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dc.date.accessioned 2022-09-12T13:11:38Z
dc.date.available 2022-09-12T13:11:38Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/141868
dc.description.abstract It was speculated (Witten, 1984) about the possibility that quarks (u,d,s) strange matter will be the fundamental level of the hadronic matter. If this is true, it seems possible the existence of transitions of exothermic phases of nuclear matter to strange matter. The conditions reached at the nucleus post-bounce epoch for a supernova of type II should be adequate for this process to take place. Assuming the existence of this transition we present the consequences of an explosion under these conditions. We used a gas at a finite temperature as equation of state for the quarks matter, while for the nuclear matter we used the equation of state for free neutrons as also the model of Bethe-Johnson. We conclude that in both situations the process is possible and it may be the responsible for the type II supernova explosions. en
dc.language es es
dc.subject Galaxia es
dc.title Can a phase transition of nuclear matter to quarks strange matter trigger the explosion of supernovae of type II? en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Benvenuto, Omar Gustavo es
sedici.creator.person Horvath, Jorge Ernesto es
sedici.creator.person Vucetich, Héctor es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion 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.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 33 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) es


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