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- W3042920238 abstract "In this undergraduate project, f-mode oscillations in neutron stars are used to constrain the equation of state of dense matter. For the first time, a systematic investigation of the role of nuclear saturation parameters on the mode oscillations is performed. It is found that the uncertainty in the determination of effective nucleon mass plays the most significant role in controlling the f-mode frequencies. Correlations of the frequencies with astrophysical observables relevant for asteroseismology are also investigated. Future detection of f-mode frequencies could then provide a unique way of constraining nuclear empirical parameters and therefore the behaviour of dense matter." @default.
- W3042920238 created "2020-07-23" @default.
- W3042920238 creator A5026518696 @default.
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- W3042920238 date "2021-05-10" @default.
- W3042920238 modified "2023-10-10" @default.
- W3042920238 title "Constraining Dense Matter Physics Using f-Mode Oscillations in Neutron Stars" @default.
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- W3042920238 doi "https://doi.org/10.3390/physics3020022" @default.
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