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dc.date.accessioned 2021-08-31T17:45:45Z
dc.date.available 2021-08-31T17:45:45Z
dc.date.issued 2017-08-13
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/123861
dc.description.abstract We study the possibility of a hadron-quark phase transition in the interior of neutron stars, taking into account different schematic evolutionary stages at finite temperature. Furthermore, we analyze the astrophysical properties of hot and cold hybrid stars, considering the constraint on maximum mass given by the pulsars J1614-2230 and J1614-2230. We obtain cold hybrid stars with maximum masses ≥ 2 M⊙ . Our study also suggest that during the proto-hybrid star evolution a late phase transition between hadronic matter and quark matter could occur, in contrast with previous studies of proto-neutron stars. en
dc.language en es
dc.subject Stars es
dc.subject Neutron es
dc.subject Equation of state es
dc.subject Dense matter es
dc.title Simplified Thermal Evolution of Proto-hybrid Stars en
dc.type Articulo es
sedici.identifier.other arXiv:1704.07732 es
sedici.identifier.other doi:10.1142/s2010194517600412 es
sedici.identifier.issn 2010-1945 es
sedici.creator.person Mariani, Mauro es
sedici.creator.person Orsaria, Milva Gabriela es
sedici.creator.person Vucetich, Héctor es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution 4.0 International (CC BY 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by/4.0/
sedici.relation.event 7th International Workshop on Astronomy and Relativistic Astrophysics (IWARA 2016) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle International Journal of Modern Physics: Conference Series es
sedici.relation.journalVolumeAndIssue vol. 45 es


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Creative Commons Attribution 4.0 International (CC BY 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution 4.0 International (CC BY 4.0)