Fig. 1.
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First overtone of the ℓ = 2 crustal torsional oscillations for a neutron star model with M = 1.6 M⊙, R = 12 km, and Ns/Nd = 0. The marks denote the torsional oscillation frequencies estimated for the neutron star models constructed based on the crustal EOSs listed in Table 1, as a function of ς. The thick solid line is the quadratic fitting given by Eq. (3).
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