The g-mode frequencies in cold neutron stars and nuclear saturation parameters

arXiv:2608.02463 · nucl-th, astro-ph.HE · Submitted 2026-08-03 · Read on arXiv

nucl-th, astro-ph.HE

Submitted: 2026-08-03

Updated: 2026-08-03

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 6× in this paper · explained in 2 episodes
• Accuracy — 3× in this paper · explained in 1 episode
• Equation of State (EoS) — 1× in this paper · explained in 4 episodes
• Inverse Problem — 1× in this paper · explained in 2 episodes
• Systematic Bias — 1× in this paper · explained in 3 episodes

Sources

• Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations

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