Equations of state for mixed stars

AUTOR(ES)

Menezes, D. P., Providência, C.

FONTE

Brazilian Journal of Physics

DATA DE PUBLICAÇÃO

2004-09

RESUMO

We investigate the properties of mixed stars formed by hadronic and quark matter in beta-equilibrium described by appropriate equations of state (EOS) in the framework of relativistic mean-field theory. We use the non-linear Walecka model for the hadron matter and the MIT Bag and the Nambu-Jona-Lasinio models for the quark matter. The calculations were performed for T = 0 and for finite temperatures in order to describe neutron and proto-neutron stars. The star properties are discussed. Both the Bag model and the NJL model predict a mixed phase in the interior of the star.

Documentos Relacionados

• Analysis of equations of state for polymers
• A reduction method for phase equilibrium calculations with cubic equations of state
• Relativistic equations of state at finite temperature
• Considerations about equations for steady state flow in natural gas pipelines
• Mixed-state transport characteristics of magnesium diboride films