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 7. The posterior distribution of the symmetry energy, Esym(2ρ0), for 30 ≤ L ≤ 90 MeV and 69 ≤ L ≤ 143 MeV. |
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