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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 2.

The optimal ranges of Lop ± 1σ to identify the observed QPO frequencies with the crustal torsional oscillations, shown for various NS models. The gray shaded regions denote the range of fiducial value of L, i.e., L = 60 ± 20 MeV in light gray (M. B. Tsang et al. 2012; W. G. Newton et al. 2014; B.-A. Li et al. 2019), and the range of L constrained from the identification of magnetar QPOs observed in SGR 1806-20 with crustal torsional oscillations, i.e., L = 58–73 MeV in dark gray (H. Sotani et al. 2018; H. Sotani 2024).

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