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- W2013886559 abstract "We study the properties of neutron stars involving antikaon condensation with three different models in the framework of relativistic mean field (RMF) approximation theory: the Glendenning-Moszkowski (GM) model, the Zimanyi-Moszkowski (ZM) model, and the hybrid derivative coupling (HD) model. We take the isovector-scalar (ensuremath{delta}-meson) channel interaction into account in our calculations and find that large mass neutron stars with kaon condensation can exist if the kaon optical potential is appropriately weak. The ensuremath{delta}-meson channel interaction has a significant influence on the property of neutron stars and the effects are a little different for the three models." @default.
- W2013886559 created "2016-06-24" @default.
- W2013886559 creator A5004299434 @default.
- W2013886559 creator A5024962900 @default.
- W2013886559 creator A5042830817 @default.
- W2013886559 date "2008-08-08" @default.
- W2013886559 modified "2023-09-27" @default.
- W2013886559 title "Kaon condensation in neutron stars in relativistic mean field theory with isovector-scalar channel interaction" @default.
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