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- W2019923031 abstract "We investigate the role of the strange σ* and ϕ meson fields on the delineation of the main properties of neutron stars using a parameterized Lagrangian density model in the effective baryon and meson sectors. We assume strange quarks are localized within the hyperon fields which carry the strangeness content of the model. Our main goal is to analyze stability conditions of neutron stars with a large amount of strangeness per baryon. Our main result indicates the inclusion of the strange meson fields σ* and ϕ into nuclear matter make the equation of state stiffer thereby increasing the gravitational mass of the neutron star." @default.
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- W2019923031 date "2007-02-01" @default.
- W2019923031 modified "2023-09-23" @default.
- W2019923031 title "STABILITY OF NEUTRON STARS WITH A LARGE AMOUNT OF STRANGENESS" @default.
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- W2019923031 doi "https://doi.org/10.1142/s0218271807010110" @default.
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