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dc.date.accessioned 2020-07-14T17:08:04Z
dc.date.available 2020-07-14T17:08:04Z
dc.date.issued 2015-11
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/100637
dc.description.abstract 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. en
dc.format.extent 986-1009 es
dc.language en es
dc.subject Classical theories of gravity es
dc.subject Cosmic rays es
dc.subject Diffusion es
dc.subject Statistical methods es
dc.subject Ultradistributions es
dc.title New solution of diffusion-advection equation for cosmic-ray transport using ultradistributions en
dc.type Articulo es
sedici.identifier.uri https://ri.conicet.gov.ar/11336/20907 es
sedici.identifier.other http://dx.doi.org/10.1007/s10955-015-1359-x es
sedici.identifier.other hdl:11336/20907 es
sedici.identifier.issn 1572-9613 es
sedici.creator.person Rocca, Mario Carlos es
sedici.creator.person Plastino, Ángel Ricardo es
sedici.creator.person Plastino, Ángel Luis es
sedici.creator.person Ferri, Gustavo Luis es
sedici.creator.person De Paoli, Ángel Luis es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Exactas es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Journal of Statistical Physics es
sedici.relation.journalVolumeAndIssue vol. 161, no. 4 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)