Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2021-10-13T13:44:35Z
dc.date.available 2021-10-13T13:44:35Z
dc.date.issued 2017-10
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/126543
dc.description.abstract The nonmesonic weak decay of Λ hypernuclei is studied within a microscopic diagrammatic approach which is extended to include the ΛN - ΣN strong interaction coupling. We adopt a nuclear matter formalism which, through the local density approximation, allows us to model finite hypernuclei. One-meson-exchange potentials are used for the weak and strong four-baryon interactions. The rates for the neutron- and proton-induced weak decays, ΛN → nN and ΛN → ΣN → nN (N = n or p; Σ = Σ⁻, Σ⁰, and Σ⁺), are predicted for Λ¹²C, Λ²⁸Si, Λ⁵⁶Fe, and Λ²⁰⁸Pb. The ΛN - ΣN coupling turns out to provide a contribution of about 23% (5%) to the total neutron-induced rate (proton-induced rate). Again as an effect of the hyperon coupling, the total one-nucleon-induced rate increases by about 9%, while the Γnp ratio increases by about 17%. The saturation property of the nonmesonic rates with increasing hypernuclear mass number is clearly obtained and explained. The above percentage modifications remain almost unaltered through the hypernuclear mass number. All the non-negligible changes introduced by the ΛN - ΣN coupling lead to a definite improvement of our predictions once compared with the available KEK and FINUDA data. en
dc.language en es
dc.subject Physics es
dc.subject hypernuclei es
dc.subject microscopic diagrammatic approach es
dc.subject nuclear matter es
dc.subject meson es
dc.subject nonmesonic weak decay es
dc.title Nonmesonic weak decay of Λ hypernuclei: The ΛN - ΣN coupling en
dc.type Articulo es
sedici.identifier.other arXiv:1701.03957 es
sedici.identifier.other doi:10.1103/physrevc.96.044303 es
sedici.identifier.issn 2469-9985 es
sedici.identifier.issn 2469-9993 es
sedici.creator.person Bauer, Eduardo es
sedici.creator.person Garbarino, G. es
sedici.creator.person Rodríguez Peña, Carlos Andrés es
sedici.subject.materias Astronomía es
sedici.subject.materias Ciencias Exactas es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
mods.originInfo.place Facultad de Ciencias Exactas es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Articulo 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 Physical Review C es
sedici.relation.journalVolumeAndIssue vol. 96, no. 4 es


Descargar archivos

Este ítem aparece en la(s) siguiente(s) colección(ones)

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)