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- W4210365662 abstract "The recent measurement of the mass of neutron stars (PSR J1614ensuremath{-}2230, PSR J0348+0432, MSP J0740+6620) restricts the lower limit $ensuremath{sim}2{M}_{ensuremath{bigodot}}$ of the maximum mass of such compact stars, making it possible for dense matter to exist in massive stars. The relativistic mean-field theory with parameter sets FSUGold including kaon condensation is used to describe the properties of neutron stars in $ensuremath{beta}$ equilibrium. Through careful choice of the parameter of the $ensuremath{sigma}$-cut ${c}_{ensuremath{sigma}}$, we are able to produce a maximum mass neutron star with kaon condensation heavier than $2{M}_{ensuremath{bigodot}}$, and we find that the parameter ${mathrm{ensuremath{Lambda}}}_{ensuremath{nu}}$ of the $ensuremath{rho}ensuremath{-}ensuremath{omega}$ interaction term in this model has a significant effect on ${K}^{ensuremath{-}}$ condensation. In the case of using the $ensuremath{sigma}$-cut scheme, ${K}^{ensuremath{-}}$ condensation occurs only when the $ensuremath{rho}ensuremath{-}ensuremath{omega}$ interaction ${mathrm{ensuremath{Lambda}}}_{ensuremath{nu}}$ is switched off." @default.
- W4210365662 created "2022-02-08" @default.
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- W4210365662 date "2022-01-31" @default.
- W4210365662 modified "2023-10-01" @default.
- W4210365662 title "Kaon meson condensate in neutron star matter including hyperons" @default.
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- W4210365662 doi "https://doi.org/10.1103/physrevc.105.015807" @default.
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