Nucleosynthesis in type II supernovae

K. Nomoto; M. Hashimoto; T. Tsujimoto; F. K. Thielemann; N. Kishimoto; Y. Kubo; N. Nakasato

doi:10.1016/S0375-9474(97)00076-6

Nucleosynthesis in type II supernovae

K. Nomoto, M. Hashimoto, T. Tsujimoto, F. K. Thielemann, N. Kishimoto, Y. Kubo, N. Nakasato

Experimental Particle Physics

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

211 Citations (Scopus)

Abstract

Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 M_⊙ to 70 M_⊙ are calculated. We examine the dependence of the supernova yields on the stellar mass, ¹²C(α, γ)¹⁶O rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

Original language	English
Pages (from-to)	79-90
Number of pages	12
Journal	Nuclear Physics A
Volume	616
Issue number	1-2
DOIs	https://doi.org/10.1016/S0375-9474(97)00076-6
Publication status	Published - Apr 14 1997

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics

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title = "Nucleosynthesis in type II supernovae",

abstract = "Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 M⊙ to 70 M⊙ are calculated. We examine the dependence of the supernova yields on the stellar mass, 12C(α, γ)16O rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.",

author = "K. Nomoto and M. Hashimoto and T. Tsujimoto and Thielemann, {F. K.} and N. Kishimoto and Y. Kubo and N. Nakasato",

note = "Funding Information: This work has been supported in part by the Grant in Aid for Scientific Research (05243206, 06234210) and COE research (07CE2002) of the Ministry of Education, Science, and Culture in Japan. Copyright: Copyright 2018 Elsevier B.V., All rights reserved.",

year = "1997",

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doi = "10.1016/S0375-9474(97)00076-6",

language = "English",

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TY - JOUR

T1 - Nucleosynthesis in type II supernovae

AU - Nomoto, K.

AU - Hashimoto, M.

AU - Tsujimoto, T.

AU - Thielemann, F. K.

AU - Kishimoto, N.

AU - Kubo, Y.

AU - Nakasato, N.

N1 - Funding Information: This work has been supported in part by the Grant in Aid for Scientific Research (05243206, 06234210) and COE research (07CE2002) of the Ministry of Education, Science, and Culture in Japan. Copyright: Copyright 2018 Elsevier B.V., All rights reserved.

PY - 1997/4/14

Y1 - 1997/4/14

N2 - Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 M⊙ to 70 M⊙ are calculated. We examine the dependence of the supernova yields on the stellar mass, 12C(α, γ)16O rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

AB - Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 M⊙ to 70 M⊙ are calculated. We examine the dependence of the supernova yields on the stellar mass, 12C(α, γ)16O rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

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DO - 10.1016/S0375-9474(97)00076-6

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SP - 79

EP - 90

JO - Nuclear Physics A

JF - Nuclear Physics A

SN - 0375-9474

IS - 1-2

ER -

Nucleosynthesis in type II supernovae

Abstract

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