuration is less than about 1 MeV Schulze10 ().

All of these mean-field calculations have assumed axial symmetric deformation. Although many nuclei are considered to have axially symmetric shape, the triaxial degree of freedom plays an important role in transitional nuclei, nuclei with shape coexistence, and nuclei with gamma soft deformation Hayashi84 (); Redon86 (); Javid01 (); Bonche85 (); Girod09 (); ZPLi10 (); Kurath71 (). In particular, we mention that recent studies with the constrained Hartree-Fock-Bogoliubov plus local quasi-particle random phase approximation (CHFB+LQRPA) method Hinohara10 () as well as the RMF plus generator coordinate method (RMF+GCM) Yao () have revealed an important role of triaxiality in large amplitude collective motion in sd-shell nuclei.

The aim of this paper is to extend the previous mean-field studies on deformation of hypernuclei by taking into account the triaxial degree of freedom, that is, by including both the and deformations in order to investigate the effect of hyperon in the full (,) deformation plane. We particularly study the potential energy surface (PES) in (,) deformation plane with the SHF method for Carbon hypernuclei as well as some sd-shell hypernuclei. Notice that the shape evolution of the C isotopes in the full () plane has been studied by Zhang et al. using the SHF method Ying08 (). We extend the work of Zhang et al. by introducing a hyperon degree of freedom.

The paper is organised as follows. In Sec. II, we briefly summarise the Skyrme-Hartree-Fock method for hypernuclei. In Sec. III, we present the results for the potential energy surface for the C isotopes as well as for sd-shell nuclei, Si and Mg. We also discuss the softness of the energy surface along the deformation. In Sec. IV, we summarize the paper.

## Ii Skyrme Hartree-Fock+BCS method for Hypernuclei

The self-consistent mean field approach provides a useful means to study the ground state properties of hypernuclei. The core polarization effect, that is, the change of properties of a core nucleus due to an addition of particle such as a change of total energy and radius can be automatically taken into account with this method Lanskoy98 (); Harada05 (). The self-consistent non-relativistic mean field calculations with a Skyrme-type -nucleon(N) interaction have been performed by Rayet in Refs. Rayet76 (); Rayet81 (). The relativistic mean field approach has also been applied to hypernuclei in e.g., Refs. Rufa87 (); Mares89 (); Rufa90 (); Vretener98 (). It has been pointed out that the neutron drip line is extended by the addition of hyperon Zhou08 (); Vretener98 ().

In the present paper, we employ the Skyrme-type N interaction and perform mean-field calculations by extending the computer code ev8 Bonche05 () to hypernuclei. The code solves the Hartree-Fock equations by discretizing individual single-particle wave functions on a three-dimensional Cartesian mesh. The pairing correlation is taken into account in the BCS approximation. With this method, both axial and triaxial quadrupole deformations can be automatically described. The code ev8 has been applied to the study of shape transition and deformation of several nuclei Sarriguren08 (); Tajima96 (); Bonche85 (); Ying08 () in the () deformation plane.

The Skyrme-type N interaction is given in complete analogy with the nuclear Skyrme interaction Rayet81 (). The Skyrme part of the total hypernuclear energy thus reads

(1) |

where (r) is the standard nuclear Hamiltonian density based on the Skyrme interaction. See e.g., Refs. Vautherin72 (); BHR03 () for its explicit form. (r) is the hyperon Hamiltonian density given in terms of the lambda and nucleon densities as (with a correction for the coefficient of the term) Rayet81 ()

(2) | |||||

Here, , , and are the particle density, the kinetic energy density, and the spin density of the hyperon. These are expressed using the single-particle wave function for the particle. , , and are the total densities for the nucleons. , and are the Skyrme parameters for the N interaction.

The Hartree-Fock equations for the single-particle wave functions are obtained by taking variation of the energy . The equation for the nucleons reads,

(3) |

where refers to protons or neutrons, while that for the particle reads

(4) |

Here, and are the single-particle energies and the effective mass for the hyperon is given by

(5) |

is the single-particle potential originating from the nucleon-nucleon Skyrme interaction Vautherin72 (); BHR03 (). and are the single-particle potentials originating from the N interaction. These are expressed as Rayet81 ()

(6) | |||||

and

(7) | |||||

The pairing correlations among the nucleons are treated in the BCS approximation. For the pairing interaction, we employ a zero-range density-dependent pairing force Terasaki96 (),

(8) |

where is the spin-exchange operator, fm, and .

In this paper, we mainly use the SGII interaction Vangiai81 () for the NN interaction, while the set No. in Ref. Yamamoto88 () for the N interaction. The latter interaction was constructed by fitting to the binding energy of O, yielding the well depth for a particle, = 29.38 MeV, in infinite nuclear matter. Notice that the spin-orbit strength in the interaction is zero for the set No. 1 Yamamoto88 (). For the pairing interaction, we follow Ref. Ying08 () to use MeVfm for both protons and neutrons for Carbon hypernuclei, while we follow Ref. Terasaki96 () to use MeVfm for calculations of sd-shell hypernuclei. A smooth pairing energy cutoff of 5 MeV around the Fermi level is used Terasaki96 (). We assume that the particle occupies the lowest single-particle state.

Since the primary purpose of this paper is to draw the potential energy surfaces (PES) of hypernuclei as a function of and deformation parameters, the isoscalar quadrupole constraint is imposed on the total energy. We relate the deformation parameter for hypernuclei with the total quadrupole moment using the equation

(9) |

where is the mass number of the core nucleus and fm is the radius of the hypernucleus.

## Iii Results

### iii.1 Carbon Hypernuclei

We now numerically solve the Hartree-Fock equations and discuss the deformation properties of hypernuclei in the () deformation plane. We first investigate the shape of carbon hypernuclei from C to C. To this end, we follow Refs. Sagawa04 (); Ying08 (); Zhou07 (); Schulze10 () and reduce the strength of the spin-orbit interaction by a factor of 0.6 in the Skyrme functional. This prescription was introduced in order to reproduce an oblate ground state of C Sagawa04 ().

Figure 1 shows the potential energy surfaces for C and C so obtained. The triangles in the figure indicate the ground state minimum in the energy surface. The energy curve along the axially symmetric deformation is also shown in Fig. 2 as a function of the quadrupole deformation parameter . Along the axially symmetric configuration, there are deep energy minima in both sides of prolate and oblate configurations of C (that is, the shape coexistence), having a very small energy difference of less than 40 keV between them. The ground state corresponds to the prolate configuration with =0.35. However, the energy surface is almost flat along the triaxial deformation as one can see in Fig. 1 (a) in the () deformation plane. With the addition of a hyperon, the ground state configuration moves from prolate to oblate, although the energy surface is so flat along the degree of freedom (see Fig. 1(b)) that the ground state configuration may not be well defined in the mean field approximation. We have confirmed that this feature remains the same even if we use the Skyrme N interaction set No.2 and No. 5 Yamamoto88 (), instead of No. 1.

Figs. 3 (a) and 4 show the energy surface for C in the deformation plane and that along the line, respectively. For this nucleus, the Skyrme-Hartree-Fock method with the reduced spin-orbit interaction yields a deep oblate minimum. In this case, the addition of a particle shows little effect on the energy surface, although the deformation is slightly smaller than its core nucleus (see Figs. 3(b) and 4). This is similar to the result for Ne discussed in Ref.Myaing08 () with the RMF method.

For the case of C, it has a triaxial minimum at and at an energy of 0.154MeV with respect to the prolate configuration (see Fig. 5 (a)). We find that C has a ground state configuration with similar values of and deformation parameters to those of the core nucleus, C, as indicated in Fig. 5 (b). The triaxial minimum is again shallow with an energy difference of 0.077 MeV between the optimum deformation and the prolate configuration. In Fig. 6, we plot the energy curve as a function of the triaxial deformation parameter for the optimum values of the deformation parameter. With the addition of a particle to C, one sees that the energy curve becomes slightly softer (compare also Figs. 5(a) and 5(b)).

The energy difference between C and C at each deformation, that is, , in the deformation plane is plotted in Fig. 7. It clearly shows that the addition of a particle prefers the spherical configuration even if the core nucleus has a deformed minimum. We have confirmed that this is the case for the other carbon isotopes as well. Notice that the particle slightly prefers the prolate configuration for a fixed value of , causing the slightly softer energy curve towards the prolate configuration shown in Fig. 5. This originates from the fact that the overlap between the deformed nuclear density and a spherical density is maximum at the prolate configuration, as we discuss in the Appendix.

The results of our calculations are summarised in Table I, together with the results for the other carbon isotopes.

### iii.2 sd shell Hypernuclei

#### iii.2.1 Potential Energy Surface

Let us next discuss the deformation energy surfaces of Si,and Mg nuclei in the () deformation plane. For these nuclei, we use the original strength for the spin-orbit interaction. We first show the potential energy surface of Si and Mg in Figs. 8(a) and Fig. 9(a), respectively. The energy surface for Si shows a deep oblate minimum, while that for Mg shows a deep prolate minimum. Notice that N=Z=14 is an oblate magic number. The energy curves for Mg as a function of with , and of with are also plotted in in Figs. 10(a) and 10(b), respectively.

For these nuclei, as the potential minimum is deep, the addition of a particle does not change significantly the shape of the potential energy surface, as shown in Figs. 8(b), 9(b),and 10. As shown in the previous subsection, the energy gain due to the additional particle appears mainly around the spherical configuration. Notice, however, that the particle makes the energy curve slightly softer along the triaxial degree of freedom, .

We next discuss the Mg and Si nuclei. Mg has Z=12 and N=14, that is, the protons favour a prolate configuration while the neutrons favour an oblate configuration. As a competition of these two opposite effects, the structure of Mg may not be trivial Hinohara10 (). Si is the mirror nucleus of Mg, and the deformation properties are expected to be similar to Mg.

Figures 11(a) and Fig. 12(a) show the potential energy surfaces for Si and Mg, respectively. Indeed, the two energy surfaces are similar to each other, and show an oblate minimum with a considerably flat surface along the direction. The energy difference between the oblate and the prolate configurations is 0.12 MeV for Si and 0.39 MeV for Mg. The energy curve for Mg as a function of with , and of with are plotted in in Figs. 13(a) and 13(b), respectively. The energy curves for Si are qualitatively similar, and are not shown.

As in Mg and Si, the addition of a hyperon does not significantly alter the potential energy surface of these nuclei, although it somewhat softens the energy surface along the direction (see Figs. 11(b), 12(b), and 13). We again find that the additional particle favours the spherical configuration.

The calculations presented in this subsection are performed with the SGII set of the Skyrme interaction. We have repeated the same calculations with another Skyrme parameter, SIII, and have found that the results are qualitatively the same as the results obtained with SGII.

#### iii.2.2 vibration

For a long time, the Mg nucleus has been considered to be a candidate of nuclei with a triaxial shape, because of the low-lying second 2state in the rotational spectrum Robinson68 (). That is, the experimental spectrum of Mg has been interpreted as consisting of a =0 ground state rotational band and a =2 rotational band built upon a vibrational state at 4.23 MeV Cohen62 (); Batchelor60 (). The previous mean-field calculations for the ground state of Mg using RMF Koepf88 () and SHF Bonche87 () have shown an axially symmetric prolate ground state. Recently, it has been pointed out that the angular momentum projection is essential in order to reproduce the triaxial ground state of MgYao10 (). The 3-dimensional angular momentum projection plus generator coordinate method (3DAMP+GCM) calculations have shown a good agreement with the experimental data on low-spin states of Mg Yao10 ().

In order to see the effect of hyperon on vibration, we compute the second derivative of the energy curve with respect to around the minimum, . That is, when we approximate the energy curve around the minimum as,

(10) |

the second derivative provides information on the frequency for the vibration if the vibrational moment of inertia is known. By numerically taking the second derivative, we obtain = 0.961 and = 0.988. That is, the addition of a particle makes the vibration softer if the change in the moment of inertia is negligible.

Although the particle softens the energy curve both for Mg and Mg, the mechanism is somewhat different between the two nuclei. For the Mg nucleus, the prolate configuration decreases more energy as compared to the oblate configuration (see Fig. 13 (b)), because the prolate configuration has a larger overlap between the particle and the nucleon densities, as is discussed in the Appendix. As a consequence, the curvature of the energy curve at the oblate minimum becomes smaller with the addition of a particle. In contrast, the effect of the smaller value of is more significant in Mg. That is, the energy curve along the axially symmetric configuration is considerably steep for (see Fig. 10 (a)), and even a small change in induces a significant energy change at the oblate configuration. Therefore, for Mg, the energy decreases more at the oblate side as compared to the prolate side for a fixed value of (see Fig. 10 (b)), leading to the softer gamma-vibration. Notice that the absolute value of is relatviely small for Mg, lying in a “flat” region, and this effect is much less important in the Mg nucleus.

nucleus | (MeV) | ||||||||

C | 0.182 | 0.175 | - | 0.35 | 0 | 0 | - | 0 | 63.222 |

C | 0.140 | 0.087 | 0.010 | 0.223 | 59.619 | 60 | 59.723 | 59.989 | 72.573 |

C | 0.154 | 0.151 | - | 0.301 | 60 | 59.969 | - | 60 | 91.6 |

C | 0.145 | 0.142 | 0.012 | 0.283 | 59.971 | 60 | 59.657 | 59.657 | 102.468 |

C | 0 | 0 | - | 0 | - | - | - | - | 112.496 |

C | 0 | 0 | 0 | 0 | - | - | - | - | 124.962 |

C | 0.084 | 0.224 | - | 0.296 | 0 | 0 | - | 0 | 118.354 |

C | 0.063 | 0.167 | 0.005 | 0.224 | 0 | 0 | 0 | 0 | 136.242 |

C | 0.090 | 0.254 | - | 0.342 | 26.078 | 15.290 | - | 17.996 | 124.478 |

C | 0.085 | 0.243 | 0.007 | 0.326 | 25.940 | 15.368 | 19.871 | 18.045 | 138.102 |

C | 0.083 | 0.234 | - | 0.315 | 47.96 | 11.62 | - | 59.58 | 131.156 |

C | 0.083 | 0.237 | 0.007 | 0.318 | 60 | 59.840 | 60 | 60 | 145.325 |

C | 0.064 | 0.185 | - | 0.249 | 60 | 59.756 | - | 60 | 132.779 |

C | 0.061 | 0.172 | 0.005 | 0.232 | 60 | 59.770 | 60 | 60 | 147.551 |

Si | 0.1 | 0.128 | - | 0.224 | 60 | 59.988 | 60 | - | 216.938 |

Si | 0.129 | 0.1 | 0.004 | 0.224 | 60 | 59.900 | 60 | 60 | 233.373 |

Si | 0.144 | 0.140 | - | 0.278 | 59.979 | 60 | - | 60 | 245.900 |

Si | 0.132 | 0.128 | 0.004 | 0.255 | 59.980 | 60 | 60 | 60 | 262.773 |

Mg | 0.2 | 0.195 | - | 0.387 | 0 | 0 | - | 0 | 206.924 |

Mg | 0.190 | 0.185 | 0.007 | 0.368 | 0 | 0 | 0 | 0 | 222.714 |

Mg | 0.104 | 0.126 | - | 0.226 | 59.951 | 60 | - | 60 | 227.144 |

Mg | 0.093 | 0.112 | 0.003 | 0.201 | 59.954 | 60 | 60 | 60 | 243.609 |

## Iv Summary

We have investigated the shape of hypernuclei in the () deformation plane with the Skyrme-Hartree-Fock + BCS approach. In contrast to the previous mean-field studies, we have taken into account the triaxial deformation using a 3-D Cartesian mesh method. We have studied the potential energy surface for the Carbon hypernuclei from C to C as well as sd-shell hypernuclei Si, Si, Mg and Mg. The potential energy surface for C, Mg, and Si is characterized by a flat surface along the degree of freedom connecting the prolate and the oblate configurations. We have found that the addition of a particle makes the energy surface slightly softer along the triaxial degree of freedom, although the gross feature of the energy surface remains similar to the energy surface for the corresponding core nuclei.

In Refs. Myaing08 (); Schulze10 (), we have argued that the influence of the addition of a particle is stronger in the relativistic mean-field approach as compared to the non-relativistic Skyrme-Hartree-Fock approach employed in this paper. This implies that the softening of the energy curve for the -vibration may be larger than that estimated in this paper, if we employ the RMF approach instead of the SHF approach. It would be an interesting future subject to carry out three-dimensional calculations for hypernuclei with RMF in order to confirm whether it is the case.

There would be many ways to improve our calculations presented in this paper. Firstly, as the angular momentum projection is shown to be essential to yield the triaxial shape of Mg Yao10 (), it may be important to carry out the angular momentum projection on top of the mean-field energy surface in order to discuss the effect of particle on the shape of hypernuclei. Secondly, for nuclei with a flat energy surface along the direction, the generator coordinate method may be required. In particular, it will provide a more quantitative estimate for the energy change of the vibrational state due to the addition of particle. In any case, the mean-field calculations presented in this paper provide a good starting point for these calculations.

It will be an interesting subject to experimentally measure the deformation properties and collective motions of hypernuclei. A discussion has been started for a future experiment of -ray spectroscopy of sd-shell hypernuclei at the new generation experimental facilities, e.g., the J-PARC facility Koike08 (); Tamura09 (). The change of deformation will be well investigated if excitation energies in a rotational band and the B(E2) values can be measured experimentally.

###### Acknowledgements.

We thank H. Tamura, Y. Zhang, N. Hinohara and A. Ono for useful discussions. This work was supported by the Japanese Ministry of Education, Culture, Sports, Science and Technology by Grant-in-Aid for Scientific Research under the program number 22540262.## Appendix A Overlap between -particle and nucleon densities

In this Appendix, we discuss the overlap between particle and nucleon density distributions using simple parametrizations for the density distributions. Since we consider that a particle occupies the lowest single-particle state, we assume that the particle density is almost spherical and is given by,

(11) |

On the other hand, for the nucleon density, we assume that it is given by a deformed Woods-Saxon form, that is,

(12) |

where

(13) | |||||

Here, the radius is determined for each and in order to satifsy the volume conservation condition, that is,

(14) |

is independent of and .

Figure 14 shows the overlap between and , that is,

(15) |

as a function of the triaxiality for a fixed value of . To this end, we use fm, and =0.55 fm. The value of is fixed so that the volume integral of is 24. We use =1.565 fm, which corresponds to the harmonic oscillator with a frequency of MeV. As one can see, the overlap is the largest for the prolate configuration, although the variation is small with respect to .

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