New solution of diffusion–advection equation for cosmic-ray transport using ultradistributions

In this paper we exactly solve the diffusion–advection equation (DAE) for cosmic-ray transport. For such a purpose we use the Theory of Ultradistributions of J. Sebastiao e Silva, to give a general solution for the DAE. From the ensuing solution, we obtain several approximations as limiting cases of...

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Detalles Bibliográficos
Autores: Rocca, Mario Carlos, Plastino, Ángel Ricardo, Plastino, Ángel Luis, Ferri, Gustavo Luis, de Paoli, Ángel Luis
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2015
País:Argentina
Institución:Consejo Nacional de Investigaciones Científicas y Técnicas
Repositorio:CONICET Digital (CONICET)
Idioma:inglés
OAI Identifier:oai:ri.conicet.gov.ar:11336/20907
Acceso en línea:http://hdl.handle.net/11336/20907
Access Level:acceso abierto
Palabra clave:CLASSICAL THEORIES OF GRAVITY
COSMIC RAYS
DIFFUSION
STATISTICAL METHODS
ULTRADISTRIBUTIONS
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
Descripción
Sumario:In this paper we exactly solve the diffusion–advection equation (DAE) for cosmic-ray transport. For such a purpose we use the Theory of Ultradistributions of J. Sebastiao e Silva, to give a general solution for the DAE. From the ensuing solution, we obtain several approximations as limiting cases of various situations of physical and astrophysical interest. One of them involves Solar cosmic-rays’ diffusion.