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- W2169397311 abstract "We show that the superburst would be originated from thermonuclear burning ignited by accumulated fuels in the deep layers compared to normal X-ray bursts. Two cases are investigated for models related to superbursts by following thermal evolution of a realistic neutron star: helium flash and carbon flash accompanied with many normal bursts. For a helium flash, the burst shows the long duration when the accretion rate is low compared with the observation. The flash could become a superburst if the burning develops to the deflagration and/or detonation. For a carbon flash accompanied with many normal bursts, after successive 2786 normal bursts during 1.81 × 10 9 s, the temperature reaches the deflagration temperature. This is due to the produced carbon which amount reaches to ≈0.1 in the mass fraction. The flash will develop to dynamical phenomena of the deflagration and/or detonation, which may lead to a superburst." @default.
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- W2169397311 date "2014-07-23" @default.
- W2169397311 modified "2023-09-26" @default.
- W2169397311 title "Numerical Experiments for Nuclear Flashes toward Superbursts in an Accreting Neutron Star" @default.
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- W2169397311 doi "https://doi.org/10.1155/2014/817986" @default.
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