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dc.contributor.authorHaas, Fernandopt_BR
dc.contributor.authorPascoal, Kellen Alvespt_BR
dc.contributor.authorMendonça, José Titopt_BR
dc.date.accessioned2018-08-17T02:33:12Zpt_BR
dc.date.issued2017pt_BR
dc.identifier.issn1070-664Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/181073pt_BR
dc.description.abstractWe analyze the role of collisional effects on the coupling between ion-acoustic waves and neutrino flavor oscillations, discussing its relevance for plasma instabilities in extreme plasma environments like in type II supernovae, where intense neutrino bursts exist. Electrons (leptons) are coupled to the electron-neutrino fluid through the weak Fermi force, but the electron-neutrinos are allowed to convert to other neutrino flavors and vice versa. Due to the typically slow frequency of neutrino flavor oscillations, many orders smaller than, e.g., the plasma frequency, an effective energy transfer between plasma waves and neutrino flavor oscillations takes place at the low-frequency electrostatic branch, viz., the ion-acoustic mode. We show the destabilization of ion-acoustic waves in dense astrophysical scenarios, with a focus on the collisional effects mediated by electron-ion scattering. The maximal instability growth-rate is evaluated and compared to the characteristic inverse times of type II supernova explosions. The results can be used for independent experimental verification of the non-zero neutrino mass, in a plasma physics context. Published by AIP Publishing.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofPhysics of plasmas. Melville. Vol. 24, no. 5 (May 2017), 052115, 4 p.pt_BR
dc.rightsOpen Accessen
dc.subjectOscilações de neutrinospt_BR
dc.subjectOndas íon-acústicas em plasmaspt_BR
dc.subjectProcessos de colisao em plasmaspt_BR
dc.titleCollisional effects, ion-acoustic waves, and neutrino oscillationspt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001021336pt_BR
dc.type.originEstrangeiropt_BR


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