Non-characteristic half-lives in radioactive decay

dc.contributor
Centre de Recerca Matemàtica
dc.contributor.author
Corral, Álvaro
dc.contributor.author
Font Martinez, Francesc
dc.contributor.author
Camacho Castro, Juan
dc.date.accessioned
2011-09-21T07:44:51Z
dc.date.accessioned
2024-09-19T13:21:21Z
dc.date.available
2011-09-21T07:44:51Z
dc.date.available
2024-09-19T13:21:21Z
dc.date.created
2011
dc.date.issued
2011
dc.identifier.uri
http://hdl.handle.net/2072/169739
dc.description.abstract
Half-lives of radionuclides span more than 50 orders of magnitude. We characterize the probability distribution of this broad-range data set at the same time that explore a method for fitting power-laws and testing goodness-of-fit. It is found that the procedure proposed recently by Clauset et al. [SIAM Rev. 51, 661 (2009)] does not perform well as it rejects the power-law hypothesis even for power-law synthetic data. In contrast, we establish the existence of a power-law exponent with a value around 1.1 for the half-life density, which can be explained by the sharp relationship between decay rate and released energy, for different disintegration types. For the case of alpha emission, this relationship constitutes an original mechanism of power-law generation.
cat
dc.format.extent
16
ca
dc.format.extent
291411 bytes
dc.format.mimetype
application/pdf
dc.language.iso
eng
ca
dc.publisher
Centre de Recerca Matemàtica
ca
dc.relation.ispartofseries
Prepublicacions del Centre de Recerca Matemàtica;1023
dc.rights
Aquest document està subjecte a una llicència d'ús de Creative Commons, amb la qual es permet copiar, distribuir i comunicar públicament l'obra sempre que se'n citin l'autor original, la universitat i el centre i no se'n faci cap ús comercial ni obra derivada, tal com queda estipulat en la llicència d'ús (http://creativecommons.org/licenses/by-nc-nd/2.5/es/)
cat
dc.subject.other
Radioactivitat
ca
dc.title
Non-characteristic half-lives in radioactive decay
ca
dc.type
info:eu-repo/semantics/preprint
ca
dc.subject.udc
539
ca


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