Constraining the Nuclear Equation of State of a Neutron Star via High-frequency Quasi-periodic Oscillation in Short Gamma-Ray Bursts
The determination of the equation of state (EOS) of a neutron star (NS) and its maximum mass is very important for understanding the formation and properties of NSs under extreme conditions, but they remain open questions.Short-duration gamma-ray bursts Baby Cereals (GRBs) are believed to originate from the merger of binary NSs or giant flares (GFs