dc.creatorOrsaria, Milva Gabriela
dc.creatorRanea Sandoval, Ignacio Francisco
dc.creatorVucetich, Héctor
dc.date2011
dc.date2019-10-24T12:55:53Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/83944
dc.identifierissn:0004-637X
dc.descriptionWe present an analytical model of a magnetar as a high-density magnetized quark bag. The effect of strong magnetic fields (B > 5 × 10 16 G) in the equation of state is considered. An analytic expression for the mass-radius relationship is found from the energy variational principle in general relativity. Our results are compared with observational evidence of possible quark and/or hybrid stars.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectdense matter
dc.subjectmagnetic fields
dc.subjectmethods: analytical
dc.subjectstars: agnetars
dc.subjectstars: individual (Quark Stars)
dc.titleMagnetars as highly magnetized quark stars: An analytical treatment
dc.typeArticulo
dc.typeArticulo


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