Neutron star structure in a quark model with excluded volume correction

We study the effects of the finite size of baryons on the equation of state of homogeneous hadronic matter. The finite extension of hadrons is introduced in order to improve the performance of field theoretical models at very high densities. We simulate the in-medium averaged baryon-baryon strong re...

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Detalles Bibliográficos
Autores principales: Aguirre, Ricardo Miguel, De Paoli, Ángel Luis
Formato: Articulo
Lenguaje:Inglés
Publicado: 2003
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/125903
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