Research Article  Open Access
Spin and Pseudospin Symmetries with Trigonometric PöschlTeller Potential including Tensor Coupling
Abstract
We study approximate analytical solutions of the Dirac equation with the trigonometric PöschlTeller (tPT) potential and a Coulomblike tensor potential for arbitrary spinorbit quantum number κ under the presence of exact spin and pseudospin (spin) symmetries. The bound state energy eigenvalues and the corresponding twocomponent wave functions of the Dirac particle are obtained using the parametric generalization of the NikiforovUvarov (NU) method. We show that tensor interaction removes degeneracies between spin and pseudospin doublets. The case of nonrelativistic limit is studied too.
1. Introduction
The Dirac equation, which describes the motion of a spin1/2 particle, has been used in solving many problems of nuclear and highenergy physics. The spin and the spin symmetries of the Dirac Hamiltonian had been discovered many years ago; however, these symmetries have recently been recognized empirically in nuclear and hadronic spectroscopes [1]. Within the framework of Dirac equation, spin symmetry used to feature the deformed nuclei and the super deformation to establish an effective shellmodel [2–4], whereas spin symmetry is relevant for mesons [5]. The spin symmetry occurs when the scalar potential is nearly equal to the vector potential or equivalently , and spin symmetry occurs when [6, 7]. The spin symmetry refers to a quasidegeneracy of single nucleon doublets with nonrelativistic quantum number and , where , , and are single nucleon radial, orbital, and total angular quantum numbers, respectively [8, 9]. The total angular momentum is given by , where pseudoangular momentum and is spin angular momentum [10, 11]. Liang et al. [12] investigated the symmetries of the Dirac Hamiltonian and their breaking in realistic nuclei in the framework of perturbation theory. Guo [13] used the similarity renormalization group to transform the spherical Dirac operator into a diagonal form, and then the upper (lower) diagonal element became an operator describing Dirac (anti)particle, which holds the form of the Schrödingerlike operator with the singularity disappearing in every component. Chen and Guo [14] investigated the evolution toward the nonrelativistic limit from the solutions of the Dirac equation by a continuous transformation of the Compton wavelength. Lu et al. [15] recently showed that the spin symmetry in single particle resonant states in nuclei is conserved when the attractive scalar and repulsive vector potentials have the same magnitude but opposite sign.
Tensor potentials were introduced into the Dirac equation with the substitution , and a spinorbit coupling is added to the Dirac Hamiltonian [16, 17]. Lisboa et al. [18] have studied a generalized relativistic harmonic oscillator for spin particles by considering a Dirac Hamiltonian that contains quadratic vector and scalar potentials together with a linear tensor potential, under the conditions of pseudospin and spin symmetry. Alberto et al. [19] studied the contribution of the isoscalar tensor coupling to the realization of pseudospin symmetry in nuclei. Akcay showed that the Dirac equation with scalar and vector quadratic potentials and a Coulomblike tensor potential can be solved exactly [20]; also, he exactly solved Dirac equation with tensor potential containing a linear and Coulomblike terms too [21]. Aydoğdu and Sever obtained exact solution of Dirac equation for the pseudoharmonic potential in the presence of linear tensor potential under the pseudospin symmetry and showed that tensor interactions remove all degeneracies between members of pseudospin doublets [22]. Zhou et al. solved Dirac equation approximately for Hulthén potential including Coulomblike tensor potential with arbitrary spinorbit coupling number under spin and pseudospin symmetry limit [10]. Aydoğdu and Sever solved approximately for the WoodsSaxon potential and a tensor potential with the arbitrary spinorbit coupling quantum number under pseudospin and spin symmetry [23]. Very recently, Hamzavi et al. gave exact solutions of the Dirac equation for Mietype potential and positiondependent mass Coulomb potential with a Coulomblike tensor potential [24, 25] and pseudoharmonic potential with linear plus Coulomblike tensor potential [26].
The tPT potential has been proposed for the first time by Pöschl and Teller [27] in 1933 to describe the diatomic molecular vibration. Chen [28] and Zhang and Wang [29] have studied the relativistic bound state solutions for the tPT potential and hyperbolical PT (Second PT) potential, respectively. Liu et al. [30] studied the tPT potential within the framework of the Dirac theory. Recently, Candemir [31] investigated the analytical wave solutions of Dirac equation for tPT potential under the spin symmetry condition. Very recently, Hamzavi and Rajabi [32] studied the exact wave solution of the Schrödinger equation for the vibrational tPT potential. The tPT takes the form: where the parameters and describe the property of the potential well, while the parameter is related to the range of this potential [30]. We find out that this potential has a minimum value at . The case when , the minimum value is at for . The second derivative which determines the force constants at is given by for any value, and thus which means that at has a relative minimum for . When then minimum value is and . In Figures 1(a) and 1(b), we draw the tPT potential (1) for parameter values , and . Here the potential has a minimum value at . The curve is nodeless in . For example, with and minimum potential . It is worthy to note that in the limiting case when , the tPT potential can be reduced to the Kratzer potential [33, 34] , where is the equilibrium intermolecular separation and is the dissociation energy between diatomic molecules. In our case, , and . In the case of it reduces to the molecular potential which is called the modified Kratzer potential proposed by Simons et al. [35] and Molski and Konarski [36]. In the case of , this potential turns into the Kratzer potential, which includes an attractive Coulomb potential and a repulsive inverse square potential introduced by Kratzer in 1920 [37].
(a)
(b)
The aim of the present work is to extend our previous work [32] to the relativistic case and (rotational case) including a Coulomblike tensor potential. We introduce a convenient approximation scheme to deal with the strong singular centrifugal term. The ansätz of this approximation possesses the same form of the potential and is singular as the centrifugal term .
Since the relativistic solution is indispensable, we need to solve the Dirac equation with flexible parameters tPT potential model. However, the DiractPT problem can no longer be solved in a closed form due to the existence of spinorbit coupling term and it is necessary to resort to approximation methods. Therefore, we use an approximation scheme to deal with this term and solve approximately the Dirac equation with the tPT potential for arbitrary spinorbit quantum number . In the presence of spin and spin symmetric limitation, we obtain the approximate relativistic bound state solutions including the energy eigenvalue equations and the corresponding unnormalized upper and lowerspinor components of the wave functions using the concepts of parametric generalization of the NU method [38] since the relativistic corrections are not neglected.
Over the past years, the NikiforovUvarov (NU) method [39] has shown to be a powerful tool in solving the secondorder differential equation. It was applied successfully to a large number of potential models [40–46]. This method has also been used to solve the spinless (spin) Schrödinger [47–51] and KleinGordon (KG) [52–57] equations and also relativistic spin Dirac equation [58–63] with different potential models.
The structure of the paper is as follows. In Section 2, in the context of spin and spin symmetry, we briefly introduce the Dirac equation with scalar and vector tPT and also tensor potential potentials for arbitrary spinorbit quantum number . The parametric generalization of the NU method is displayed in the appendix. In the presence of the spin and spin symmetry, the approximate energy eigenvalue equations and corresponding twocomponent wave functions of the DiractPT problem are obtained, and effect of tensor potential is shown in this section. The nonrelativistic limit of the problem is discussed in this section too. Finally, our final concluding remarks are given in Section 3.
2. Dirac Equation including Tensor Coupling
The Dirac equation for fermionic massive spin particles moving in an attractive scalar potential , a repulsive vector potential , and a tensor potential is where is the relativistic energy of the system, is the threedimensional momentum operator, and is the mass of the fermionic particle [64]. and are the usual Dirac matrices given as where is unitary matrix and are threevector spin matrices The total angular momentum operator and spinorbit operator , where is orbital angular momentum operator, of the spherical nucleons commute with the Dirac Hamiltonian. The eigenvalues of spinorbit coupling operator are and for unaligned spin and the aligned spin , respectively. () can be taken as the complete set of the conservative quantities. Thus, the spinor wave functions can be classified according to their angular momentum , spinorbit quantum number , and the radial quantum number and can be written as follows: where is the upper (large) component and is the lower (small) component of the Dirac spinors. and are spin and pseudospin spherical harmonics, respectively, and is the projection of the angular momentum on the axis. Substituting (7) into (4) and using the following relations: with the following properties: one obtains two coupled differential equations for upper and lower radial wave functions and aswhere Eliminating and from (10a) and (10b), we obtain the following two Schrödingerlike differential equations for the upper and lower radial spinor components, respectively: where and . The quantum number is related to the quantum numbers for spin symmetry and pseudospin symmetry as and the quasidegenerate doublet structure can be expressed in terms of a pseudospin angular momentum and pseudoorbital angular momentum , which is defined as where . For example, and can be considered as pseudospin doublets.
2.1. Spin Symmetric Limit
In the spin symmetric limitation, or [7, 65–67]; then, (11) with and tensor potential as Coulomb potential, becomeswhere is new spinorbit centrifugal term and and for and , respectively. The Schrödingerlike equation (15a) that results from the Dirac equation is a secondorder differential equation containing a spinorbit centrifugal term which has a strong singularity at and needs to be treated very carefully while performing the approximation. In absence of tensor interaction, (15a) has an exact rigorous solution only for the states with because of the existence of the centrifugal term. However, when this term taken into account, the corresponding radial Dirac equation can no longer be solved in a closed form, and it is necessary to resort to approximate methods. Over the last few decades, several schemes have been used to calculate the energy spectrum. The main idea of these schemes relies on using different approximations of the spinorbit centrifugal coupling term . So, we need to perform a new approximation for the spinorbit term as a function of the tPT potential parameters. Therefore, we resort to use an appropriate approximation scheme to deal with the centrifugal potential term as where is a dimensionless shifting parameter and . The approximation (16) is done on the basis that and in the limit when . To show the validity and accuracy of our choice to the approximation scheme (16), we plot the centrifugal potential term and its approximations: and in Figure 2. As illustrated, the three curves coincide together and show how accurate this replacement is.
Thus, employing such an approximation scheme, we can then write (15a) as Followed by making a new change of variables , this allows us to decompose the spinsymmetric Dirac equation (17) into the Schrödingertype equation satisfying the upperspinor component , where has been used. If the previous equation is compared with , we can obtain the specific values for constants as In order to obtain the bound state solutions of (17), it is necessary to calculate the remaining parametric constants, that is, , by means of the relation . Their specific values are displayed in Table 1 for the relativistic tPT potential model. Further, using these constants along with , we can readily obtain the energy eigenvalue equation for the DiractPT problem as or equivalently To show the procedure of determining the energy eigenvalues from (21), we take a set of physical parameter values,, , , , and , and [30].

In Tables 2 and 3, we present the energy spectrum for the spin symmetric case. Obviously, the pairs , and so on are degenerate states. Thus, each pair is considered as spin doublet and has positive energy. In Table 2, we can see that tensor interaction removes degeneracies between spin doublets. Further, when potential range parameter approaches zero, the energy eigenvalues approaches a constant. From (21), we find that this constant is ; that is, , which can be seen from Table 3 too.


In Figure 3, we have investigated the effect of the tensor potential on the spin doublet splitting by considering the following pairs of orbital: and . We observe that in the case of (no tensor interaction), members of spin doublets have same energy. However, in the presence of the tensor potential, these degeneracies are removed. We can also see that spin doublet splitting increases with increasing. The reason is that term gives different contributions to each level in the spin doublet because takes different values for each state in the spin doublet.
On the other hand, in order to establish the upperspinor component of the wave functions , namely, (15a), the relations , , , and are used. Firstly, we find the first part of the wave function as Secondly, we calculate the weight function as which gives the second part of the wave function as where are the orthogonal Jacobi polynomials. Finally the upper spinor component for arbitrary can be found through the relation or where and is the normalization constant. Further, the lowerspinor component of the wave function can be calculated by using where and in the presence of the exact spin symmetry (), only positive energy states do exist.
2.2. pSpin Symmetric Limit
Ginocchio showed that there is spin symmetry in case when the relationship between the vector potential and the scalar potential is given by [7]. Further, Meng et al. showed that if , then , for which the spin symmetry is exact in the Dirac equation [65–67]. Thus, choosing the as tPT potential and as Coulomb potential, (12) under this symmetry becomeswhere, and for and , respectively. Employing the new approximation for the spinorbit pseudocentrifugal term,, that is, (16), the spin Dirac equation (29a) can be written as To avoid repetition of the negative energy solution of (30), the spin symmetric case can be readily obtained directly via the spin symmetric solution throughout the following parametric mappings: Following the previous procedure, one can obtain the spin symmetric energy equation as Furthermore, the lowerspinor component of the wave functions is found as with where is the normalization constant.
In Tables 4 and 5, we give the numerical results for the spin symmetric case. In this case, we take the set of parameter values, , , , , and , and [30]. We observe the degeneracy in the following doublets,,, ,, and so on. Thus, each pair is considered as spin doublet and has negative energy. In Table 4, we can see that tensor interaction removes degeneracies between spin doublets.


In Figure 4, we have investigated the effect of the tensor potential on the spin doublet splitting by considering the following pairs of orbital: and , and one can observe that the results obtained in the spin symmetric limit resemble the ones observed in the spin symmetric limit.
On the other hand, the upperspinor component of the Dirac wave function can be calculated by where , and in the presence of the exact spin symmetry (), only negative energy states do exist.
2.3. The Nonrelativistic Limiting Case
In this section, we study the energy eigenvalue equation (21) and upperspinor component of wave function (26) of the DiractPT problem under the nonrelativistic limits: ,,, and . Thereby, we obtain the energy equation of the Schrödinger equation with any arbitrary orbital state for the tPT potential as In the limit when , the vibrationrotation energy formula (36) reduces into a constant value: Further, there is no loss of generality if ; then, (36) becomes where and are the vibration and rotation quantum numbers, respectively. To obtain numerical energy eigenvalues for the present potential model, we take the following set of parameter values; namely, , , , and , and [30]. As seen from Table 6, in the limit when potential range parameter approaches zero, the energy eigenvalues approach a constant value given by (37).

Also, we can get the radial wave functions of the Schrödinger equation with tPT potential as Inserting in the previous equation, we can obtain where is a normalization factor to be calculated from the normalization conditions.
3. Concluding Remarks
In this work, we have studied the bound state solutions of the Dirac equation with trigonometric PöschlTeller and Coulomblike tensor potentials for any spinorbit quantum number . By making an appropriate approximation to deal with the spinorbit centrifugal (pseudocentrifugal) coupling term, we have obtained the approximate energy eigenvalue equation and the unnormalized two components of the radial wave functions expressed in terms of the Jacobi polynomials using the NU method. It is found that tensor interaction removes degeneracies between each pair of pseudospin or spin doublets.
Appendix
Parametric Generalization of the NU Method
The NU method is used to solve secondorder differential equations with an appropriate coordinate transformation [39] where and are polynomials, at most of second degree, and is a firstdegree polynomial. To make the application of the NU method simpler and direct without need to check the validity of solution, we present a shortcut for the method. So, at first, we write the general form of the Schrödingerlike equation (A.1) in a more general form applicable to any potential as follows [38]: satisfying the wave functions Comparing (A.2) with its counterpart (A.1), we obtain the following identifications: Following the NU method [39], we obtain the following [38]:
(i) the relevant constants: (ii) the essential polynomial functions: (iii) the energy equation: