Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics

T. Rauscher; A. Heger; R. D. Hoffman; S.E. Woosley

doi:10.1016/S0375-9474(03)00852-2

Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics

T. Rauscher
, A. Heger
, R. D. Hoffman
, S.E. Woosley

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

19 Citations (Scopus)

Abstract

We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type 11 supernova. Calculations were done for 15 M-circle dot, 19 M-circle dot, 20 Mcircle dot, 21 Mcircle dot, and 25 Mcircle dot Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here, we focus on the nuclear inputs.

Original language	English
Pages (from-to)	463C-465C
Number of pages	3
Journal	Nuclear Physics A
Volume	718
DOIs	https://doi.org/10.1016/S0375-9474(03)00852-2
Publication status	Published - 5 May 2003
Event	7th International Symposium on Nuclei in the Cosmos (NIC7) - FUJI, Japan Duration: 8 Jul 2002 → 12 Jul 2002

Keywords

THERMONUCLEAR REACTION-RATES
MODEL CALCULATIONS
CROSS-SECTIONS
BEAM
O-18(ALPHA,GAMMA)NE-22

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10.1016/S0375-9474(03)00852-2

Cite this

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title = "Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics",

abstract = "We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type 11 supernova. Calculations were done for 15 M-circle dot, 19 M-circle dot, 20 Mcircle dot, 21 Mcircle dot, and 25 Mcircle dot Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here, we focus on the nuclear inputs.",

keywords = "THERMONUCLEAR REACTION-RATES, MODEL CALCULATIONS, CROSS-SECTIONS, BEAM, O-18(ALPHA,GAMMA)NE-22",

author = "T. Rauscher and A. Heger and Hoffman, \{R. D.\} and S.E. Woosley",

year = "2003",

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doi = "10.1016/S0375-9474(03)00852-2",

language = "English",

volume = "718",

pages = "463C--465C",

journal = "Nuclear Physics A",

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publisher = "Elsevier",

note = "7th International Symposium on Nuclei in the Cosmos (NIC7) ; Conference date: 08-07-2002 Through 12-07-2002",

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TY - JOUR

T1 - Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics

AU - Rauscher, T.

AU - Heger, A.

AU - Hoffman, R. D.

AU - Woosley, S.E.

PY - 2003/5/5

Y1 - 2003/5/5

N2 - We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type 11 supernova. Calculations were done for 15 M-circle dot, 19 M-circle dot, 20 Mcircle dot, 21 Mcircle dot, and 25 Mcircle dot Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here, we focus on the nuclear inputs.

AB - We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type 11 supernova. Calculations were done for 15 M-circle dot, 19 M-circle dot, 20 Mcircle dot, 21 Mcircle dot, and 25 Mcircle dot Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here, we focus on the nuclear inputs.

KW - THERMONUCLEAR REACTION-RATES

KW - MODEL CALCULATIONS

KW - CROSS-SECTIONS

KW - BEAM

KW - O-18(ALPHA,GAMMA)NE-22

U2 - 10.1016/S0375-9474(03)00852-2

DO - 10.1016/S0375-9474(03)00852-2

M3 - Article

SN - 0375-9474

VL - 718

SP - 463C-465C

JO - Nuclear Physics A

JF - Nuclear Physics A

T2 - 7th International Symposium on Nuclei in the Cosmos (NIC7)

Y2 - 8 July 2002 through 12 July 2002

ER -

Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics

Abstract

Keywords

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