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Linear second-order differential equations for barotropic FRW cosmologies
HARET CODRATIAN ROSU
OCTAVIO CORNEJO PEREZ
Acceso Abierto
Atribución-NoComercial-SinDerivadas
https://doi.org/10.1023/B:IJTP.0000006019.28659.88
Cosmology
Supersymmetry
Barotropic fluids
Dirac equations
Dissipation
"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."
Springer Link
2003
Artículo
Inglés
Público en general
Rosu, H.C., Cornejo, O., Reyes, M. et al. International Journal of Theoretical Physics (2003) 42: 2923.
FÍSICA
Versión revisada
submittedVersion - Versión revisada
Aparece en las colecciones: Publicaciones Científicas Nanociencias y Materiales

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