General solution of a fractional diffusion–advection equation for solar cosmic-ray transport

dc.creatorRocca, Mario Carlos
dc.creatorPlastino, Ángel Ricardo
dc.creatorPlastino, Ángel Luis
dc.creatorFerri, Gustavo Luís
dc.creatorDe Paoli, Ángel Luis
dc.date2016-04
dc.date2022-02-07T18:02:03Z
dc.date.accessioned2023-07-15T04:15:33Z
dc.date.available2023-07-15T04:15:33Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/130639
dc.identifierissn:0378-4371
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7468862
dc.descriptionIn this effort we exactly solve the fractional diffusion–advection equation for solar cosmic-ray transport and give its general solution in terms of hypergeometric distributions. Numerical analysis of this equation shows that its solutions resemble power-laws.
dc.descriptionFacultad de Ciencias Exactas
dc.descriptionInstituto de Física La Plata
dc.formatapplication/pdf
dc.format402-410
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Exactas
dc.subjectFísica
dc.subjectDistributions
dc.subjectCosmic rays
dc.subjectDiffusion
dc.subjectSun
dc.subjectHeliosphere
dc.titleGeneral solution of a fractional diffusion–advection equation for solar cosmic-ray transport
dc.typeArticulo
dc.typeArticulo


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