The importance of the mixed phase in hybrid stars built with the Nambu-Jona-Lasinio model
arXiv:1009.2906 · doi:10.1140/epja/i2010-11059-0
Abstract
We investigate the structure of hybrid stars based on two different constructions: one is based on the Gibbs condition for phase coexistence and considers the existence of a mixed phase (MP), and the other is based on the Maxwell construction and no mixed phase is obtained. The hadron phase is described by the non-linear Walecka model (NLW) and the quark phase by the Nambu-Jona-Lasinio model (NJL). We conclude that the masses and radii obtained are model dependent but not significantly different for both constructions.
8 pages, 7 figures, 3 tables
References in corpus (6)
- Modern compact star observations and the quark matter equation of state
- Hadron-quark mixed phase in hyperon stars
- Stability of CFL cores in Hybrid Stars
- Influence of the hadronic equation of state on the hadron-quark phase transition in neutron stars
- Lepton effects on the proto-neutron stars with the hadron-quark mixed phase in the Nambu-Jona-Lasinio model
- Deconfinement of neutron star matter within the Nambu-Jona-Lasinio model
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