INVESTIGADORES
RANEA SANDOVAL ignacio Francisco
artículos
Título:
Properties of Magnetized Quark-Hybrid Stars
Autor/es:
MILVA G. ORSARIA; IGNACIO FRANCISCO RANEA SANDOVAL; HÉCTOR VUCETICH; FRIDOLIN WEBER
Revista:
INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS
Editorial:
WORLD SCIENTIFIC PUBL CO PTE LTD
Referencias:
Año: 2011 vol. 20 p. 25 - 28
ISSN:
0218-3013
Resumen:
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).
