Linear second-order differential equations for barotropic FRW cosmologies

"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 extensi...

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Detalles Bibliográficos
Autores: HARET CODRATIAN ROSU, OCTAVIO CORNEJO PEREZ
Tipo de recurso: artículo
Estado:Versión enviada para evaluación y publicación
Fecha de publicación:2003
País:México
Institución:Instituto Potosino de Investigación Científica y Tecnológica
Repositorio:Repositorio Institucional del IPICYT
Idioma:inglés
OAI Identifier:oai:ipicyt.repositorioinstitucional.mx:1010/954
Acceso en línea:http://ipicyt.repositorioinstitucional.mx/jspui/handle/1010/954
Access Level:acceso abierto
Palabra clave:info:eu-repo/classification/Autor/Cosmology
info:eu-repo/classification/Autor/Supersymmetry
info:eu-repo/classification/Autor/Barotropic fluids
info:eu-repo/classification/Autor/Dirac equations
info:eu-repo/classification/Autor/Dissipation
info:eu-repo/classification/cti/1
info:eu-repo/classification/cti/22
Descripción
Sumario:"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."