Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-06-09
Phys.Rev. C72 (2005) 035802
Astronomy and Astrophysics
Astrophysics
10 pages, 6 figures
Scientific paper
10.1103/PhysRevC.72.035802
The properties of neutron stars constituted of a crust of hadrons and an internal part of hadrons and kaon condensate are calculated within the quark-meson-coupling model. We have considered stars with nucleons only in the hadron phase and also stars with hyperons as well. The results are compared with the ones obtained from the non-linear Walecka model for the hadronic phase.
Menezes Débora P.
Panda Prafulla Kumar
Providencia Constança
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