The plasma mechanism of stabilization of neutron-excess nuclei in stars

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dc.creatorVasiliev, B. V.
dc.date2009-02-12
dc.date2009-02-23
dc.date.accessioned2026-07-07T12:44:54Z
dc.date.available2026-07-07T12:44:54Z
dc.descriptionThe mechanism of stabilization of neutron-excess nuclei in stars is considered. This mechanism must produce the neutronisation process in hot stars in the same way as it occurs in the dwarfs.
dc.identifierhttps://arxiv.org/abs/0902.2077
dc.identifierhttp://arxiv.org/abs/0902.2077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/220929
dc.subjectSolar and Stellar Astrophysics
dc.titleThe plasma mechanism of stabilization of neutron-excess nuclei in stars
dc.typetext

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