Nucleosynthesis and Kilonovae from Strange Star Mergers

dc.creatorHorvath, J.
dc.creatorBenvenuto, Omar Gustavo
dc.creatorBauer, Eduardo
dc.creatorPaulucci, L.
dc.creatorBernardo, A.
dc.creatorViturro, H.
dc.date2019
dc.date2021-09-24T18:17:16Z
dc.date.accessioned2023-07-15T03:22:04Z
dc.date.available2023-07-15T03:22:04Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/125613
dc.identifierhttps://www.mdpi.com/2218-1997/5/6/144
dc.identifierissn:2218-1997
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7465442
dc.descriptionIn this talk, we summarize the work in progress toward a full characterization of strange star–strange star (SS–SS) mergers related to the GW/GRB/kilonova events. In addition, we show that the a priori probability constructed from the observed neutron star mass distribution points toward an asymmetric binary system as the progenitor of the GW170817 event.
dc.descriptionInstituto de Astrofísica de La Plata
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectCiencias Astronómicas
dc.subjectkilonovae
dc.subjectcompact star mergers
dc.subjectnucleosynthesis
dc.titleNucleosynthesis and Kilonovae from Strange Star Mergers
dc.typeArticulo
dc.typeComunicacion


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