{"title":"考虑微扰方法的海尔曼哈密顿量的李代数逼近","authors":"H. Rahmati","doi":"10.1134/S0040577924120092","DOIUrl":null,"url":null,"abstract":"<p> We show that the Lie algebraic approach with the perturbation method can be used to study the eigenvalues of the Hellmann Hamiltonian. The key element is the Runge–Lenz vector, which appears in problems with radial symmetry. This symmetry implies that the proper lie algebra for these Hamiltonians is <span>\\(so(4)\\)</span>, which is a sum of two <span>\\(so(3)\\)</span> Lie algebras and requires symmetry of the angular momentum vector <span>\\(\\vec{L}\\)</span> and the Runge–Lenz vector <span>\\(\\vec{M}\\)</span>, and therefore their cross products as <span>\\(\\vec{W}=\\vec{L}\\times\\vec{M}\\)</span>. Here, Yukawa potential is considered as a perturbation term, which is added to the Coulomb Hamiltonian to produce the Hellmann Hamiltonian. Lie algebraically, the perturbation term adds a magnitude of precession rate <span>\\(\\Omega\\)</span> to all three operators <span>\\(\\vec{L}\\)</span>, <span>\\(\\vec{M}\\)</span>, and <span>\\(\\vec{W}\\)</span>. Topologically, we show that the appearance of this precession has a significant effect on the spectrum and the corresponding Lie algebra of the Hellmann potential. By using Lie algebraic properties of the Runge–Lenz vector and using the Kolmogorov method, we obtain the energy spectrum of this Hamiltonian. </p>","PeriodicalId":797,"journal":{"name":"Theoretical and Mathematical Physics","volume":"221 3","pages":"2144 - 2154"},"PeriodicalIF":1.0000,"publicationDate":"2024-12-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Lie algebraic approach to the Hellmann Hamiltonian by considering perturbation method\",\"authors\":\"H. Rahmati\",\"doi\":\"10.1134/S0040577924120092\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p> We show that the Lie algebraic approach with the perturbation method can be used to study the eigenvalues of the Hellmann Hamiltonian. The key element is the Runge–Lenz vector, which appears in problems with radial symmetry. This symmetry implies that the proper lie algebra for these Hamiltonians is <span>\\\\(so(4)\\\\)</span>, which is a sum of two <span>\\\\(so(3)\\\\)</span> Lie algebras and requires symmetry of the angular momentum vector <span>\\\\(\\\\vec{L}\\\\)</span> and the Runge–Lenz vector <span>\\\\(\\\\vec{M}\\\\)</span>, and therefore their cross products as <span>\\\\(\\\\vec{W}=\\\\vec{L}\\\\times\\\\vec{M}\\\\)</span>. Here, Yukawa potential is considered as a perturbation term, which is added to the Coulomb Hamiltonian to produce the Hellmann Hamiltonian. Lie algebraically, the perturbation term adds a magnitude of precession rate <span>\\\\(\\\\Omega\\\\)</span> to all three operators <span>\\\\(\\\\vec{L}\\\\)</span>, <span>\\\\(\\\\vec{M}\\\\)</span>, and <span>\\\\(\\\\vec{W}\\\\)</span>. Topologically, we show that the appearance of this precession has a significant effect on the spectrum and the corresponding Lie algebra of the Hellmann potential. By using Lie algebraic properties of the Runge–Lenz vector and using the Kolmogorov method, we obtain the energy spectrum of this Hamiltonian. </p>\",\"PeriodicalId\":797,\"journal\":{\"name\":\"Theoretical and Mathematical Physics\",\"volume\":\"221 3\",\"pages\":\"2144 - 2154\"},\"PeriodicalIF\":1.0000,\"publicationDate\":\"2024-12-25\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Theoretical and Mathematical Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1134/S0040577924120092\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"PHYSICS, MATHEMATICAL\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Theoretical and Mathematical Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S0040577924120092","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, MATHEMATICAL","Score":null,"Total":0}
Lie algebraic approach to the Hellmann Hamiltonian by considering perturbation method
We show that the Lie algebraic approach with the perturbation method can be used to study the eigenvalues of the Hellmann Hamiltonian. The key element is the Runge–Lenz vector, which appears in problems with radial symmetry. This symmetry implies that the proper lie algebra for these Hamiltonians is \(so(4)\), which is a sum of two \(so(3)\) Lie algebras and requires symmetry of the angular momentum vector \(\vec{L}\) and the Runge–Lenz vector \(\vec{M}\), and therefore their cross products as \(\vec{W}=\vec{L}\times\vec{M}\). Here, Yukawa potential is considered as a perturbation term, which is added to the Coulomb Hamiltonian to produce the Hellmann Hamiltonian. Lie algebraically, the perturbation term adds a magnitude of precession rate \(\Omega\) to all three operators \(\vec{L}\), \(\vec{M}\), and \(\vec{W}\). Topologically, we show that the appearance of this precession has a significant effect on the spectrum and the corresponding Lie algebra of the Hellmann potential. By using Lie algebraic properties of the Runge–Lenz vector and using the Kolmogorov method, we obtain the energy spectrum of this Hamiltonian.
期刊介绍:
Theoretical and Mathematical Physics covers quantum field theory and theory of elementary particles, fundamental problems of nuclear physics, many-body problems and statistical physics, nonrelativistic quantum mechanics, and basic problems of gravitation theory. Articles report on current developments in theoretical physics as well as related mathematical problems.
Theoretical and Mathematical Physics is published in collaboration with the Steklov Mathematical Institute of the Russian Academy of Sciences.