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Measurement of the -3 keV resonance in the 13C(α,n)16O reaction and its influence on the synthesis of A > 90 nuclei
Marco La Cognata  1@  
1 : Istituto Nazionali di Fisica Nucleare - Laboratori Nazionali del Sud  (INFN-LNS)

The 13C(α, n)16O reaction is the neutron source for the main component of the s-process, responsible of the production of most nuclei in the mass range 90 < A < 204. It is active inside the helium-burning shell in asymptotic giant branch stars, at temperatures


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