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 4. The most probable Esym(2ρ0) as a function of the f-mode frequency (with a 1% relative error) of a canonical neutron star, where the gray area denotes the uncertainty band at a 90% credibility level. For comparison, the posterior distributions of two points (f = 1.720 & 1.900 kHz) with a 5% relative error are also presented. |
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