The12C(14N,α20Ne)2H and12C(14N,p23Na)2H reactions have been measured at a14N beam energy of 30.0 MeV. The experiment aims to explore24Mg excited states that can be populated in the quasi-free reaction off the deuteron in14N. In particular, the24Mg excitation region explored in the measurement plays a key role in stellar carbon burning whose cross section is obtained by extrapolating high-energy fusion data. From preliminary results, α and proton channels are clearly identified. In particular, ground and first excited states of20Ne and23Na play a major role.

C-burning via the Trojan horse method

Cherubini, S.;Guardo, L.;Indelicato, I.;La Cognata, M.;Lamia, L.;Rapisarda, G. G.;Romano, S.;Sergi, M. L.;Spartá, R.
2017-01-01

Abstract

The12C(14N,α20Ne)2H and12C(14N,p23Na)2H reactions have been measured at a14N beam energy of 30.0 MeV. The experiment aims to explore24Mg excited states that can be populated in the quasi-free reaction off the deuteron in14N. In particular, the24Mg excitation region explored in the measurement plays a key role in stellar carbon burning whose cross section is obtained by extrapolating high-energy fusion data. From preliminary results, α and proton channels are clearly identified. In particular, ground and first excited states of20Ne and23Na play a major role.
9780735415263
Physics and Astronomy (all)
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11769/321562
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