Table 1.
The EOS parameters adopted in this study, where η and ς are the combination of K0 and L given by η = (K0L2)1/3 and 
.
| K0 (MeV) | L (MeV) | η (MeV) | ς (MeV) | SP–C (fm−3) | C–S (fm−3) | Δf/f (%) |
|---|---|---|---|---|---|---|
| 180 | 31.0 | 55.7 | 67.8 | 0.05887 | 0.07629 | −1.25 |
| 180 | 52.2 | 78.9 | 90.5 | 0.06000 | 0.07186 | 1.14 |
| 230 | 42.6 | 74.7 | 90.1 | 0.06238 | 0.07671 | −0.12 |
| 230 | 73.4 | 107 | 122 | 0.06421 | 0.07099 | 0.81 |
| 280 | 54.9 | 94.5 | 113 | 0.06638 | 0.07743 | −1.10 |
| 280* | 97.5 | 139 | 156 | 0.06678 | 0.06887 | 0.43 |
| 360 | 12.8 | 38.9 | 56.4 | 0.05777 | 0.08217 | 0.62 |
| 360 | 76.4 | 128 | 152 | 0.07239 | 0.07797 | −0.60 |
Notes. The corresponding transition density from spherical to cylindrical nuclei (SP–C) and that from cylindrical to slab-like nuclei (C–S) are also listed. The asterisk at the value of K0 denotes the EOS model where cylindrical nuclei directly change to uniform matter. In the rightmost column, we also show the relative deviation of the frequencies estimated with the fit given by Eq. (3) from the eigenfrequencies for the model shown in Fig. 1.
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