{"title":"Metamorphosis of Positronium Moving Across a Magnetic Field","authors":"B. O. Kerbikov, A. A. Simovonian","doi":"arxiv-2409.09496","DOIUrl":null,"url":null,"abstract":"Positronium spectrum and lifetimes are known with a high precision. The\nsituation is different for positronium moving across a magnetic field. The\ntotal momentum does not commute with the Hamiltonian and is replaced by\nconserved pseudomomentum. The internal dynamics is not separated from the\nmotion of the system as a whole. The Coulomb potential well is distorted and a\nwide outer potential well is created. We analytically determine the energy\nspectrum for a broad range of the magnetic field and pseudomomentum values. We\nlocate the region of these parameters for which the ground state resides in the\nouter well. The results may play a role in the supression of pulsars radio\nemission (polar cap problem).","PeriodicalId":501343,"journal":{"name":"arXiv - PHYS - High Energy Astrophysical Phenomena","volume":"40 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - High Energy Astrophysical Phenomena","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.09496","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Positronium spectrum and lifetimes are known with a high precision. The
situation is different for positronium moving across a magnetic field. The
total momentum does not commute with the Hamiltonian and is replaced by
conserved pseudomomentum. The internal dynamics is not separated from the
motion of the system as a whole. The Coulomb potential well is distorted and a
wide outer potential well is created. We analytically determine the energy
spectrum for a broad range of the magnetic field and pseudomomentum values. We
locate the region of these parameters for which the ground state resides in the
outer well. The results may play a role in the supression of pulsars radio
emission (polar cap problem).