Nucleosynthesis in a massive star associated with magnetohydrodynamical jets from collapsars

Masaomi Ono; Masa-Aki Hashimoto; S. Fujimoto; K. Kotake; S. Yamada

doi:10.1063/1.4763437

Nucleosynthesis in a massive star associated with magnetohydrodynamical jets from collapsars

Masaomi Ono, Masa-Aki Hashimoto, S. Fujimoto, K. Kotake, S. Yamada

Experimental Particle Physics

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

Abstract

We investigate the nucleosynthesis during the stellar evolution and the jet-like supernova explosion of a massive star of 70 M_⊙ having the solar metallicity in the main sequence stage. The nucleosynthesis calculations have been performed with large nuclear reaction networks, where the weak s-, p-, and r-processes are taken into account. As a result s-elements of 60 > A > 90 and r-elements of 90 > A > 160 are highly overproduced relative to the solar system abundances. We find that the Sr-Y-Zr isotopes are primarily synthesized in the explosive nucleosynthesis which could be one of the sites of the lighter element primary process (LEPP).

Original language	English
Title of host publication	Origin of Matter and Evolution of Galaxies 2011
Pages	412-414
Number of pages	3
DOIs	https://doi.org/10.1063/1.4763437
Publication status	Published - Dec 1 2012
Event	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan Duration: Nov 14 2011 → Nov 17 2011

Publication series

Name	AIP Conference Proceedings
Volume	1484
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Country/Territory	Japan
City	Wako
Period	11/14/11 → 11/17/11

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

Access to Document

10.1063/1.4763437

Cite this

Ono, M, Hashimoto, M-A, Fujimoto, S, Kotake, K & Yamada, S 2012, Nucleosynthesis in a massive star associated with magnetohydrodynamical jets from collapsars. in Origin of Matter and Evolution of Galaxies 2011. AIP Conference Proceedings, vol. 1484, pp. 412-414, International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011, Wako, Japan, 11/14/11. https://doi.org/10.1063/1.4763437

@inproceedings{ec8ab859c0114a028bd55190cc4f1cfa,

title = "Nucleosynthesis in a massive star associated with magnetohydrodynamical jets from collapsars",

abstract = "We investigate the nucleosynthesis during the stellar evolution and the jet-like supernova explosion of a massive star of 70 M⊙ having the solar metallicity in the main sequence stage. The nucleosynthesis calculations have been performed with large nuclear reaction networks, where the weak s-, p-, and r-processes are taken into account. As a result s-elements of 60 > A > 90 and r-elements of 90 > A > 160 are highly overproduced relative to the solar system abundances. We find that the Sr-Y-Zr isotopes are primarily synthesized in the explosive nucleosynthesis which could be one of the sites of the lighter element primary process (LEPP).",

author = "Masaomi Ono and Masa-Aki Hashimoto and S. Fujimoto and K. Kotake and S. Yamada",

year = "2012",

month = dec,

day = "1",

doi = "10.1063/1.4763437",

language = "English",

isbn = "9780735410961",

series = "AIP Conference Proceedings",

pages = "412--414",

booktitle = "Origin of Matter and Evolution of Galaxies 2011",

note = "International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 ; Conference date: 14-11-2011 Through 17-11-2011",

}

TY - GEN

T1 - Nucleosynthesis in a massive star associated with magnetohydrodynamical jets from collapsars

AU - Ono, Masaomi

AU - Hashimoto, Masa-Aki

AU - Fujimoto, S.

AU - Kotake, K.

AU - Yamada, S.

PY - 2012/12/1

Y1 - 2012/12/1

N2 - We investigate the nucleosynthesis during the stellar evolution and the jet-like supernova explosion of a massive star of 70 M⊙ having the solar metallicity in the main sequence stage. The nucleosynthesis calculations have been performed with large nuclear reaction networks, where the weak s-, p-, and r-processes are taken into account. As a result s-elements of 60 > A > 90 and r-elements of 90 > A > 160 are highly overproduced relative to the solar system abundances. We find that the Sr-Y-Zr isotopes are primarily synthesized in the explosive nucleosynthesis which could be one of the sites of the lighter element primary process (LEPP).

AB - We investigate the nucleosynthesis during the stellar evolution and the jet-like supernova explosion of a massive star of 70 M⊙ having the solar metallicity in the main sequence stage. The nucleosynthesis calculations have been performed with large nuclear reaction networks, where the weak s-, p-, and r-processes are taken into account. As a result s-elements of 60 > A > 90 and r-elements of 90 > A > 160 are highly overproduced relative to the solar system abundances. We find that the Sr-Y-Zr isotopes are primarily synthesized in the explosive nucleosynthesis which could be one of the sites of the lighter element primary process (LEPP).

UR - http://www.scopus.com/inward/record.url?scp=84874527654&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84874527654&partnerID=8YFLogxK

U2 - 10.1063/1.4763437

DO - 10.1063/1.4763437

M3 - Conference contribution

AN - SCOPUS:84874527654

SN - 9780735410961

T3 - AIP Conference Proceedings

SP - 412

EP - 414

BT - Origin of Matter and Evolution of Galaxies 2011

T2 - International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011

Y2 - 14 November 2011 through 17 November 2011

ER -

Nucleosynthesis in a massive star associated with magnetohydrodynamical jets from collapsars

Abstract

Publication series

Other

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this