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dc.contributor.authorHaas, Fernandopt_BR
dc.contributor.authorPascoal, Kellen Alvespt_BR
dc.date.accessioned2018-11-08T02:47:03Zpt_BR
dc.date.issued2017pt_BR
dc.identifier.issn1070-664Xpt_BR
dc.identifier.urihttp://hdl.handle.net/10183/184488pt_BR
dc.description.abstractIn a previous work [Haas et al., Phys. Plasmas 23, 012104 (2016)], a new model was introduced, taking into account the role of the Fermi weak force due to neutrinos coupled to magnetohydrodynamic plasmas. The resulting neutrino-magnetohydrodynamics was investigated in a particular geometry associated with the magnetosonic wave, where the ambient magnetic field and the wavevector are perpendicular. The corresponding fast, short wavelength neutrino beam instability was then obtained in the context of supernova parameters. The present communication generalizes these results, allowing for arbitrary direction of wave propagation, including fast and slow magnetohydrodynamic waves and the intermediate cases of oblique angles. The numerical estimates of the neutrino-plasma instabilities are derived in extreme astrophysical environments where dense neutrino beams exist. Published by AIP Publishing.en
dc.format.mimetypeapplication/pdfpt_BR
dc.language.isoengpt_BR
dc.relation.ispartofPhysics of plasmas. Melville. Vol. 24, no. 9 (Sept. 2017), 092109, 6 p.pt_BR
dc.rightsOpen Accessen
dc.subjectNeutrinospt_BR
dc.subjectMagneto-hidrodinâmica de plasmaspt_BR
dc.subjectOndas em plasmaspt_BR
dc.subjectInstabilidade em plasmaspt_BR
dc.subjectRelações de dispersãopt_BR
dc.titleInstabilities and propagation of neutrino magnetohydrodynamic waves in arbitrary directionpt_BR
dc.typeArtigo de periódicopt_BR
dc.identifier.nrb001047805pt_BR
dc.type.originEstrangeiropt_BR


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