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- W2789713210 abstract "Gravitational collapse, bounce, and explosion of an iron core of an 11.2M⊙ star are simulated by two-dimensional neutrino-radiation hydrodynamic code. The explosion is driven by the neutrino heating aided by multi-dimensional hydrodynamic effects such as convection. Following the explosion phase, we continue the simulation focusing on the thermal evolution of the protoneutron star up to ∼ 70 s when the crust of the neutron star is formed, using one-dimensional simulation. We find that the crust forms at a high-density region (ρ ∼ 10 14 gc m −3 )a nd it proceeds from inside to outside. This is the first self-consistent simulation that successfully follows from the collapse phase to the protoneutron star cooling phase based on multi-dimensional hydrodynamic simulation." @default.
- W2789713210 created "2018-03-29" @default.
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- W2789713210 date "2018-01-23" @default.
- W2789713210 modified "2023-10-16" @default.
- W2789713210 title "From Supernovae to Neutron Stars" @default.
- W2789713210 doi "https://doi.org/10.7566/jpscp.20.011020" @default.
- W2789713210 hasPublicationYear "2018" @default.
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