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dc.date.accessioned 2024-07-08T17:55:49Z
dc.date.available 2024-07-08T17:55:49Z
dc.date.issued 2016
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/167889
dc.description.abstract The merger of a binary neutron star system is suggested as the central engine of short gamma-ray bursts (sGRBs). For the merger process, simulations predict that magnetic field is amplified beyond magnetar field strength by Kelvin-Helmholtz instabilities. With the Large Area Telescope (LAT), bursts have been detected that show a temporally extended component in coincidence with a short-lasting peak at the end of the prompt phase. We show that the presence of these LAT components in a sGRB could provide evidence of magnetic field amplification in the neutron star merger. en
dc.format.extent 49-54 es
dc.language en es
dc.subject binary neutron star system es
dc.subject short gamma-ray bursts es
dc.title High-energy emission as signature of magnetic field amplification in neutron star mergers en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-3-4 es
sedici.creator.person Fraija Cabrera, Nissim Illich es
sedici.creator.person Lee, William Henry es
sedici.creator.person Veres, Peter es
sedici.creator.person Barniol Duran, Rodolfo es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Objeto de conferencia 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.date.exposure 2015-10
sedici.relation.event High-Energy Phenomena tn Relativistic Outflows V (La Plata, 5 al 8 de octubre de 2015) es
sedici.description.peerReview peer-review es
sedici.relation.isRelatedWith https://sedici.unlp.edu.ar/handle/10915/167830 es
sedici.relation.bookTitle Proceedings of the High-Energy Phenomena in Relativistic Outflows V meeting es


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