<?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.2014.512106</article-id><article-id pub-id-type="publisher-id">JMP-47739</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>Perturbation of Hydrogen Degenerate Levels and SO(4)</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Enrico</surname><given-names>Onofri</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>1Dipartimento di Fisica e Scienze della Terra, Università di Parma, Parma, Italy
2INFN, Gruppo Collegato di Parma, Parma, Italy</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>enrico.onofri@unipr.it</email></corresp></author-notes><pub-date pub-type="epub"><day>11</day><month>07</month><year>2014</year></pub-date><volume>05</volume><issue>12</issue><fpage>1051</fpage><lpage>1054</lpage><history><date date-type="received"><day>22</day>	<month>February</month>	<year>2014</year></date><date date-type="rev-recd"><day>21</day>	<month>March</month>	<year>2014</year>	</date><date date-type="accepted"><day>14</day>	<month>April</month>	<year>2014</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>
	We
present a short note about the perturbative correction to Rydberg energies
under a perturbation cosθ/r<sup>μ</sup> and discuss the role of SO(4) symmetry.
</p></abstract><kwd-group><kwd>Rydberg States</kwd><kwd> &lt;i&gt;SO&lt;/i&gt;(4) Symmetry</kwd><kwd> Runge-Lenz-Pauli Vector</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>The subject of this short note stems from a classroom exercise. I proposed my students to evaluate the effect on the degenerate levels of the hydrogen atom of a perturbation with potential energy<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\117747da-5f4b-462f-b859-515ec8edde6e.png" xlink:type="simple"/></inline-formula>. At the first order in perturbation theory this problem requires the diagonalization of the matrix representing the perturbation restricted to the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\48d8b1e0-1591-4d3e-8518-dcf730502111.png" xlink:type="simple"/></inline-formula> degenerate subspace (see Appendix A).</p><disp-formula id="scirp.47739-formula1923"><label>(1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\2f6f3b47-7868-4112-973b-59f84955b832.png"/></disp-formula><p>The problem in itself appears to involve a rather standard (and boring) calculation based on the properties of Laguerre and Legendre functions. To save time one can attack the problem using a computer algebra system, like Mathematica<sup>1</sup> and the matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\4d36f285-ff80-43bd-8dc9-3c1dc2da55e6.png" xlink:type="simple"/></inline-formula> can be readily constructed; if we are lucky enough, its spectrum could be exhibited in closed form or at least in numerical terms. Now, the surprise is that the eigenvalues turn out to be all simple rationals of the form <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\187e6dff-e5a9-4a2c-99ea-14fff107ea86.png" xlink:type="simple"/></inline-formula> where m runs from <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\ccf4e92f-f342-46e7-998d-a800ec05a674.png" xlink:type="simple"/></inline-formula> to <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\b919e1ca-0da4-4e05-9019-c9e3dd8368d0.png" xlink:type="simple"/></inline-formula> and they are <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\483b96b2-b0f5-4c3a-a40e-3f9a92747cab.png" xlink:type="simple"/></inline-formula> degenerate. The result is so simple that one cannot be satisfied by the brute-force calculation, and he or she is forced to look for some explanation. Obviously the first idea that comes to mind is that this result should rely on some Lie-algebraic property. In the following I’m going to explain how hydrogen’s <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\e4f696d0-116f-4c51-8c40-1bd1cb131cae.png" xlink:type="simple"/></inline-formula> symmetry accounts for the result.</p></sec><sec id="s2"><title>2. Dipole Operators and the SO(4) Generators</title><p>The origin of the Lie-theoretic explanation lies in one of the first papers about quantum mechanics [<xref ref-type="bibr" rid="scirp.47739-ref1">1</xref>] . In the book by Gottfried and Yan [<xref ref-type="bibr" rid="scirp.47739-ref2">2</xref>] <sup>2</sup> one can find all details in a masterly presentation. In this note, however, we present a somewhat simpler derivation, suitable for an introductory Quantum Mechanics course. In particular we give a simple derivation of Pauli’s link between <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\6f11557c-1d7f-4b72-8453-799a0eaae0a8.png" xlink:type="simple"/></inline-formula> Casimir operator and the Hamiltonian, which cannot be found in most textbooks (see Appendix B). Other relevant information is contained in the recent paper [<xref ref-type="bibr" rid="scirp.47739-ref3">3</xref>] with generalization to higher multipoles.</p><p>The fact is: hydrogen atom, in its simplest terms, described by the Hamiltonian<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\cdaffea3-d2f1-4690-9dea-73e381d44511.png" xlink:type="simple"/></inline-formula>, exhibits a larger</p><p>degeneracy than required by rotational invariance, the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\a2f42a59-d8ba-43e1-951e-6039fb08ef95.png" xlink:type="simple"/></inline-formula> level being <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\393b6df0-fa0d-4c77-871b-5b2dbff7f309.png" xlink:type="simple"/></inline-formula> degenerate. This fact was related, since Pauli’s paper, to the presence of an extra conserved vector quantity, which in classical mechanics is known as the Laplace-Runge-Lenz vector and was used by Pauli in the calculation of the spectrum. This should be considered as the first example of dynamical symmetry in Quantum Mechanics. The quantum conserved vector is</p><disp-formula id="scirp.47739-formula1924"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\7316a5c9-b7db-4e93-bd58-e9fbe0cebbdc.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\2d6d98b0-d59d-41e0-9f54-97c4d5d8fcf6.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\15739cf2-37e5-476d-af60-c1c96ab809f1.png" xlink:type="simple"/></inline-formula>. Since <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\8acabc37-2db5-4ac8-8d66-46fb648420c6.png" xlink:type="simple"/></inline-formula> commutes with the Hamiltonian it can be normalized by adding a</p><p>factor <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\2ac4ba25-9501-4c44-b77b-a1b7a5333572.png" xlink:type="simple"/></inline-formula> in such a way that <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\a94e4af9-67af-4a30-823f-1012a462f3a3.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\dcadd0a7-d135-4997-972b-eca3f4d04e0e.png" xlink:type="simple"/></inline-formula> close the Lie algebra of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\8ec97a18-03fd-4540-82c2-03deccb7a8d2.png" xlink:type="simple"/></inline-formula> under commutation. In his 1926 paper Pauli showed that this fact was sufficient to derive Balmer’s formula and the “dipole matrix elements” <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\d7e3cd35-f9f9-42e5-8529-e7811d597f78.png" xlink:type="simple"/></inline-formula>in terms of the matrix of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\daf9a389-db5c-4c67-9a6b-d66aaab39fd2.png" xlink:type="simple"/></inline-formula> in the same <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\bcab940f-99b0-4982-92cf-d5c42de2965f.png" xlink:type="simple"/></inline-formula> degene-</p><p>rate subspace. Denoting by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\5f6d7172-7fd1-4772-b195-827f76b01045.png" xlink:type="simple"/></inline-formula> the orthogonal projector on the <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\adb67af7-2804-468c-b422-9760594353f1.png" xlink:type="simple"/></inline-formula> degenerate subspace, it is immediately</p><p>realized that<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\1dd15bba-ba34-41d6-ba14-4f9c5fd7c367.png" xlink:type="simple"/></inline-formula>; no contributions arise from the term <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\9aefcb46-ffab-4dc9-a004-23743a90a617.png" xlink:type="simple"/></inline-formula> which has va-</p><p>nishing matrix elements between degenerate states since it coincides with the commutator<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\a0b9eab8-2722-4c4a-9c35-9175cfb4da32.png" xlink:type="simple"/></inline-formula>. Now, since N belongs to the Lie algebra of the symmetry group<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\7d2a72c0-bb54-496b-bd2c-0861185bf65a.png" xlink:type="simple"/></inline-formula>, its spectrum is fixed by group theory alone. Simply enough, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\afed0910-4de5-4f90-b772-39d901e28526.png" xlink:type="simple"/></inline-formula>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\f58c7b4a-913d-45d8-adb2-e8ec9d69ef34.png" xlink:type="simple"/></inline-formula> are the generators of the two <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\764287c2-09b4-4433-82d2-ca636d284777.png" xlink:type="simple"/></inline-formula> factors of<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\d33fcd46-6f02-4ef8-a60f-771db27a3980.png" xlink:type="simple"/></inline-formula>. Since <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\70c39c3d-6ccb-4021-9918-a13af48159fd.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\168c772d-b2a9-4124-a703-4d1c5a34c902.png" xlink:type="simple"/></inline-formula> commute, and the total angular momentum is <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\6df18aa0-6a51-4fbd-a960-baaaffea329f.png" xlink:type="simple"/></inline-formula> for each of them, the spectrum is simply given by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\12f14d33-1fef-41fa-95c9-ea95e11fbde4.png" xlink:type="simple"/></inline-formula> that is <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\76203425-6e3a-4141-897b-29630bc1a925.png" xlink:type="simple"/></inline-formula> with degeneracy<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\978a409b-c3c3-452b-b123-82905f0910ca.png" xlink:type="simple"/></inline-formula>. As a result the spectrum of the matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\c9998c63-5676-4373-8675-1b539aa82c15.png" xlink:type="simple"/></inline-formula> is precisely given, as anticipated, by</p><disp-formula id="scirp.47739-formula1925"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\58372103-c31b-41d8-864e-20067c749e2c.png"/></disp-formula><p>For the sake of completeness we recall the detailed expression for the eigenfunctions and the matrix elements in appendix.</p></sec><sec id="s3"><title>3. Conclusion</title><p>It is clear that the use of a symbolic algebra system can easily give the spectrum of the dipole x or, more generally,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\3266c047-1eaf-4c3f-a29e-8c6d937e5790.png" xlink:type="simple"/></inline-formula>. For instance one can check immediately that the matrix identically vanishes for<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\1-7501630x\5f2da00a-a1a7-461c-9f06-c4f519d09330.png" xlink:type="simple"/></inline-formula>, the case of the electric dipole perturbation. However the connection with group theory gives a deeper insight into the result, which by itself could remain a simple mathematical curiosity. Let us notice that in the classical book [<xref ref-type="bibr" rid="scirp.47739-ref4">4</xref>] by Condon and Shortley the calculations of the Stark effect perturbative corrections to the Balmer energies are beautifully obtained using parabolic coordinates, but the result of Equation (3) takes on a new light when interpreted group-theoretically.</p></sec><sec id="s4"><title>Acknowledgements</title><p>This paper has a mere didactic interest and it is related to my thesis of 1968. It is my pleasure to thank Prof. Massimo Pauri, then my advisor and today Professor Emeritus at our Department, who taught me quite a lot about symmetry and group theory in Quantum Mechanics.</p></sec></body><back><ref-list><title>References</title><ref id="scirp.47739-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">PAULI, W. (1926) ZEITSCHRIFT FUR PHYSIK, 36, 336-363. HTTP://DX.DOI.ORG/10.1007/BF01450175</mixed-citation></ref><ref id="scirp.47739-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">GOTTFRIED, K. AND YAN, T.-M. (2004) QUANTUM MECHANICS, FUNDAMENTALS. 2ND EDITION, SPRINGER, NEW YORK.</mixed-citation></ref><ref id="scirp.47739-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">OSTROVSKY, V.N., VRINCEANU, D. AND FLANNERY, M.R. (2006) PHYSICAL REVIEW A, 74, ARTICLE ID: 022720.</mixed-citation></ref><ref id="scirp.47739-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">CONDON, E.U. AND SHORTLEY, G.H. (1964) THE THEORY OF ATOMIC SPECTRA. CAMBRIDGE UNIVERSITY PRESS, CAMBRIDGE.</mixed-citation></ref></ref-list></back></article>