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Estimation of the Neutron Star Mass and Radius of FRB 20240114A by Identification of Crustal Oscillations

  • Authors: Hajime Sotani, Z. Wadiasingh, C. Chirenti

Hajime Sotani et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

Constraint on K0 obtained from the combination of the constraints on L shown in Figure 2 and ς shown in Figure 4 by identifying the QPO frequencies with the crustal torsional oscillations. For reference, the fiducial value of K0 obtained from the terrestrial experiments, i.e., K0 = 240 ± 20 MeV (S. Shlomo et al. 2006), is also shown.

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