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20122022
most citedPost-shock-revival evolutions in the neutrino-heating mechanism of core-collapse supernovae

32 citations · 110 across the 9 of their papers we have counts for

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Showing astro-ph.HEShow all

5 papers · 1 filter

astro-ph.HE2018★ 13 cited

On the importance of progenitor asymmetry to shock revival in core-collapse supernovae

Hiroki Nagakura, Kazuya Takahashi, Yu Yamamoto

The progenitor stars of core-collapse supernovae (CCSNe) are asymmetrically fluctuating due to turbulent convections in the late stages of their lives. The progenitor asymmetry at…

astro-ph.HE2018★ 20 cited

Effects of rotation and magnetic field on the revival of a stalled shock in supernova explosions

Kotaro Fujisawa, Hirotada Okawa, Yu Yamamoto +1

We investigate axisymmetric steady solutions of (magneto)hydrodynamics equations that describe approximately accretion flows through a standing shock wave and discuss the effects o…

astro-ph.HE2016★ 23 cited

Links between the shock instability in core-collapse supernovae and asymmetric accretions of envelopes

Kazuya Takahashi, Wakana Iwakami, Yu Yamamoto +1

The explosion mechanism of core-collapse supernovae has not been fully understood yet but multi-dimensional fluid instabilities such as standing accretion shock instability (SASI)…

astro-ph.HE2012★ 32 cited

Post-shock-revival evolutions in the neutrino-heating mechanism of core-collapse supernovae

Yu Yamamoto, Shin-ichiro Fujimoto, Hiroki Nagakura +1

We perform some experimental simulations in spherical symmetry and axisymmetry to understand the post-shock-revival evolution of core-collapse supernovae. Assuming that the stalled…

astro-ph.HE2012★ 16 cited

Semi-dynamical approach to the shock revival in core-collapse supernovae

Hiroki Nagakura, Yu Yamamoto, Shoichi Yamada

We develop a new semi-dynamical method to study shock revival by neutrino heating in core- collapse supernovae. Our new approach is an extension of the previous studies that employ…