Relativistic Ermakov–Milne–Pinney Systems and First Integrals

Detalhes bibliográficos
Autor(a) principal: Haas, Fernando
Data de Publicação: 2021
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UFRGS
Texto Completo: http://hdl.handle.net/10183/219606
Resumo: The Ermakov–Milne–Pinney equation is ubiquitous in many areas of physics that have an explicit time-dependence, including quantum systems with time-dependent Hamiltonian, cosmology, time-dependent harmonic oscillators, accelerator dynamics, etc. The Eliezer and Gray physical interpretation of the Ermakov–Lewis invariant is applied as a guiding principle for the derivation of the special relativistic analog of the Ermakov–Milne–Pinney equation and associated first integral. The special relativistic extension of the Ray–Reid system and invariant is obtained. General properties of the relativistic Ermakov–Milne–Pinney are analyzed. The conservative case of the relativistic Ermakov–Milne–Pinney equation is described in terms of a pseudo-potential, reducing the problem to an effective Newtonian form. The non-relativistic limit is considered to be well. A relativistic nonlinear superposition law for relativistic Ermakov systems is identified. The generalized Ermakov–Milne–Pinney equation has additional nonlinearities, due to the relativistic effects.
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spelling Haas, Fernando2021-04-08T04:17:32Z20212624-8174http://hdl.handle.net/10183/219606001123312The Ermakov–Milne–Pinney equation is ubiquitous in many areas of physics that have an explicit time-dependence, including quantum systems with time-dependent Hamiltonian, cosmology, time-dependent harmonic oscillators, accelerator dynamics, etc. The Eliezer and Gray physical interpretation of the Ermakov–Lewis invariant is applied as a guiding principle for the derivation of the special relativistic analog of the Ermakov–Milne–Pinney equation and associated first integral. The special relativistic extension of the Ray–Reid system and invariant is obtained. General properties of the relativistic Ermakov–Milne–Pinney are analyzed. The conservative case of the relativistic Ermakov–Milne–Pinney equation is described in terms of a pseudo-potential, reducing the problem to an effective Newtonian form. The non-relativistic limit is considered to be well. A relativistic nonlinear superposition law for relativistic Ermakov systems is identified. The generalized Ermakov–Milne–Pinney equation has additional nonlinearities, due to the relativistic effects.application/pdfengPhysics. Basel. Vol. 3, no. 1 (Mar.2021), p. 59-70Equação de PinneyRelatividadeSistemas quanticosErmakov systemErmakov–Milne–Pinney equationRelativistic Ermakov–Lewis invariantRelativistic Ray–Reid systemNonlinear superposition lawRelativistic Ermakov–Milne–Pinney Systems and First IntegralsEstrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT001123312.pdf.txt001123312.pdf.txtExtracted Texttext/plain35436http://www.lume.ufrgs.br/bitstream/10183/219606/2/001123312.pdf.txteca01034b7e0baec21ecdaad0fe26c21MD52ORIGINAL001123312.pdfTexto completo (inglês)application/pdf314417http://www.lume.ufrgs.br/bitstream/10183/219606/1/001123312.pdf5c14dbe74edbadd67be6cabb4fd29e12MD5110183/2196062023-07-20 03:36:22.309803oai:www.lume.ufrgs.br:10183/219606Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-20T06:36:22Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false
dc.title.pt_BR.fl_str_mv Relativistic Ermakov–Milne–Pinney Systems and First Integrals
title Relativistic Ermakov–Milne–Pinney Systems and First Integrals
spellingShingle Relativistic Ermakov–Milne–Pinney Systems and First Integrals
Haas, Fernando
Equação de Pinney
Relatividade
Sistemas quanticos
Ermakov system
Ermakov–Milne–Pinney equation
Relativistic Ermakov–Lewis invariant
Relativistic Ray–Reid system
Nonlinear superposition law
title_short Relativistic Ermakov–Milne–Pinney Systems and First Integrals
title_full Relativistic Ermakov–Milne–Pinney Systems and First Integrals
title_fullStr Relativistic Ermakov–Milne–Pinney Systems and First Integrals
title_full_unstemmed Relativistic Ermakov–Milne–Pinney Systems and First Integrals
title_sort Relativistic Ermakov–Milne–Pinney Systems and First Integrals
author Haas, Fernando
author_facet Haas, Fernando
author_role author
dc.contributor.author.fl_str_mv Haas, Fernando
dc.subject.por.fl_str_mv Equação de Pinney
Relatividade
Sistemas quanticos
topic Equação de Pinney
Relatividade
Sistemas quanticos
Ermakov system
Ermakov–Milne–Pinney equation
Relativistic Ermakov–Lewis invariant
Relativistic Ray–Reid system
Nonlinear superposition law
dc.subject.eng.fl_str_mv Ermakov system
Ermakov–Milne–Pinney equation
Relativistic Ermakov–Lewis invariant
Relativistic Ray–Reid system
Nonlinear superposition law
description The Ermakov–Milne–Pinney equation is ubiquitous in many areas of physics that have an explicit time-dependence, including quantum systems with time-dependent Hamiltonian, cosmology, time-dependent harmonic oscillators, accelerator dynamics, etc. The Eliezer and Gray physical interpretation of the Ermakov–Lewis invariant is applied as a guiding principle for the derivation of the special relativistic analog of the Ermakov–Milne–Pinney equation and associated first integral. The special relativistic extension of the Ray–Reid system and invariant is obtained. General properties of the relativistic Ermakov–Milne–Pinney are analyzed. The conservative case of the relativistic Ermakov–Milne–Pinney equation is described in terms of a pseudo-potential, reducing the problem to an effective Newtonian form. The non-relativistic limit is considered to be well. A relativistic nonlinear superposition law for relativistic Ermakov systems is identified. The generalized Ermakov–Milne–Pinney equation has additional nonlinearities, due to the relativistic effects.
publishDate 2021
dc.date.accessioned.fl_str_mv 2021-04-08T04:17:32Z
dc.date.issued.fl_str_mv 2021
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dc.identifier.nrb.pt_BR.fl_str_mv 001123312
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001123312
url http://hdl.handle.net/10183/219606
dc.language.iso.fl_str_mv eng
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dc.relation.ispartof.pt_BR.fl_str_mv Physics. Basel. Vol. 3, no. 1 (Mar.2021), p. 59-70
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