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Nucleosynthesis in novae: experimental progress in the determination of nuclear reaction rates

A. Coc 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 : The sources of nuclear uncertainties in nova nucleosynthesis have been identified using hydrodynamical nova models. Experimental efforts have followed and significantly reduced those uncertainties. This is important for the evaluation of nova contribution to galactic chemical evolution, gamma-ray astronomy and possibly presolar grain studies. In particular, estimations of expected gamma-ray fluxes are essential for the planning of observations by means of existing or future satellites.
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Contributor : Christine Hadrossek <>
Submitted on : Tuesday, August 27, 2013 - 4:56:13 PM
Last modification on : Wednesday, October 14, 2020 - 3:56:49 AM

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A. Coc. Nucleosynthesis in novae: experimental progress in the determination of nuclear reaction rates. 10th International Symposium on Origin of Matter and Evolution of Galaxies, Dec 2007, Sapporo, Japan. pp.119-126, ⟨10.1063/1.2943561⟩. ⟨in2p3-00854634⟩

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