dc.creatorPlastino, Ángel Luis
dc.creatorRocca, Mario Carlos
dc.creatorFerri, Gustavo Luis
dc.creatorZamora, Darío Javier
dc.date.accessioned2019-03-13T21:10:34Z
dc.date.accessioned2022-10-15T13:33:24Z
dc.date.available2019-03-13T21:10:34Z
dc.date.available2022-10-15T13:33:24Z
dc.date.created2019-03-13T21:10:34Z
dc.date.issued2016-11
dc.identifierPlastino, Ángel Luis; Rocca, Mario Carlos; Ferri, Gustavo Luis; Zamora, Darío Javier; Q-Gamow states for intermediate energies; Elsevier Science; Nuclear Physics A; 955; 11-2016; 16-26
dc.identifier0375-9474
dc.identifierhttp://hdl.handle.net/11336/71595
dc.identifierCONICET Digital
dc.identifierCONICET
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4391769
dc.description.abstractIn a recent paper Plastino and Rocca (2016) [18] we have demonstrated the possible existence of Tsallis' q-Gamow states. Now, accelerators' experimental evidence for Tsallis' distributions has been ascertained only at very high energies. Here, instead, we develop a different set of q-Gamow states for which the associated q-Breit-Wigner distribution could easily be found at intermediate energies, for which accelerators are available at many locations. In this context, it should be strongly emphasized Vignat and Plastino (2009) [2] that, empirically, one never exactly and unambiguously "detects" pure Gaussians, but rather q-Gaussians. A prediction is made via Eq. (3.4).
dc.languageeng
dc.publisherElsevier Science
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0375947416301415
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1016/j.nuclphysa.2016.05.021
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/restrictedAccess
dc.subjectGAMOW STATES
dc.subjectQ-GAMOW STATES
dc.subjectQ-GAUSSIANS
dc.titleQ-Gamow states for intermediate energies
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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