{"title":"Mass-Energy Compensation Effect of 3\\(\\alpha\\) Hamiltonian","authors":"I. Filikhin, C. Martin, A. Karoui, B. Vlahovic","doi":"10.1134/S1063778824700911","DOIUrl":null,"url":null,"abstract":"<p>The <span>\\(3\\alpha\\)</span> phenomenological model describes the structure of the carbon-12 nucleus as a cluster of three alpha particles. This model includes a pairwise <span>\\(\\alpha{-}\\alpha\\)</span> interaction and a three-body force. To fit the three-body potential, the <span>\\({}^{12}\\)</span>C data are used, while ensuring that the pair potential reproduces the <span>\\(\\alpha{-}\\alpha\\)</span> scattering data. Alternatively, the mass–energy compensation (MEC) effect can be used to simulate the effect of the three-body potential by adjusting the mass of the <span>\\(\\alpha\\)</span> particle within the effective-mass approach. We demonstrate the MEC effect for the <span>\\(3\\alpha\\)</span> ground state by numerically solving the differential Faddeev equation, in which the <span>\\(\\alpha{-}\\alpha\\)</span> interaction is described by the Ali–Bodmer potential. The effective masses of <span>\\(\\alpha\\)</span> particles are evaluated for the ground and excited <span>\\(0^{+}\\)</span> and bound <span>\\(2^{+}\\)</span> states. We demonstrate a coupling between the ground and first excited <span>\\(0^{+}\\)</span> states, indicated by an anti-crossing of these energy levels in the energy–mass coordinates. A correspondence between the effective mass and a three-body potential is demonstrated. We discuss the results of the <span>\\(0^{+}_{2}\\)</span> calculations for various models of the <span>\\(\\alpha{-}\\alpha\\)</span> interaction.</p>","PeriodicalId":728,"journal":{"name":"Physics of Atomic Nuclei","volume":"87 2 supplement","pages":"S274 - S283"},"PeriodicalIF":0.3000,"publicationDate":"2025-03-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics of Atomic Nuclei","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S1063778824700911","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"PHYSICS, NUCLEAR","Score":null,"Total":0}
引用次数: 0
Abstract
The \(3\alpha\) phenomenological model describes the structure of the carbon-12 nucleus as a cluster of three alpha particles. This model includes a pairwise \(\alpha{-}\alpha\) interaction and a three-body force. To fit the three-body potential, the \({}^{12}\)C data are used, while ensuring that the pair potential reproduces the \(\alpha{-}\alpha\) scattering data. Alternatively, the mass–energy compensation (MEC) effect can be used to simulate the effect of the three-body potential by adjusting the mass of the \(\alpha\) particle within the effective-mass approach. We demonstrate the MEC effect for the \(3\alpha\) ground state by numerically solving the differential Faddeev equation, in which the \(\alpha{-}\alpha\) interaction is described by the Ali–Bodmer potential. The effective masses of \(\alpha\) particles are evaluated for the ground and excited \(0^{+}\) and bound \(2^{+}\) states. We demonstrate a coupling between the ground and first excited \(0^{+}\) states, indicated by an anti-crossing of these energy levels in the energy–mass coordinates. A correspondence between the effective mass and a three-body potential is demonstrated. We discuss the results of the \(0^{+}_{2}\) calculations for various models of the \(\alpha{-}\alpha\) interaction.
期刊介绍:
Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.