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The internal structure of pulsar‐like compact stars is still a puzzle, as the equation of state (EoS) of cold dense matter is unclear yet. One way to distinguish between different EoSs of compact stars is based on the maximum mass of different EoSs, which can be estimated by solving the Tolman–Oppenheimer–Volkoff (TOV) equation. In a more realistic consideration, rotations should to be taken into...
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