Constraint on nuclear symmetry energy imposed by f-mode oscillation of neutron stars
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Constraint on nuclear symmetry energy imposed by f-mode oscillation of neutron stars |
| Jing Zhang,Dehua Wen,Yuxi Li |
| Figure 2. The posterior distributions and correlations of Ksym, J0, Esym(ρ0), L, and Jsym constrained by an assumed observed frequency of 1.720 kHz with a one percent relative error for a canonical neutron star (M = 1.4 M⊙). |
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