Numerical simulations of core-collapse supernovae imposing steady shock approximation

Masaru Watanabe; Tatsuya Yamasaki; Hideyuki Suzuki; Shoichi Yamada

doi:10.1088/1742-6596/31/1/030

Numerical simulations of core-collapse supernovae imposing steady shock approximation

Masaru Watanabe^*, Tatsuya Yamasaki, Hideyuki Suzuki, Shoichi Yamada

^*Corresponding author for this work

School of Advanced Science and Engineering

Research output: Contribution to journal › Article › peer-review

Abstract

We carried out one-dinensional long-term numerical simulations of core-collapse supernovae imposing steady shock approximation. As a result of a computation, we found core does not explode and shock wave stalls within several hundreds milliseconds from bounce. However, we execute long-term numerical simulation until 3.5 seconds from bounce with short CPU time using Personal Computer.

Original language	English
Pages (from-to)	155-156
Number of pages	2
Journal	Journal of Physics: Conference Series
Volume	31
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/31/1/030
Publication status	Published - 2006 Mar 22

ASJC Scopus subject areas

Physics and Astronomy(all)

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10.1088/1742-6596/31/1/030

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title = "Numerical simulations of core-collapse supernovae imposing steady shock approximation",

abstract = "We carried out one-dinensional long-term numerical simulations of core-collapse supernovae imposing steady shock approximation. As a result of a computation, we found core does not explode and shock wave stalls within several hundreds milliseconds from bounce. However, we execute long-term numerical simulation until 3.5 seconds from bounce with short CPU time using Personal Computer.",

author = "Masaru Watanabe and Tatsuya Yamasaki and Hideyuki Suzuki and Shoichi Yamada",

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doi = "10.1088/1742-6596/31/1/030",

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AU - Suzuki, Hideyuki

AU - Yamada, Shoichi

PY - 2006/3/22

Y1 - 2006/3/22

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AB - We carried out one-dinensional long-term numerical simulations of core-collapse supernovae imposing steady shock approximation. As a result of a computation, we found core does not explode and shock wave stalls within several hundreds milliseconds from bounce. However, we execute long-term numerical simulation until 3.5 seconds from bounce with short CPU time using Personal Computer.

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Numerical simulations of core-collapse supernovae imposing steady shock approximation

Abstract

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