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We study the effects of nuclear equation of state (EOS) on Type-I X-ray bursts, focusing on the  Clocked burster  GS 1826–24. According to the  shell-flush  model, the surface gravity of the neutron stars (NSs) strengthens burst activities, where the recurrence time and peak luminosity are higher for larger-radius EOSs. We show that such a prediction matches with the  full  multi-zone model, in which whole NS regions are considered in burst calculation. We also show that the large-radius EOSs are not preferred to account for the observed light curves of GS 1826–24.

Effects of Nuclear Equation of State on Type-I X-ray Bursts and Implication for Clocked Burster GS 1826–24