dc.creator | Orsaria, Milva Gabriela | |
dc.creator | Ranea Sandoval, Ignacio Francisco | |
dc.creator | Vucetich, Héctor | |
dc.date | 2011 | |
dc.date | 2019-10-24T12:55:53Z | |
dc.identifier | http://sedici.unlp.edu.ar/handle/10915/83944 | |
dc.identifier | issn:0004-637X | |
dc.description | We 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.description | Facultad de Ciencias Astronómicas y Geofísicas | |
dc.format | application/pdf | |
dc.language | en | |
dc.rights | http://creativecommons.org/licenses/by-nc-sa/4.0/ | |
dc.rights | Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) | |
dc.subject | Ciencias Astronómicas | |
dc.subject | dense matter | |
dc.subject | magnetic fields | |
dc.subject | methods: analytical | |
dc.subject | stars: agnetars | |
dc.subject | stars: individual (Quark Stars) | |
dc.title | Magnetars as highly magnetized quark stars: An analytical treatment | |
dc.type | Articulo | |
dc.type | Articulo | |