CNO neutrinos and metallicity of stars

Davini, Stefano

Contribution to a conference proceedings/Contribution to a book

PUBDB-2016-05609

CNO neutrinos and metallicity of stars

Davini, S. (Corresponding author)

2016
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-945931-08-0

Davini, Stefano "CNO neutrinos and metallicity of stars" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg
Magellan Workshop, Hamburg, Germany, 17 Mar 2016 - 18 Mar 2016 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 35-40 (2016) [10.3204/DESY-PROC-2016-05/25]

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2016-05/25

Abstract: The detection of neutrinos resulting from the CNO cycle would be the first direct evidence of the nuclear process that is believed to fuel massive stars. A precise measurement of the CNO solar neutrino fluxes would also help resolving the solar metallicity problem, as the predicted fluxes strongly depend on the inputs of the solar modelling. This articles, part of the Magellan 16 proceedings, reviews the connections between CNO neutrinos and solar metallicity, and the experimental attempts to detect them.

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