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Mass-radius relation for magnetized strange quark stars

We review the stability of magnetized strange quark matter (MSQM) within the phenomenological MIT bag model, taking into account the variation of the relevant input parameters, namely, the strange quark mass, baryon density, magnetic field and bag parameter. A comparison with magnetized asymmetric q...

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Detalles Bibliográficos
Autores principales: Martinez, A Perez, Felipe, R Gonzalez, Paret, D Manreza
Formato: info:eu-repo/semantics/article
Lenguaje:eng
Publicado: Int. J. Mod. Phys. D 2010
Materias:
Acceso en línea:https://dx.doi.org/10.1142/S0218271810017378
http://cds.cern.ch/record/1235329