| dc.creator | Orsaria, Milva Gabriela | |
| dc.creator | Ranea Sandoval, Ignacio Francisco | |
| dc.creator | Vucetich, Héctor | |
| dc.creator | Weber, Fridolin | |
| dc.date | 2011 | |
| dc.date | 2022-03-10T14:52:44Z | |
| dc.date.accessioned | 2023-07-15T04:19:38Z | |
| dc.date.available | 2023-07-15T04:19:38Z | |
| dc.identifier | http://sedici.unlp.edu.ar/handle/10915/132337 | |
| dc.identifier | issn:0218-3013 | |
| dc.identifier | issn:1793-6608 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7469121 | |
| dc.description | The structure of a magnetized quark-hybrid stars (QHS) is modeled using a standard relativistic mean-field equation of state (EoS) for the description of hadronic matter. For quark matter we consider a bag model EoS which is modified perturbatively to account for the presence of a uniform magnetic field. The mass-radius (M-R) relationship, gravitational redshift and rotational Kepler periods of such stars are compared with those of standard neutron stars (NS). | |
| dc.description | Facultad de Ciencias Astronómicas y Geofísicas | |
| dc.format | application/pdf | |
| dc.format | 25-28 | |
| 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 | Astronomía | |
| dc.subject | Quark-hybrid star | |
| dc.subject | kepler periods | |
| dc.subject | gravitational redshift | |
| dc.title | Properties of Magnetized Quark-Hybrid Stars | |
| dc.type | Articulo | |
| dc.type | Preprint | |
