dc.contributorSpringer
dc.creatorRosu Barbus, Haret-Codratian
dc.creatorCornejo Pérez, Octavio
dc.date2018-03-21T23:42:24Z
dc.date2018-03-21T23:42:24Z
dc.date2003
dc.date.accessioned2023-07-17T22:04:06Z
dc.date.available2023-07-17T22:04:06Z
dc.identifierRosu, H.C., Cornejo, O., Reyes, M. et al. International Journal of Theoretical Physics (2003) 42: 2923.
dc.identifierhttp://hdl.handle.net/11627/3478
dc.identifierhttps://doi.org/10.1023/B:IJTP.0000006019.28659.88
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7543818
dc.description"Simple linear second-order differential equations have been written down for FRW cosmologies with barotropic fluids by Faraoni. His results have been extended by Rosu, who employed techniques belonging to nonrelativistic supersymmetry to obtain time-dependent adiabatic indices. Further extensions are presented here using the known connection between the linear second-order differential equations and Dirac-like equations in the same supersymmetric context. These extensions are equivalent to adding an imaginary part to the adiabatic index which is proportional to the mass parameter of the Dirac spinor. The natural physical interpretation of the imaginary part is related to the particular dissipation and instabilities of the barotropic FRW hydrodynamics that are introduced by means of this supersymmetric scheme."
dc.formatapplication/pdf
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.rightsAcceso Abierto
dc.subjectCosmology
dc.subjectSupersymmetry
dc.subjectBarotropic fluids
dc.subjectDirac equations
dc.subjectDissipation
dc.subjectFÍSICA
dc.titleLinear second-order differential equations for barotropic FRW cosmologies
dc.typearticle


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