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Present status and perspectives in nuclear astrophysics studies of the C-12 (alpha, gamma) O-16 reaction

A. Lefebvre-Schuhl 1
1 CSNSM AN
CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse, CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière
Abstract : Present status of the C-12(alpha,gamma)O-16 cross section knowledge at stellar helium-core burning temperature is presented. Its consequences on the reaction rate uncertainties are discussed considering available models to extrapolate experimental results down to stellar helium-core burning temperature. Some experimental perspectives to reach the desired precision at stellar temperatures are described.
Keywords : R-MATRIX ANALYSIS CROSS-SECTION MASSIVE STARS KEY REACTION NUCLEOSYNTHESIS GAMMA)O-16 C-12(ALPHA SCATTERING C-12
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Conference papers
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http://hal.in2p3.fr/in2p3-00854775
Contributor : Christine Hadrossek Connect in order to contact the contributor
Submitted on : Thursday, August 29, 2013 - 11:43:07 AM
Last modification on : Wednesday, September 16, 2020 - 5:42:12 PM

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A. Lefebvre-Schuhl. Present status and perspectives in nuclear astrophysics studies of the C-12 (alpha, gamma) O-16 reaction. Workshop on State of the Art in Nuclear Cluster Physics, May 2008, Strasbourg, France. pp.2171-2175, ⟨10.1142/S021830130801129X⟩. ⟨in2p3-00854775⟩

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