<?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">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2011.28092</article-id><article-id pub-id-type="publisher-id">JMP-6677</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>
 
 
  Spin Dependent Selection Rules for Photonic Transitions in Hydrogen-Like Atoms
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>iya</surname><given-names>Saglam</given-names></name><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mesude</surname><given-names>Saglam</given-names></name><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><author-notes><corresp id="cor1">* E-mail:<email>zsaglam@aksaray.edu.tr(IS)</email>;<email>saglam@science.ankara.edu.tr(MS)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>08</day><month>08</month><year>2011</year></pub-date><volume>02</volume><issue>08</issue><fpage>787</fpage><lpage>791</lpage><history><date date-type="received"><day>March</day>	<month>22,</month>	<year>2011</year></date><date date-type="rev-recd"><day>April</day>	<month>28,</month>	<year>2011</year>	</date><date date-type="accepted"><day>May</day>	<month>19,</month>	<year>2011</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>
 
 
  Spin dependent selection rules for photonic transitions in hydrogen-like atoms is derived by using the solution of Dirac equation for hydrogen-like atoms. It is shown that photonic transitions occur when [ Δj=0,&#177;1,&#177;2, while Δm&lt;sub&gt;j&lt;/sub&gt;=0,&#177;1,&#177;2 ]. By applying the spin dependent selection rules, we can explain the observed (6s→7s) transition in Cesium (Cs) atom.
 
</p></abstract><kwd-group><kwd>Dirac Hydrogen Atom</kwd><kwd> Hydrogen-Like (Hydrogenic) Atoms</kwd><kwd> Photonic Transitions</kwd><kwd> Selection Rules</kwd><kwd> Fermi-Golden Rule</kwd><kwd> Transition Rate.</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Applications of hydrogen-like atoms in technology are more than the hydrogen atom itself. Accurate determination of the excited-state properties of atomic and molecular systems, such as fine and hyperfine coupling constants, oscillator strengths play important roles for testing the high-precision atomic theory and quantum mechanics. The aim of the present study is to find spin dependent selection rules for photonic transitions in hydrogen-like atoms. We first derive the spin dependent eigenstates of the hydrogen-like atoms then find a more accurate correspondence between these eigenstates. So far in literature the states have been denoted by the quantum numbers (n, l, j) [<xref ref-type="bibr" rid="scirp.6677-ref1">1</xref>] but not by the quantum numbers (n, l, m<sub>j</sub>). In this way, we distinguish the states in the Zeeman sense including the quantum number, m<sub>j</sub>. By using the Fermi-Golden rule, we calculate the non-zero matrix elements and then develop the spin dependent selection rules for the photonic transitions in the hydrogen-like atoms. We show that photonic transitions occur when <img src="3-7500406\f42cab46-faca-4258-a8c4-36c644b5b913.jpg" /> and<img src="3-7500406\e2297b9c-dae1-421f-b5c5-7d912f6ff8de.jpg" />. By applying the spin dependent selection rules, we can explain the observed <img src="3-7500406\64d1ff18-297b-4ac9-9714-ff9c02c7b957.jpg" /> transition in Cesium (Cs) atom. The outline of the present study is as follows. In Section 2 we give a short summary of the Dirac hydrogen atom and then extend it to the hydrogen-like atoms. In Section 3 we develop the spin dependent transition rates for Dirac hydrogen-like atoms. In Section 4 we give the explanation of the (6 s - 7 s) transition of Cs in terms of the spin dependent selection rules. In Section 5 we give the conclusions.</p></sec><sec id="s2"><title>2. The Dirac Hydrogen Atom</title><p>To find the eigenvalue of the Dirac hydrogen-like atom, we will begin with the Dirac Hamiltonian of the hydrogen atom [2-4]:</p><disp-formula id="scirp.6677-formula84875"><label>(1)</label><graphic position="anchor" xlink:href="3-7500406\1912422d-448b-4ff1-b8c9-64ba08fdcc17.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="3-7500406\e5a29100-5d8a-46eb-ad4d-4b69e3c7abdc.jpg" /> is the Coulomb potential, m is the mass of an electron, c is the velocity of light, <img src="3-7500406\0b318394-ca5c-4908-bdaf-f9e82904ae9d.jpg" />and <img src="3-7500406\ed1f4cf4-9c99-4980-83d4-178133aeccdf.jpg" /> are the standard Dirac matrices in the Dirac representation:</p><disp-formula id="scirp.6677-formula84876"><label>(2)</label><graphic position="anchor" xlink:href="3-7500406\83c9789f-23f3-4356-be00-781b36ad261f.jpg"  xlink:type="simple"/></disp-formula><p>Here the 1's and 0's stand for 2 &#215; 2 unit and zero matrices respectively and the <img src="3-7500406\d69e5bf4-30e4-46e7-a89a-3a887943b88a.jpg" /> is the standard vector composed of the three Pauli matrices<img src="3-7500406\05cb650c-747e-45a4-a27d-1fab1e3bd226.jpg" />. Since the Hamiltonian is invariant under rotations, we look for simultaneous eigenfunctions of H<sub>D</sub>, |J|<sup>2</sup>, and J<sub>z</sub>, where</p><disp-formula id="scirp.6677-formula84877"><label>(3a)</label><graphic position="anchor" xlink:href="3-7500406\8c58c64a-6c54-4628-a1a4-7b8fcbcbdae4.jpg"  xlink:type="simple"/></disp-formula><p>and J<sub>z</sub> = L<sub>z</sub> + S<sub>z</sub> or m<sub>j</sub> = m + m<sub>s</sub>(3b)</p><p>We remark that the spin operator is diagonal in terms of 2 &#215; 2 Pauli spin matrices; therefore the angular part should be precisely that of the Pauli two-component theory. Defining</p><p><img src="3-7500406\6afadf2d-737c-4e03-9dde-1b9e005b4985.jpg" />and <img src="3-7500406\c3b2ed8c-ccd4-4341-9acb-e9b518b61661.jpg" /></p><p>the spin dependent wave functions can be written as [<xref ref-type="bibr" rid="scirp.6677-ref5">5</xref>]:</p><disp-formula id="scirp.6677-formula84878"><label>(4a)</label><graphic position="anchor" xlink:href="3-7500406\b65813ae-e341-4fd3-a912-7bb5e784f951.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.6677-formula84879"><label>(4b)</label><graphic position="anchor" xlink:href="3-7500406\23578c97-1a6a-41b5-a54b-dc0ee7e9b9a6.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="3-7500406\4676d548-a23e-468f-a3bb-425f3ccbf644.jpg" /> is the radial wave function, <img src="3-7500406\eec01e70-0c92-423c-ae8b-fbb8f903e61d.jpg" />are the spherical harmonics. Further in Equation (4a), <img src="3-7500406\836b34c4-93e1-48b1-963c-3992e44fe269.jpg" />can be replaced by (<img src="3-7500406\68065eb4-2415-44e9-8919-cb6be5e10c1c.jpg" />) (spin-up case);and in Equation(4b), <img src="3-7500406\65842a5f-afc7-4607-b0dd-cd10be81fc33.jpg" />can be replaced by <img src="3-7500406\60faa510-b8ca-4e63-9ee0-71c187513240.jpg" /> (spin-down case). In a hydro-gen-like atom the potential <img src="3-7500406\35c31209-0be1-4ee7-a44e-1fd2c2f01a4b.jpg" /> is replaced by<img src="3-7500406\2e1ca551-1a78-4e4a-b5c7-6021adf23829.jpg" />, where Z is the atomic number. So the spin dependent eigenfunctions for hydrogen-like atoms are written as:</p><p><img src="3-7500406\7af1d6a9-4a95-4eb8-a359-411c9f3f1251.jpg" />(5a)</p><p><img src="3-7500406\2d118d92-b604-49c5-82d1-1ae4e3ba0133.jpg" />(5b)</p><p>where</p><disp-formula id="scirp.6677-formula84880"><label>(5c)</label><graphic position="anchor" xlink:href="3-7500406\e5b89721-d129-4e8a-8fb8-00879c6327a0.jpg"  xlink:type="simple"/></disp-formula><p>Here <img src="3-7500406\be03fd5e-ccc2-4dbc-a417-53f9ad824533.jpg" /> are the Laguerre polynomials and <img src="3-7500406\28365483-1088-4acb-8ed3-1ad921f801dd.jpg" /> is the Bohr radius.</p></sec><sec id="s3"><title>3. Developing Spin Dependent Transition Rates for Photonic Transitions in Dirac Hydrogen-Like Atoms</title><p>To develop the spin dependent selection rules for hydrogen-like atoms, we need to consider energy shifts coming from the electric field E and the magnetic field B separately. When the atom is subject to an external electric and magnetic field, it will have interactions through the Hamiltonians: <img src="3-7500406\332ae4a6-71be-4bba-9f55-1a4b022607db.jpg" />and<img src="3-7500406\6e6ee540-67a5-4bce-aff0-0a9b9333bda7.jpg" />.</p><p>However, the electric and the magnetic field of a photon are not independent fields and they are related to each other with the same vector potential <img src="3-7500406\136a2167-90e6-4caa-a8c5-bc4f94321a9e.jpg" /> which obeys the Coulomb gauge condition (<img src="3-7500406\87873c1a-ad82-4bfc-9c1d-6ac99f1ae59e.jpg" />). In this case the electric and the magnetic field vectors are given by:</p><disp-formula id="scirp.6677-formula84881"><label>(6a)</label><graphic position="anchor" xlink:href="3-7500406\d1dfbbea-c5ed-45d0-ad46-af891d5d001e.jpg"  xlink:type="simple"/></disp-formula><p>and</p><disp-formula id="scirp.6677-formula84882"><label>(6b)</label><graphic position="anchor" xlink:href="3-7500406\e67f020f-aa8e-47a7-bd6a-840448010258.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="3-7500406\a8926e8f-b359-4844-a0a1-c78ffa0fee8f.jpg" /> is the wave vector of the photon.</p><p>In general the effect of the vector potential <img src="3-7500406\3245d475-fd39-4acc-ad8f-e29fb78cf76c.jpg" /> on electron is considered through the canonical momentum that produces an interaction potential <img src="3-7500406\de686abc-5572-411a-83ce-56fa1d3b9e02.jpg" /> which has the linear and the quadratic terms [<xref ref-type="bibr" rid="scirp.6677-ref6">6</xref>]:</p><disp-formula id="scirp.6677-formula84883"><label>(7)</label><graphic position="anchor" xlink:href="3-7500406\70cb8189-5c92-402d-b6e1-b0d053810812.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="3-7500406\a08c1f80-897c-4cbb-b75f-d513020eaf94.jpg" /> is the linear momentum of the electron.</p><p>We will see that to develop the selection rules for photonic transitions, the Hamiltonian <img src="3-7500406\114676de-befc-40fd-a368-f4b7507a4569.jpg" /> will be adequate and the Hamiltonian <img src="3-7500406\e2221dfd-2980-42b8-9296-c74ba20abf1b.jpg" /> will not produce anything new.</p><p>Let us first start with the effect of the electric field. In Dirac notations, if at t = 0 the electron is at an initial state</p><p>| i &gt; &#186;<img src="3-7500406\4122c91d-f84d-495c-8aac-18b578a24f58.jpg" /></p><p>given by Equation (5a) and Equation (5b), then at t &gt; 0, because of the interaction with H', there will be a non-zero transition rate to some other states</p><p>| f &gt;<img src="3-7500406\1ada4275-c932-4ed4-a81f-10fa4138f611.jpg" /></p><p>which will be called the final states. According to the Golden rule, the transition probability will be proportional to the square of the matrix element of H' between the initial and the final states:<img src="3-7500406\8e42d3b0-3005-4162-973c-8e4a693b8552.jpg" />. To calculate the matrix element<img src="3-7500406\8070be0a-9c53-447e-88ef-27990ed65a07.jpg" />, we follow a similar way as followed by Saglam et al. [<xref ref-type="bibr" rid="scirp.6677-ref5">5</xref>]. Namely we will consider two different cases: a) The polarization of the electric field is in x-y plane (along the xor the y-axis) b) The polarization of the electric field is in z-direction. Since the dipole moment vector <img src="3-7500406\0d194b78-fb3c-4fa8-902f-a677d3a1b224.jpg" /> is equal to (<img src="3-7500406\8108cdab-838a-45a5-afa8-d15626486eec.jpg" />), for the case a), we calculate the matrix elements of the quantities x &#177; iy= rsinq exp(&#177;if) and for the case b) we calculate the matrix elements of the quantity: rcos q. For the case a) we can write:</p><p><img src="3-7500406\bf64d003-49a4-4dfc-86b4-1c3f422ff492.jpg" /></p><p><img src="3-7500406\dde5b4db-2920-4cb4-b328-a058874f64f7.jpg" /></p><p><img src="3-7500406\e925f550-723e-41a5-84e7-7bd68c581172.jpg" /></p><p><img src="3-7500406\0ab0b0be-a36b-492d-8781-7e95a922e4ad.jpg" /></p><p><img src="3-7500406\b66b2dd9-e479-49d6-b08d-4a58dc419513.jpg" />.</p><disp-formula id="scirp.6677-formula84884"><label>(8)</label><graphic position="anchor" xlink:href="3-7500406\53dfb97e-8fef-4d35-81c4-4cca862ca7aa.jpg"  xlink:type="simple"/></disp-formula><p>Substitution of Equation (5a) in <img src="3-7500406\a76c57d7-bb0d-428d-adcc-d82d6ce1f2c3.jpg" /> we obtain:</p><disp-formula id="scirp.6677-formula84885"><label>(9)</label><graphic position="anchor" xlink:href="3-7500406\b3f1fb34-ad34-472e-8e3d-f423f599bc0a.jpg"  xlink:type="simple"/></disp-formula><p>which will be non-zero for:</p><p><img src="3-7500406\5062fc37-0d8a-4efd-8392-8f37c671be7c.jpg" />;<img src="3-7500406\9bc159bd-3198-4cd8-8683-01bd83a6dfe8.jpg" /> (10a)</p><p><img src="3-7500406\93c9bed2-5d7f-4eed-96f8-f41f2ed93344.jpg" />;<img src="3-7500406\abda94ae-cb04-4dbe-82f2-8041a7c3f952.jpg" /> (10b)</p><p>To evaluate the integral (9) we have used the relation:</p><disp-formula id="scirp.6677-formula84886"><label>(11)</label><graphic position="anchor" xlink:href="3-7500406\59ccf411-f8c3-4054-a8da-09a66aed6e46.jpg"  xlink:type="simple"/></disp-formula><p>Next substituting Equation (5b) in <img src="3-7500406\55890b0d-38e9-4389-baba-d9b29aeaf66c.jpg" /> we obtain:</p><disp-formula id="scirp.6677-formula84887"><label>(12)</label><graphic position="anchor" xlink:href="3-7500406\fbfe3388-8b02-41bb-b2e6-7afe2c4147fa.jpg"  xlink:type="simple"/></disp-formula><p>which will be non-zero for:</p><p><img src="3-7500406\8e174eb6-3291-4c39-8f0b-347c3d0d0f73.jpg" />;<img src="3-7500406\e53d1e99-9322-498a-aaf3-b3cf45640e28.jpg" /> (13a)</p><p><img src="3-7500406\f54ea873-2012-4ad3-861a-36ff8d1b5cf1.jpg" />;<img src="3-7500406\278abf47-6178-46fe-b1e4-09c38bf32aa2.jpg" /> (13b)</p><p>where we have used Equation (11) again.</p><p>Similarly substitution of Equations (5a) and (5b) in <img src="3-7500406\2078deac-920d-459d-8747-9585d8d2549b.jpg" /> we obtain:</p><disp-formula id="scirp.6677-formula84888"><label>(14)</label><graphic position="anchor" xlink:href="3-7500406\8ef69de0-63c3-4a71-9f23-79e23457bf4e.jpg"  xlink:type="simple"/></disp-formula><p>which will be non-zero for</p><disp-formula id="scirp.6677-formula84889"><label>(15a)</label><graphic position="anchor" xlink:href="3-7500406\3e1cc44f-15ec-4aa0-9e21-81b5b3e03193.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.6677-formula84890"><label>(15b)</label><graphic position="anchor" xlink:href="3-7500406\be9a3e21-b2ab-44e4-b38e-5864cb2af144.jpg"  xlink:type="simple"/></disp-formula><p>Similarly substitution of Equations (5a) and (5b) in <img src="3-7500406\bcdd743c-9e14-409b-baee-633e9d73f907.jpg" /> we obtain:</p><p><img src="3-7500406\c38e9303-b8c9-4fee-9407-c53bea3318e1.jpg" />(16)</p><p>which will be non-zero for</p><p><img src="3-7500406\c3fdbc01-ff88-491e-bea1-e8ae6c72e107.jpg" /><img src="3-7500406\8576b75a-6a8b-4782-9b09-3a2483c71eef.jpg" /> (17)</p><p>Next we consider the case (b):</p><p><img src="3-7500406\b04f605c-2d98-4a1c-a7b6-5c380eea4848.jpg" /></p><p><img src="3-7500406\b8ff2200-4701-428b-b901-ee2538267899.jpg" /><img src="3-7500406\96c2bc89-9dae-4713-89ea-3c2c5cc61a39.jpg" /></p><p>+<img src="3-7500406\c8ce0849-697c-4974-8512-f2960fca45e2.jpg" /><img src="3-7500406\96392d9d-9063-44fa-9672-a2f98c3fdc59.jpg" /></p><disp-formula id="scirp.6677-formula84891"><label>(18)</label><graphic position="anchor" xlink:href="3-7500406\2170081d-09d0-4a14-b14a-2686d17aa415.jpg"  xlink:type="simple"/></disp-formula><p>Substitution of Equation (5a) in <img src="3-7500406\dc7a7ef6-d411-4b19-bd7c-2d172957cf91.jpg" /> we obtain:</p><disp-formula id="scirp.6677-formula84892"><label>(19)</label><graphic position="anchor" xlink:href="3-7500406\5a46e4af-476d-4970-a6c6-734c46117fb8.jpg"  xlink:type="simple"/></disp-formula><p>which will be non-zero for</p><disp-formula id="scirp.6677-formula84893"><label>(20)</label><graphic position="anchor" xlink:href="3-7500406\0a1ce31c-2afd-4dde-8f36-1253b9f09d11.jpg"  xlink:type="simple"/></disp-formula><p>where we used the relations:</p><disp-formula id="scirp.6677-formula84894"><label>(21)</label><graphic position="anchor" xlink:href="3-7500406\0c1b2c0e-4b67-49f3-90bf-360769c83e75.jpg"  xlink:type="simple"/></disp-formula><p>Similarly substitution of Equation (5b) in <img src="3-7500406\59e3ad9f-586e-46f9-aa64-bd4f85a75ed7.jpg" /> we obtain:</p><disp-formula id="scirp.6677-formula84895"><label>(22)</label><graphic position="anchor" xlink:href="3-7500406\de165309-5209-4ea3-99fa-777d60c95626.jpg"  xlink:type="simple"/></disp-formula><p>which will be non-zero for</p><disp-formula id="scirp.6677-formula84896"><label>(23)</label><graphic position="anchor" xlink:href="3-7500406\0b7af0ae-275a-4290-87cf-e1d1602280e9.jpg"  xlink:type="simple"/></disp-formula><p>Substitution of Equations (5a) and (5b) in <img src="3-7500406\948e8d0e-87bd-47df-8361-b982eb93b472.jpg" /> we obtain:</p><disp-formula id="scirp.6677-formula84897"><label>(24)</label><graphic position="anchor" xlink:href="3-7500406\d661c63d-bf0d-44c7-8105-f07b22e92ac4.jpg"  xlink:type="simple"/></disp-formula><p>which will be non-zero for</p><disp-formula id="scirp.6677-formula84898"><label>(25)</label><graphic position="anchor" xlink:href="3-7500406\84e170c7-ea21-43e8-8a9a-7ddb6e84ef20.jpg"  xlink:type="simple"/></disp-formula><p>Similarly substitution of Equations (5a) and (5b) in <img src="3-7500406\e9d90c2f-10ea-40a4-95ad-b06a3a59bd96.jpg" /> we obtain:</p><disp-formula id="scirp.6677-formula84899"><label>(26)</label><graphic position="anchor" xlink:href="3-7500406\6e06e2c9-1659-4d7b-86d4-bf10d0bf23dd.jpg"  xlink:type="simple"/></disp-formula><p>which will be non-zero for&#160;</p><disp-formula id="scirp.6677-formula84900"><label>. (27)</label><graphic position="anchor" xlink:href="3-7500406\aeae169f-c85c-4dc0-995b-63661a07416a.jpg"  xlink:type="simple"/></disp-formula><p>So far we have considered the effect of the electric dipole transitions. If we want to add the effect of the magnetic field, we must take <img src="3-7500406\e66f5dba-e93e-4e76-95f8-7f6e14484729.jpg" /> as the perturbing potential. To calculate the matrix element&#160; <img src="3-7500406\3a42bc91-ad41-410e-a2b7-e73df24de073.jpg" /> , we will follow a similar way as we did above. Namely we will consider two different cases: a) The polarization of the magnetic field is in x-y plane (along the xor the y-axis) b) The polarization of the magnetic field is in z-direction. The only difference is that the magnetic moment vector <img src="3-7500406\a463904c-0829-4d4e-8a34-e9fa5b188665.jpg" /> will be proportional to (<img src="3-7500406\5f38528c-18df-4ac6-9dfb-d0b8a3825237.jpg" />), so <img src="3-7500406\64cf564d-2c85-4df9-a2c8-41a489c50b17.jpg" /> will be perpendicular to the vector<img src="3-7500406\587a1e78-02ae-4d2b-8adf-9d99f33ca6c4.jpg" />. Therefore for the case a) we calculate the matrix elements of the quantity rcos q&#160; and for the case b) we calculate the matrix elements of the quantity x &#177; iy= rsinq exp(&#177;if ). That means for the case a) we will calculate the matrix elements <img src="3-7500406\b18e452d-001b-489e-a213-e619576b6c0e.jpg" /> given in Equation (18) and for the case b) we will calculate the matrix elements <img src="3-7500406\b3516f48-7dca-45f5-a9bb-bd21995d901e.jpg" /> given in Equation (8). Therefore the selection rules of the magnetic dipole transitions will be the same as the selection rules for the electric dipole transitions. Combining the results of the Equations (10), (13), (15), (17), (20), (23), (25) and (27), we write the selection rules for a photonic transitions in Hydrogen-like atoms:</p><p><img src="3-7500406\ed909eb0-ad14-45b2-af2c-cb20c6549bdf.jpg" /><img src="3-7500406\405948b8-fa10-4738-9fa2-e4cc7cf91f00.jpg" /> (28)</p></sec><sec id="s4"><title>4. Application of the Spin Dependent</title><p>Selection Rules to (<img src="3-7500406\af56bbe8-eb65-480c-bd44-23afbc77f32a.jpg" />) Transition in Cs According to the conventional selection rules (<img src="3-7500406\3be936f0-56a6-4dee-9ffa-f99ad3459851.jpg" />and<img src="3-7500406\54dbd8e5-6365-472c-bdc9-a502184fd01d.jpg" />) which are derived from the Schr&#246;dinger equation in the same way as in Section 3, a transition such as <img src="3-7500406\8a5a8647-0d07-4806-b56b-fb4478219a4f.jpg" /> is not allowed ( because this is a transition (<img src="3-7500406\6806d49f-fa90-4905-92ac-757129de9042.jpg" /><img src="3-7500406\f230c754-18f9-4f1d-b56b-e88a926a8179.jpg" /><img src="3-7500406\e8cb36f4-e7cc-4614-9fe8-3e01d55e634f.jpg" />) in which<img src="3-7500406\ecfbc18f-d87d-40f9-ba93-71125b3cb73f.jpg" />, so it does not meet the condition<img src="3-7500406\8d2d9b32-e8d7-45f7-9b2f-08c68fec5f27.jpg" />). But <img src="3-7500406\3e70f6ba-8f4b-4fef-b318-26d88292d7bd.jpg" /> transition in Cs atom has been already observed [7-9]. However, the present spin dependent selection rules allow the transition: <img src="3-7500406\dfff1218-8b49-4268-a879-8ded76d20b28.jpg" /><img src="3-7500406\e3b89fbd-b46b-4816-bf3d-ca099f2bad33.jpg" /><img src="3-7500406\9c4ceac7-e4d5-49dc-b1ee-2722197cd783.jpg" />in Cs atom. Because here we have<img src="3-7500406\07bf2a8c-ec91-4e50-9e97-dadda21f0e72.jpg" /> and <img src="3-7500406\4b160acb-baa0-493b-a67c-5a1789d03706.jpg" /> which are allowed by the present spin dependent selection rules given in Equation (28). To prove the above transition in detail, let us assume that the outer electron of the Cs atom is initially at the state <img src="3-7500406\8760aa9b-1e3d-49e0-b995-4cb54e6002a9.jpg" />=<img src="3-7500406\e98d3730-0b65-4746-91cf-8b5d8ea205bb.jpg" />. From Equation (5a) we write:</p><disp-formula id="scirp.6677-formula84901"><label>(29)</label><graphic position="anchor" xlink:href="3-7500406\8f5f3067-1a0e-4012-9ece-acc20bb5abd4.jpg"  xlink:type="simple"/></disp-formula><p>where A is the normalization constant. When it is excited to the <img src="3-7500406\412913cd-456b-4f43-b768-0159f6adbf20.jpg" />state, the possible final states are:</p><p><img src="3-7500406\39b0c678-edef-4365-abfb-f688f265e7c7.jpg" />and<img src="3-7500406\7a4e8b6a-e6e2-4c73-9b7f-d2de61ddb81c.jpg" />.</p><p>From Equations (5a) and (5b) these states are:</p><disp-formula id="scirp.6677-formula84902"><label>(30a)</label><graphic position="anchor" xlink:href="3-7500406\d8a31c96-ef3d-459d-a797-52cbe573f6f2.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.6677-formula84903"><label>(30b)</label><graphic position="anchor" xlink:href="3-7500406\79ab0d19-215a-4c32-8b6e-6036cdbc6ebb.jpg"  xlink:type="simple"/></disp-formula><p>where B, and C are the normalization constants. Substituting the wave functions from Equation (29) and Equations (30a)-(30b) in Equations (8) and (18) we find:</p><disp-formula id="scirp.6677-formula84904"><label>(31)</label><graphic position="anchor" xlink:href="3-7500406\1ca6f6b0-83b0-4324-a87c-472df9fd87af.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.6677-formula84905"><label>(32)</label><graphic position="anchor" xlink:href="3-7500406\6b7f9552-5ce9-4c76-a1ee-fb77694fa891.jpg"  xlink:type="simple"/></disp-formula><p>Therefore the non-zero matrix element in Equation (31) gives us a non-transition between the states <img src="3-7500406\bd418259-18e2-4bfe-84ac-abe2ab851c16.jpg" /> and <img src="3-7500406\210b3bda-c934-4531-bfc6-5b5d15ca9519.jpg" /> which is&#160; also allowed by the present spin dependent selection rules given in Equation (28) (<img src="3-7500406\b99984be-9fde-4e66-addb-d421fe276a95.jpg" />and<img src="3-7500406\d1db6fd8-5aae-42a5-befc-b5de8a187596.jpg" />).</p></sec><sec id="s5"><title>5. Conclusions</title><p>We have derived the spin dependent selection rules for photonic transitions in hydrogen-like atoms by using the solution of Dirac equation for hydrogen-like atoms. It is shown that photonic transitions occur when [<img src="3-7500406\42af2753-b41e-41ef-b97d-e6cfbad48336.jpg" />while<img src="3-7500406\d3d635b7-338c-4b3c-8b0f-23e858b437a3.jpg" />]. By applying the present spin dependent selection rules we can explain the observed (6 s<img src="3-7500406\2c64749f-6c34-41f8-b85c-8a7174098cdb.jpg" />7 s) transition in Cesium (Cs) atom [7,8]. Because in the (6s<img src="3-7500406\24c5aebb-e617-4a35-af31-94043ea48333.jpg" />7s) transition in Cesium (Cs) atom we have [<img src="3-7500406\5be9f033-745a-4842-b0d8-b4a465ff9a18.jpg" />while<img src="3-7500406\d6535482-fe13-415a-af3b-7029592491a8.jpg" />] which is an allowed transition according to the present selection rules given in Equation (28). The present result is believed to be helpful for a deeper understanding of the photonic transitions and the spectrum of Cs atom [<xref ref-type="bibr" rid="scirp.6677-ref1">1</xref>]. A detailed study will be presented in the future.</p></sec><sec id="s6"><title>REFERENCES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.6677-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">S. B. Bayram, S. Kin, M. J. Welsh and J. D. Hinkle, “Collisional Depolarization of Zeeman Coherences in the 133Cs 6p 2P3/2 Level: Double-resonance Two-photon Polarization Spectroscopy,” Physical Review A (Atomic, Molecular and Optical Physics), Vol. 73, No. 4, April 2006, pp. 42713-1-6. doi:10.1007/s10946-007-0015-6</mixed-citation></ref><ref id="scirp.6677-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">M. Saglam, Z. Saglam, B. Boyacioglu and K. K. 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