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dc.contributor.authorHaas, Fernandopt_BR
dc.date.accessioned2021-04-08T04:17:32Zpt_BR
dc.date.issued2021pt_BR
dc.identifier.issn2624-8174pt_BR
dc.identifier.urihttp://hdl.handle.net/10183/219606pt_BR
dc.description.abstractThe 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.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofPhysics. Basel. Vol. 3, no. 1 (Mar.2021), p. 59-70pt_BR
dc.rightsOpen Accessen
dc.subjectErmakov systemen
dc.subjectEquação de Pinneypt_BR
dc.subjectErmakov–Milne–Pinney equationen
dc.subjectRelatividadept_BR
dc.subjectSistemas quanticospt_BR
dc.subjectRelativistic Ermakov–Lewis invarianten
dc.subjectRelativistic Ray–Reid systemen
dc.subjectNonlinear superposition lawen
dc.titleRelativistic Ermakov–Milne–Pinney Systems and First Integralspt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001123312pt_BR
dc.type.originEstrangeiropt_BR


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