Aspherical abundance distribution of ejecta from neutrino-driven core collapse supernova

Shinichiro Fujimoto; Kei Kotake; Masa-Aki Hashimoto; Masaomi Ono; Naofumi Ohnishi

doi:10.1063/1.3485205

Aspherical abundance distribution of ejecta from neutrino-driven core collapse supernova

Shinichiro Fujimoto, Kei Kotake, Masa-Aki Hashimoto, Masaomi Ono, Naofumi Ohnishi

Experimental Particle Physics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

We examine explosive nucleosynthesis during a delayed neutrino-driven, supernova explosion aided by standing accretion shock instability, based on two-dimensional hydrodynamic simulations of the explosion of a 15 M⊙progenitor.We find that abundance pattern of the supernova ejecta is similar to that of the solar system, for cases with high explosion energies of ≃ 10⁵¹ergs. Aspherical distribution of Fe, Si, and O, which is observed in a nearby core-collapse SN remnant such as Cas A, is obtained in spite of the explosion of the non-rotating, spherical progenitor.

Original language	English
Title of host publication	10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10
Pages	472-474
Number of pages	3
Volume	1269
DOIs	https://doi.org/10.1063/1.3485205
Publication status	Published - Sep 21 2010
Event	10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10 - Osaka, Japan Duration: Mar 8 2010 → Mar 10 2010

Other

Other	10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10
Country/Territory	Japan
City	Osaka
Period	3/8/10 → 3/10/10

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

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10.1063/1.3485205

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Aspherical abundance distribution of ejecta from neutrino-driven core collapse supernova. / Fujimoto, Shinichiro; Kotake, Kei; Hashimoto, Masa-Aki; Ono, Masaomi; Ohnishi, Naofumi.

10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10. Vol. 1269 2010. p. 472-474.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Fujimoto, S, Kotake, K, Hashimoto, M-A, Ono, M & Ohnishi, N 2010, Aspherical abundance distribution of ejecta from neutrino-driven core collapse supernova. in 10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10. vol. 1269, pp. 472-474, 10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10, Osaka, Japan, 3/8/10. https://doi.org/10.1063/1.3485205

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abstract = "We examine explosive nucleosynthesis during a delayed neutrino-driven, supernova explosion aided by standing accretion shock instability, based on two-dimensional hydrodynamic simulations of the explosion of a 15 M⊙progenitor.We find that abundance pattern of the supernova ejecta is similar to that of the solar system, for cases with high explosion energies of ≃ 1051ergs. Aspherical distribution of Fe, Si, and O, which is observed in a nearby core-collapse SN remnant such as Cas A, is obtained in spite of the explosion of the non-rotating, spherical progenitor.",

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doi = "10.1063/1.3485205",

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AU - Fujimoto, Shinichiro

AU - Kotake, Kei

AU - Hashimoto, Masa-Aki

AU - Ono, Masaomi

AU - Ohnishi, Naofumi

PY - 2010/9/21

Y1 - 2010/9/21

N2 - We examine explosive nucleosynthesis during a delayed neutrino-driven, supernova explosion aided by standing accretion shock instability, based on two-dimensional hydrodynamic simulations of the explosion of a 15 M⊙progenitor.We find that abundance pattern of the supernova ejecta is similar to that of the solar system, for cases with high explosion energies of ≃ 1051ergs. Aspherical distribution of Fe, Si, and O, which is observed in a nearby core-collapse SN remnant such as Cas A, is obtained in spite of the explosion of the non-rotating, spherical progenitor.

AB - We examine explosive nucleosynthesis during a delayed neutrino-driven, supernova explosion aided by standing accretion shock instability, based on two-dimensional hydrodynamic simulations of the explosion of a 15 M⊙progenitor.We find that abundance pattern of the supernova ejecta is similar to that of the solar system, for cases with high explosion energies of ≃ 1051ergs. Aspherical distribution of Fe, Si, and O, which is observed in a nearby core-collapse SN remnant such as Cas A, is obtained in spite of the explosion of the non-rotating, spherical progenitor.

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BT - 10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10

T2 - 10th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG10

Y2 - 8 March 2010 through 10 March 2010

ER -

Aspherical abundance distribution of ejecta from neutrino-driven core collapse supernova

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