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 5. The posterior distribution of Esym(2ρ0) constrained by an assumed observed frequency of 1.720 kHz with a one percent relative error, where the stellar masses are limited to the range 1.2–2.0 M⊙. |
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