Alpha-clustering and the stellar nucleosynthesis of carbon

H. Oberhummer; H. Krauss; K. Grun; T. Rauscher; H. Abele; P. Mohr; G. Staudt

Alpha-clustering and the stellar nucleosynthesis of carbon

H. Oberhummer
, H. Krauss
, K. Grun
, T. Rauscher
, H. Abele
, P. Mohr
, G. Staudt

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

8 Citations (Scopus)

43 Downloads (Pure)

Abstract

The astrophysical S-factor and reaction rates for the triple-alpha process are calculated in the direct-capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N-N interaction.

Original language	English
Pages (from-to)	241-242
Number of pages	2
Journal	Zeitschrift fur Physik A-Hadrons and Nuclei
Volume	349
Issue number	3-4
Publication status	Published - Sept 1994
Event	2nd International Conference on Atomic and Nuclear Clusters - SANTORINI, Greece Duration: 28 Jun 1993 → 2 Jul 1993

Keywords

LIGHT-NUCLEI
SCATTERING

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@article{74a5e5f46d9e4bd5b3449e5659f52fe4,

title = "Alpha-clustering and the stellar nucleosynthesis of carbon",

abstract = "The astrophysical S-factor and reaction rates for the triple-alpha process are calculated in the direct-capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N-N interaction.",

keywords = "LIGHT-NUCLEI, SCATTERING",

author = "H. Oberhummer and H. Krauss and K. Grun and T. Rauscher and H. Abele and P. Mohr and G. Staudt",

year = "1994",

month = sep,

language = "English",

volume = "349",

pages = "241--242",

journal = "Zeitschrift fur Physik A-Hadrons and Nuclei",

issn = "0939-7922",

publisher = "Springer Nature ",

number = "3-4",

note = "2nd International Conference on Atomic and Nuclear Clusters ; Conference date: 28-06-1993 Through 02-07-1993",

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TY - JOUR

T1 - Alpha-clustering and the stellar nucleosynthesis of carbon

AU - Oberhummer, H.

AU - Krauss, H.

AU - Grun, K.

AU - Rauscher, T.

AU - Abele, H.

AU - Mohr, P.

AU - Staudt, G.

PY - 1994/9

Y1 - 1994/9

N2 - The astrophysical S-factor and reaction rates for the triple-alpha process are calculated in the direct-capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N-N interaction.

AB - The astrophysical S-factor and reaction rates for the triple-alpha process are calculated in the direct-capture model. It is shown that the stellar carbon production is extremely sensitive to small variations in the N-N interaction.

KW - LIGHT-NUCLEI

KW - SCATTERING

M3 - Article

SN - 0939-7922

VL - 349

SP - 241

EP - 242

JO - Zeitschrift fur Physik A-Hadrons and Nuclei

JF - Zeitschrift fur Physik A-Hadrons and Nuclei

IS - 3-4

T2 - 2nd International Conference on Atomic and Nuclear Clusters

Y2 - 28 June 1993 through 2 July 1993

ER -

Alpha-clustering and the stellar nucleosynthesis of carbon

Abstract

Keywords

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