<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">AM</journal-id><journal-title-group><journal-title>Applied Mathematics</journal-title></journal-title-group><issn pub-type="epub">2152-7385</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/am.2013.410A3001</article-id><article-id pub-id-type="publisher-id">AM-37488</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  Solutions of the Dirac Equation with Gravitational plus Exponential Potential
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>enedict</surname><given-names>Iserom Ita</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Alexander</surname><given-names>Immaanyikwa Ikeuba</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Pure and Applied Chemistry, University of Calabar, Calabar, Nigeria</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>iserom2001@yahoo.com(EII)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>10</day><month>10</month><year>2013</year></pub-date><volume>04</volume><issue>10</issue><fpage>1</fpage><lpage>6</lpage><history><date date-type="received"><day>July</day>	<month>14,</month>	<year>2013</year></date><date date-type="rev-recd"><day>August</day>	<month>14,</month>	<year>2013</year>	</date><date date-type="accepted"><day>August</day>	<month>21,</month>	<year>2013</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   The solutions of the Alhaidari formalism of the Dirac equation for the gravitational plus exponential potential have been presented using the parametric Nikiforov-Uvarov method. The energy eigenvalues and the corresponding unnormalized eigenfunctions are obtained in terms of Laguerre polynomials. 
 
</p></abstract><kwd-group><kwd>Dirac Equation; Alhaidari Formalism; Gravitational Potential; Exponential Potential; Nikiforov-Uvarov Method</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The bound state solutions of the Dirac equation are only possible for some potentials of physical interest [1-5]. These solutions could be exact or approximate and they nornally contain all the necessary information for the quantum system. Quite recently, several authors have tried to solve the problem of obtaining exact or approximate solutions of the Dirac equation for a number of special potentials using different methods [6-20]. Some of these potentials are known to play very important roles in many fields of Physics such as Molecular Physics, Solid State and Chemical Physics [<xref ref-type="bibr" rid="scirp.37488-ref21">21</xref>]. When a particle is in a strong potential field, the relativistic effects must be considered, leading to the relativistic quantum mechanical description of such a particle [22-26]. In the relativistic limit, the particle’s motions are very often described using either the Klien-Gordon (KG) equation or the Dirac equation depending on the spin character of the particle [23,24]. The spin-zero particles like the mesons are satisfactorily described by the KG equation while the spin-half particles such as the electrons are described by the Dirac equation. It is therefore of interest in nuclear and high energy physics to obtain exact solutions of the KG and Dirac equations.</p><p>The purpose of the present work is to present the solution of the Alhaidari formalism of the Dirac equation [<xref ref-type="bibr" rid="scirp.37488-ref25">25</xref>] with the gravitational plus exponential potential (GEP) of the form:</p><disp-formula id="scirp.37488-formula10368"><label>(1)</label><graphic position="anchor" xlink:href="1-7401725\6808a137-e868-4399-8519-26d5fca29d0c.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7401725\53f90c5c-320e-4dd8-8cbb-e8c45fe9b561.jpg" /> is the displacement, <img src="1-7401725\aeee0a3b-3cd3-43b1-a176-2824a9c790d1.jpg" />is the momentum, <img src="1-7401725\08998fe9-985a-42d1-b4f3-27ef4f1b75cc.jpg" />is the mass, <img src="1-7401725\4eff6161-07f1-418b-b98b-795794088fb1.jpg" />is gravitational acceleration and δ is an adjustable parameter. The GEP could be used to calculate the energy of a body falling under gravity from quantum mechanical point of view. Berberan-Santos et al. [<xref ref-type="bibr" rid="scirp.37488-ref22">22</xref>] have studied the motion of a particle in a gravitational field using the GEP without the exponential term. They obtained the classical and quantum mechanical position probability distribution function for the particle. Also quite recently, Ita and Ikeuba [<xref ref-type="bibr" rid="scirp.37488-ref27">27</xref>] have obtained the bound state solutions of the Klein-Gordon equation for the GEP using the parametric NU method. However, not much has been achieved in the area of solving the Dirac equation with GEP in the literature.</p></sec><sec id="s2"><title>2. The Dirac Equation</title><p>The Dirac equation for the lower and upper spinor components can be written as [<xref ref-type="bibr" rid="scirp.37488-ref25">25</xref>]:</p><disp-formula id="scirp.37488-formula10369"><label>(2)</label><graphic position="anchor" xlink:href="1-7401725\e39c0a16-c972-4d42-b816-90656a9cbc6b.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7401725\d1dacb0a-31f9-412f-b07c-3e48ac8c1a06.jpg" /> is the rest mass, <img src="1-7401725\ab9962dc-5ec2-48df-b12b-d34c1ed0b975.jpg" />is the relativistic energy, and <img src="1-7401725\d21088d4-1e2c-4a42-9c25-4a380008476b.jpg" /> is the vector potential.</p><disp-formula id="scirp.37488-formula10370"><label>(3)</label><graphic position="anchor" xlink:href="1-7401725\8853f379-d95f-4528-a99c-0d915ac4e392.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7401725\029480cf-6c9a-4934-83b2-dc6a215539a9.jpg" /> and <img src="1-7401725\1c7068c4-0131-42ef-93f0-29817ad24a00.jpg" /> is a real parameter. The “<img src="1-7401725\654fb560-d5ed-4f24-8676-dea16533b487.jpg" />” designate the upper and lower components respectively.</p></sec><sec id="s3"><title>3. The Nikiforov-Uvarov Method</title><p>The Nikiforov-Uvarov (NU) method is based on the solutions of a generalized second-order linear differential equation with special orthogonal functions [<xref ref-type="bibr" rid="scirp.37488-ref28">28</xref>]. The Schrodinger equation of the type as:</p><disp-formula id="scirp.37488-formula10371"><label>(4)</label><graphic position="anchor" xlink:href="1-7401725\f5a2df10-2923-4799-aad0-3ec16e54b498.jpg"  xlink:type="simple"/></disp-formula><p>can be solved by this method. This can be done by transforming Equation (2) into an equation of hypergeometric type with appropriate coordinate transformation <img src="1-7401725\42ed7115-0fbf-431a-8d3e-691d1c92c004.jpg" /> to get</p><disp-formula id="scirp.37488-formula10372"><label>(5)</label><graphic position="anchor" xlink:href="1-7401725\d2479a9f-19f3-43db-8e38-312e7c937344.jpg"  xlink:type="simple"/></disp-formula><p>To find the exact solution to Equation (3), we write <img src="1-7401725\ab358bad-737c-45cf-9d54-127916983b2e.jpg" /> as</p><disp-formula id="scirp.37488-formula10373"><label>. (6)</label><graphic position="anchor" xlink:href="1-7401725\4fcd1bc3-bcc8-443e-bb11-f982f6bc3c05.jpg"  xlink:type="simple"/></disp-formula><p>Substitution of Equation (6) into Equation (5) yields Equation (7) of hypergeometric type as</p><disp-formula id="scirp.37488-formula10374"><label>(7)</label><graphic position="anchor" xlink:href="1-7401725\20469516-52ca-49a1-a146-cc2b3628a227.jpg"  xlink:type="simple"/></disp-formula><p>In Equation (6), the wave function <img src="1-7401725\0de93dab-f6ca-4035-a556-7eeeca692954.jpg" /> is defined as the logarithmic derivative [<xref ref-type="bibr" rid="scirp.37488-ref29">29</xref>]</p><disp-formula id="scirp.37488-formula10375"><label>(8)</label><graphic position="anchor" xlink:href="1-7401725\d53a9bbf-fe8b-4877-80c3-0639029ad481.jpg"  xlink:type="simple"/></disp-formula><p>with <img src="1-7401725\70f81f01-c095-4317-a0de-490df87378fa.jpg" /> being at most first order polynomials. Also, the hypergeometric-type functions in Equation (7) for a fixed integer <img src="1-7401725\7963d8ac-d73d-4a3d-91a1-a69c791f2dd0.jpg" /> is given by the Rodrigue relation as</p><disp-formula id="scirp.37488-formula10376"><label>(9)</label><graphic position="anchor" xlink:href="1-7401725\6384f867-d253-41bd-b3dc-1cddea8e0dcc.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7401725\de65e257-7680-41e2-8b84-4814875446a4.jpg" /> is the normalization constant and the weight function <img src="1-7401725\062e45fb-1eea-49e8-869e-db5972d2ce36.jpg" /> must satisfy the condition</p><disp-formula id="scirp.37488-formula10377"><label>(10)</label><graphic position="anchor" xlink:href="1-7401725\69bf13d5-157b-4842-b58a-a7efdd44d644.jpg"  xlink:type="simple"/></disp-formula><p>with</p><disp-formula id="scirp.37488-formula10378"><label>(11)</label><graphic position="anchor" xlink:href="1-7401725\b5ee5959-7ec6-45df-97fa-1770186b8c97.jpg"  xlink:type="simple"/></disp-formula><p>In order to accomplish the condition imposed on the weight function <img src="1-7401725\318c4b54-1b58-4196-a9d3-f5fdc4d8cd59.jpg" /> it is necessary that the polynomial <img src="1-7401725\cf5ac34d-7880-4b1b-9981-83f34f032349.jpg" /> be equal to zero at some point of an interval <img src="1-7401725\df7b3571-683c-40d9-b429-59bf5021a6c1.jpg" /> and its derivative at this interval at <img src="1-7401725\90760ac7-e84f-4f76-8615-fcfe33d90b96.jpg" /> will be negative [<xref ref-type="bibr" rid="scirp.37488-ref30">30</xref>]. That is</p><disp-formula id="scirp.37488-formula10379"><label>(12)</label><graphic position="anchor" xlink:href="1-7401725\72f01dd9-06a5-4d13-b0b9-257233321a5d.jpg"  xlink:type="simple"/></disp-formula><p>The function <img src="1-7401725\fffec241-e0d4-4894-9052-e3d2d1d61d62.jpg" /> and the parameter <img src="1-7401725\9acaf251-539e-422f-863c-5b7969aec128.jpg" /> required for the NU method are then defined as [<xref ref-type="bibr" rid="scirp.37488-ref31">31</xref>]</p><disp-formula id="scirp.37488-formula10380"><label>. (13)</label><graphic position="anchor" xlink:href="1-7401725\f2ce137d-e0f1-461b-9227-b9b6dab15297.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.37488-formula10381"><label>(14)</label><graphic position="anchor" xlink:href="1-7401725\471618bb-e7c5-4a14-b31d-710d25e951f2.jpg"  xlink:type="simple"/></disp-formula><p>The values in Equation (13) are possible to evaluate if the expression under the square-root be square of polynomials. This is possible if and only if its discriminant is zero. Therefore, the new eigenvalue equation becomes [<xref ref-type="bibr" rid="scirp.37488-ref29">29</xref>]</p><disp-formula id="scirp.37488-formula10382"><label>(15)</label><graphic position="anchor" xlink:href="1-7401725\4dd28cea-665e-4bae-9db4-6a8085f4f5e5.jpg"  xlink:type="simple"/></disp-formula><p>A comparison between Equations (14) and (15) yields the energy eigenvalues.</p><p>Secondly, the parametric generalization of the NU method is expressed by the generalized hypergeometric-type equation [<xref ref-type="bibr" rid="scirp.37488-ref32">32</xref>]</p><disp-formula id="scirp.37488-formula10383"><label>(16)</label><graphic position="anchor" xlink:href="1-7401725\513fa753-f142-4c65-82e9-4a4be0fcd646.jpg"  xlink:type="simple"/></disp-formula><p>Equation (16) is solved by comparing it with Equation (5) and the following polynomials are obtained:</p><disp-formula id="scirp.37488-formula10384"><label>(17)</label><graphic position="anchor" xlink:href="1-7401725\7a931a7c-dac0-453f-9c0f-c21643cd924d.jpg"  xlink:type="simple"/></disp-formula><p>Now, substituting Equation (17) into Equation (13) gives</p><disp-formula id="scirp.37488-formula10385"><label>(18)</label><graphic position="anchor" xlink:href="1-7401725\c5fd09e4-cb6f-49c4-8770-94173d702988.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.37488-formula10386"><label>(19)</label><graphic position="anchor" xlink:href="1-7401725\4bbc0d47-cea0-42a3-bf6d-7422755cc976.jpg"  xlink:type="simple"/></disp-formula><p>The resulting value of <img src="1-7401725\86c6ffa9-ba9f-4f2e-a172-29883bdaddc2.jpg" /> in Equation (18) is obtained from the condition that the function under the square-root should be square of a polynomial and we get</p><disp-formula id="scirp.37488-formula10387"><label>(20)</label><graphic position="anchor" xlink:href="1-7401725\31601bf1-3000-443f-9ea8-98299883cb55.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.37488-formula10388"><label>(21)</label><graphic position="anchor" xlink:href="1-7401725\a8612483-4854-4d6b-a8f5-8e3627829de6.jpg"  xlink:type="simple"/></disp-formula><p>The new <img src="1-7401725\3f01c3a9-f022-44ce-8b3a-5f07d01e78a3.jpg" /> for <img src="1-7401725\ab0c2bc5-81f7-4e4e-bb27-6b338e51f0f3.jpg" /> becomes</p><disp-formula id="scirp.37488-formula10389"><label>(22)</label><graphic position="anchor" xlink:href="1-7401725\443e43fa-f995-430e-b27e-16c00b464b37.jpg"  xlink:type="simple"/></disp-formula><p><img src="1-7401725\593da689-c271-4863-afa1-e5504650be71.jpg" />value becomes</p><disp-formula id="scirp.37488-formula10390"><label>. (23)</label><graphic position="anchor" xlink:href="1-7401725\de81abc4-4d78-4111-8c05-43ff4aa78a52.jpg"  xlink:type="simple"/></disp-formula><p>Using Equation (11), we obtain</p><disp-formula id="scirp.37488-formula10391"><label>(24)</label><graphic position="anchor" xlink:href="1-7401725\9304126e-dd2c-415f-98a9-a37b24f393ef.jpg"  xlink:type="simple"/></disp-formula><p>The physical condition for the bound state solution is <img src="1-7401725\779b60e3-4fd6-4ccb-b2fa-1a5baa1d2d89.jpg" /> and thus</p><disp-formula id="scirp.37488-formula10392"><label>(25)</label><graphic position="anchor" xlink:href="1-7401725\9971a89b-114b-4a20-bd79-0b3f8b2d6e13.jpg"  xlink:type="simple"/></disp-formula><p>With the aid of Equations (12) and (13), we obtain the energy equation as</p><disp-formula id="scirp.37488-formula10393"><label>(26)</label><graphic position="anchor" xlink:href="1-7401725\83c047e6-d208-431d-b976-de9f3f37e993.jpg"  xlink:type="simple"/></disp-formula><p>The weight function <img src="1-7401725\2267c2e6-e919-4b3c-b6e7-d7cd51449d77.jpg" /> is obtained from Equation (10) as</p><disp-formula id="scirp.37488-formula10394"><label>(27)</label><graphic position="anchor" xlink:href="1-7401725\760d290e-5abc-4e09-ab9d-c72cea7f662d.jpg"  xlink:type="simple"/></disp-formula><p>And together with Equation (9), we have</p><disp-formula id="scirp.37488-formula10395"><label>(28)</label><graphic position="anchor" xlink:href="1-7401725\1e90864a-ee1e-4b12-a9ce-aa7806c6de72.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.37488-formula10396"><label>(29)</label><graphic position="anchor" xlink:href="1-7401725\a5d72019-9ebc-487c-9884-11f806e73e7f.jpg"  xlink:type="simple"/></disp-formula><p><img src="1-7401725\ff2d4a85-d994-4180-81f8-547dd08c6ab5.jpg" />are the Jacobi polynomials. The second part of the wave function is obtained from Equation (6) as</p><disp-formula id="scirp.37488-formula10397"><label>(30)</label><graphic position="anchor" xlink:href="1-7401725\ab605afc-dffe-4eb6-9483-473959bb1924.jpg"  xlink:type="simple"/></disp-formula><p>where</p><p><img src="1-7401725\2e693559-6420-4a31-95a6-af6d6cddbd50.jpg" /></p><disp-formula id="scirp.37488-formula10398"><label>. (31)</label><graphic position="anchor" xlink:href="1-7401725\d96007e9-a222-42b1-a90e-7eebb0d61924.jpg"  xlink:type="simple"/></disp-formula><p>Thus the total wave function becomes</p><disp-formula id="scirp.37488-formula10399"><label>(32)</label><graphic position="anchor" xlink:href="1-7401725\514937ad-7d88-4e41-9758-0b3eca242d93.jpg"  xlink:type="simple"/></disp-formula><p>where N<sub>n</sub> is the normalization constant.</p></sec><sec id="s4"><title>4. Solutions of the Dirac Equation</title><p>The potential in Equation (1) can be written as</p><disp-formula id="scirp.37488-formula10400"><label>. (33)</label><graphic position="anchor" xlink:href="1-7401725\1b031eb7-1cf4-4ed9-84a0-f677987b797b.jpg"  xlink:type="simple"/></disp-formula><p>where<img src="1-7401725\0f268cc6-0939-4c6f-b687-6d4cf5fc09a4.jpg" />. We can also write Equation (33) as</p><disp-formula id="scirp.37488-formula10401"><label>. (34)</label><graphic position="anchor" xlink:href="1-7401725\f4d6af29-d135-44ee-9eb2-a096efda0207.jpg"  xlink:type="simple"/></disp-formula><p>On arranging Equation (34) we get our working potential as</p><disp-formula id="scirp.37488-formula10402"><label>. (35)</label><graphic position="anchor" xlink:href="1-7401725\f6b27907-a963-45bb-aafc-105a8a191a64.jpg"  xlink:type="simple"/></disp-formula><p>The potential of Equation (35) can be used to solve various quantum mechanical equations including the Schrodinger equation (SE), Klein-Gordon equation (KG) and Dirac equation using the NU method for their exact solutions. Writing Equation (32) with the GEP we get</p><disp-formula id="scirp.37488-formula10403"><label>. (36)</label><graphic position="anchor" xlink:href="1-7401725\8ef20fa5-ba86-4d3b-8bb3-dd39e821ac67.jpg"  xlink:type="simple"/></disp-formula><p>Ignoring all terms of the form <img src="1-7401725\76587d8d-bf05-44b5-8201-c2ae05d6e7d6.jpg" /> with <img src="1-7401725\5b7d30e1-8067-485f-a15b-ac22a09d87be.jpg" /> in Equation (36) as these will not affect the physics of the calculations, we write Equation (36) as</p><disp-formula id="scirp.37488-formula10404"><label>(37)</label><graphic position="anchor" xlink:href="1-7401725\7cada1f2-e62e-448b-bd50-448256b62c8e.jpg"  xlink:type="simple"/></disp-formula><p>where we have used <img src="1-7401725\d6aaadcc-f5c3-4006-9259-5c990db8299e.jpg" /> and <img src="1-7401725\8de81ddf-7853-4929-b8f9-2ba18e110fb9.jpg" /> transformation in Equation (36).</p><p>Comparing Equation (37) with Equation (16) yields the following parameters</p><disp-formula id="scirp.37488-formula10405"><label>(38)</label><graphic position="anchor" xlink:href="1-7401725\3cbf5bcd-d70c-406d-945c-71492c0d6cc5.jpg"  xlink:type="simple"/></disp-formula><p>Other coefficients are determined as</p><disp-formula id="scirp.37488-formula10406"><label>(39)</label><graphic position="anchor" xlink:href="1-7401725\5bbff20c-41f6-4edb-9f7e-98162ac92276.jpg"  xlink:type="simple"/></disp-formula><p>From Equation (16)</p><disp-formula id="scirp.37488-formula10407"><label>(40)</label><graphic position="anchor" xlink:href="1-7401725\708d6802-1d21-4cd8-9b49-c779a4e0e5fa.jpg"  xlink:type="simple"/></disp-formula><p>From Equation (18)</p><disp-formula id="scirp.37488-formula10408"><label>. (41)</label><graphic position="anchor" xlink:href="1-7401725\0916b4ac-3530-4f46-a006-a45691bb0dd5.jpg"  xlink:type="simple"/></disp-formula><p>From Equation (22)</p><disp-formula id="scirp.37488-formula10409"><label>. (42)</label><graphic position="anchor" xlink:href="1-7401725\b411b3a9-da63-4e22-9fa9-fb986b8381e0.jpg"  xlink:type="simple"/></disp-formula><p>The negative derivative of Equation (42) then becomes</p><disp-formula id="scirp.37488-formula10410"><label>. (43)</label><graphic position="anchor" xlink:href="1-7401725\ae7b021f-73e1-4da3-aa56-3e0ec9dceba6.jpg"  xlink:type="simple"/></disp-formula><p>The new <img src="1-7401725\41cd2a2e-ae1e-44a0-b2b7-b54d39f33d82.jpg" /> for the NU method is chosen as</p><disp-formula id="scirp.37488-formula10411"><label>. (44)</label><graphic position="anchor" xlink:href="1-7401725\ddb7204a-a85a-477e-8b32-144ff8927d4f.jpg"  xlink:type="simple"/></disp-formula><p>For</p><disp-formula id="scirp.37488-formula10412"><label>. (45)</label><graphic position="anchor" xlink:href="1-7401725\a3fe21e4-c14c-44ce-b309-1618245da808.jpg"  xlink:type="simple"/></disp-formula><p>Now using Equations (24), (38) and (39) we obtain the energy spectrum of the GEP as</p><disp-formula id="scirp.37488-formula10413"><label>(46)</label><graphic position="anchor" xlink:href="1-7401725\0d5c4953-f705-42cd-8a07-cf40654b5aba.jpg"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.37488-formula10414"><label>(47)</label><graphic position="anchor" xlink:href="1-7401725\3dbba9f6-8874-4092-8f3d-28a1633299bd.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.37488-formula10415"><label>(48)</label><graphic position="anchor" xlink:href="1-7401725\21174ccf-a445-4c2d-8cdb-b61d1192793a.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.37488-formula10416"><label>. (49)</label><graphic position="anchor" xlink:href="1-7401725\7e061eaf-490a-4621-be27-404b4ce1f471.jpg"  xlink:type="simple"/></disp-formula><p>The weight function <img src="1-7401725\c13d6b9c-4b4a-48db-af15-818d4f1511d9.jpg" /> is obtained from Equation (25) and the parameters of Equation (39) as</p><disp-formula id="scirp.37488-formula10417"><label>(50)</label><graphic position="anchor" xlink:href="1-7401725\3411ef43-58f4-4242-b54f-d2b38e2880eb.jpg"  xlink:type="simple"/></disp-formula><p>and using Equation (26) we get the wavefunction χ<sub>n</sub>(s) as</p><disp-formula id="scirp.37488-formula10418"><label>(51)</label><graphic position="anchor" xlink:href="1-7401725\6a291ec6-cd3c-4ad5-be27-9af6a7694d8d.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7401725\8431ee2e-4a58-4088-aa3b-72cd4186a8f0.jpg" /> and <img src="1-7401725\eb255101-010f-4c86-b9c6-c2e332297a7c.jpg" /> is the Laguerre polynomial. From Equation (28) the wave function is</p><disp-formula id="scirp.37488-formula10419"><label>. (52)</label><graphic position="anchor" xlink:href="1-7401725\5abf681c-dffc-4cc8-8fb0-cdd746188b0b.jpg"  xlink:type="simple"/></disp-formula><p>The unnormalized wave function is then obtained from Equation (30) as</p><disp-formula id="scirp.37488-formula10420"><label>(53)</label><graphic position="anchor" xlink:href="1-7401725\8b84ecda-b956-4357-9b55-842c02b94c07.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="1-7401725\21383dfc-080f-4a58-ac9c-351a3c95a452.jpg" /> is the normalization constant.</p><p>In addition, the corresponding lower-spinor wave function is</p><disp-formula id="scirp.37488-formula10421"><label>. (54)</label><graphic position="anchor" xlink:href="1-7401725\9b66686f-4aa3-4d7d-9f50-d4c6582e5f2d.jpg"  xlink:type="simple"/></disp-formula></sec><sec id="s5"><title>5. Conclusion</title><p>In summary, we have obtained the energy eigenvalues and the corresponding un-normalized wavefunction using the parametric NU method for the Dirac equation with the gravitational plus exponential potential.</p></sec><sec id="s6"><title>6. Acknowledgements</title><p>The authors wish to acknowledge Dr. A. N. Ikot of the Department of Physics, University of Uyo in Nigeria for some useful discussions during the preparation of this paper.</p></sec><sec id="s7"><title>REFERENCES</title></sec><sec id="s8"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.37488-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">M. K. Bahar and F. 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