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Barotropic FRW cosmologies with Chiellini damping
HARET CODRATIAN ROSU
Acceso Abierto
Atribución-NoComercial-SinDerivadas
https://doi.org/10.1016/j.physleta.2015.01.001
Barotropic
FRW cosmology
Ermakov-Pinney equation
Chiellini damping
"It is known that barotropic FRW equations written in the conformal time variable can be reduced to simple linear equations for an exponential function involving the conformal Hubble rate. Here, we show that an interesting class of barotropic universes can be obtained in the linear limit of a special type of nonlinear dissipative Ermakov-Pinney equations with the nonlinear dissipation built from Chiellini’s integrability condition. These cosmologies, which evolutionary are similar to the standard ones, correspond to barotropic fluids with adiabatic indices rescaled by a particular factor and have amplitudes of the scale factors inverse proportional to the adiabatic index."
Elsevier
2015
Artículo
Inglés
Público en general
Haret C. Rosu, Stefan C. Mancas, Pisin Chen, Barotropic FRW cosmologies with Chiellini damping, Physics Letters A, Volume 379, Issue 10, 2015, Pages 882-887, ISSN 0375-9601, http://dx.doi.org/10.1016/j.physleta.2015.01.001.
CIENCIAS FÍSICO MATEMÁTICAS Y CIENCIAS DE LA TIERRA
Versión aceptada
acceptedVersion - Versión aceptada
Aparece en las colecciones: Publicaciones Científicas Nanociencias y Materiales

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