Measurement of the 13C(α, n)16O reaction at astrophysical energies using the Trojan Horse Method. Focus on the -3 keV sub-threshold resonance

Measurement of the 13C(α, n)16O reaction at astrophysical energies using the Trojan Horse Method. Focus on the -3 keV sub-threshold resonance

Most of the nuclei in the mass range 90 ≲ A ≲ 208 are produced through the so-called s-process, namely through a series of neutron capture reactions on seed nuclei followed by β-decays. The 13C(α, n)16O reaction is the neutron source for the main component of the s-process. It is active inside the h...

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Bibliographic Details
Main Authors: La Cognata M., Spitaleri C., Trippella O., Kiss G.G., Rogachev G.V., Mukhamedzhanov A.M., Avila M., Guardo G.L., Koshchiy E., Kuchera A., Lamia L., Puglia S.M.R., Romano S., Santiago D., Spartà R.
Format: Article
Language:English
Published: EDP Sciences 2014-03-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20146607010

Internet

http://dx.doi.org/10.1051/epjconf/20146607010

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