Mirror Nuclei of 17O and 17F in Relativistic and Non- Relativistic Shell Model

We have investigated energy levels mirror nuclei of the 17O and 17F in relativistic and non-relativistic shell model. The nuclei 17O and 17F can be modeled as a doubly-magic 17O=n+(N=Z=8) and 17F=p+(N=Z=8), with one additional nucleon (valence) in the ld5/2 level. Then we have selected the quadratic Hellmann potential for interaction between core and single nucleon. Using Parametric Nikiforov-Uvarov method, we have calculated the energy levels and wave function in Dirac and Schrodinger equations for relativistic and non-relativistic, respectively. Finally, we have computed the binding and excited energy levels for mirror nuclei of 17O and 17F and compare with other works. Our results were in agreement with experimental values and hence this model could be applied for similar nuclei.


Introduction
Special interest resides in the study of masses and sizes for a given element along isotopic chains. Experimentally, their determination is increasingly difficult as one approaches the neutron drip-line; as of today, the heaviest element with available data on all existing bound isotopes is oxygen (Z=8) [1]. Theoretically, the link between nuclear properties and internucleon forces can be explored for different values of N/Z and binding regimes, thus critically testing both our knowledge of nuclear forces and many-body theories [2]. The way shell closures and single-particle energies evolve as functions of the number of nucleons is presently one of the greatest challenges to our understanding of the basic features of nuclei. The properties of single particle energies and states with a strong quasi-particle content along an isotopic chain are moreover expected to be strongly influenced by the nuclear spin-orbit force [3]. The best evidence for single-particle behavior is found near magic (also called closed-shell) nuclei, where the number of protons or neutrons in a nucleus fills the last shell before a major or minor shell gap. For example, the nuclei 17 O and 17 F can be modeled as a doubly-magic 17 O=n+(N=Z=8) and 17 F=p+(N=Z=8), with one additional (valence) nucleon in the ld5/2 level. The ground-state spin and parity of 17 O and 17 F are J π =5/2 + , which corresponds to the spin and parity of the level where the valence nucleon resides [4]. The study of relativistic effects is always useful in some quantum mechanical systems. Therefore, The Dirac equation, which describes the motion of a spin-1/2 particle, has been used in solving many problems of nuclear and high-energy physics. The spin and the pseudo-spin symmetries of the Dirac Hamiltonian were discovered many years ago, however, these symmetries have recently been recognized empirically in nuclear and hadronic spectroscopes [5-6-7]. In this work we use relativistic and non-relativistic shell model for calculation of the energy levels for 17 O and 17 F isotope. Since these isotopes have one nucleon out of the core, Dirac and Schrodinger equations are utilized to investigation them in relativistic and non-relativistic shell model, respectively. These isotopes could be considered as a single particle. We apply the modified Hellmann potential [8,9] between the core and a single particle because these 2 potentials are important nuclear potentials for a description of the interaction between single nucleon and whole nuclei. Now that the N-N potential is selected, the next step is a solution of the Dirac and Schrodinger equation for the nuclei under investigation. We use the Parametric Nikiforov-Uvarov (PNU) method [29,30] to solve them. The scheme of paper is as follows: in Section 2 and 3, energy spectrum in relativistic and nonrelativistic shell model is presented respectively. Discussion and results are given in section 4.

Energy Spectrum in Relativistic Shell Model
In the relativistic description, the Dirac equation of a single-nucleon with the mass moving in an attractive scalar potential S(r) and a repulsive vector potential V (r) can be written as [10]: Where E is the relativistic energy, M is the mass of a single particle and α and β are the 4 ×4 Dirac matrices. The wave-functions can be classified according to their angular momentum j and spin-orbit quantum number k as follows: r r r l n ,k jm n ,k l n ,k jm The quadratic Hellmann potential is defined as [12,13]: Where the parameters a and b are real parameters, these are strength parameters, and the parameter α is related to the range of the potential. Using the transformation n,k n,k F (r) rU (r)  Eq. (3) brings into the form: Equation (5) is exactly solvable only for the case of k = 0,-1. In order to obtain the analytical solutions of Eq. (5), we employ the improved Pekeris approximation [14] that is valid for α≤1. The main characteristic of these solutions lies in the substitution of the centrifugal term by an approximation, so that one can obtain an equation, normally hypergeometric, which is solvable [15,11].
3 Also this approximation in reverse order could be used. We can write the Eq. (5) by using improved Pekeris approximation as summarized below: 2 n,k n,k 2 1 0 n,k 2 Where the parameters χ2, χ1 and χ0 are considered as follows: Applying PNU method, we obtain the energy equation (with referring to reference [16,17]) as: With substituting Eq. (8) (13) Where N is the normalization constant.

Energy Spectrum in Non-Relativistic Shell Model
The radial Schrodinger equation in spherical coordinates is given as [20,21] (14) By substituting quadratic Hellmann potential in the equation (14) Since the Schrodinger equation with above potential has no analytical solution for Ɩ≠0 states, an approximation has to be made. Using improved Pekeris approximation [15,11] that is presented in the previous section the Eq. (15) is as following: 2 n,l n,l 2 Where the parameters χʹ2, χʹ1 and χʹ0 are considered as follows: Applying PNU method, we obtain the energy equation (with referring to the reference [16,17]) as below: And radial wave function for Schrodinger equation can be calculated with referring to PNU method in reference [16,17] Where Nʹ is the normalization constant.

Result and Discussion
We consider mirror nuclei 17 O and 17 F isotopes with a single nucleon on top of the 16 O and 16 F isotopes core. Since these isotopes have one nucleon out of the core, these isotopes could be considered as single particle model in relativistic and non-relativistic shell model. Relativistic mean field (RMF) theory, as a covariant density functional theory, has been successfully applied to the study of nuclear structure properties [22]. In the relativistic mean field theory, repulsive and attractive effects at the same time have been combined, via vector and scalar potentials, also it involves the antiparticle solutions and spin-orbit interaction [23]. So we could use of Dirac equation for investigation them. 5 The ground state and first excited energies of mirror nuclei 17 O and 17 F isotopes are obtained in relativistic and non-relativistic shell model by using Eq. (10) and Eq. (19), respectively. These results for relativistic and non-relativistic shell model are compared with the experimental data and others work in table 1.