We present the progress in the measurements of the nuclear reaction rates for 6,7Li,9Be and 10B (p,α) burning channels derived using the Trojan Horse Method (THM). The effects on the predicted stellar surface abundances of such elements in pre-main sequence stars are evaluated using the Pisa up-to-date stellar evolutionary code. The present analysis is restricted to the pre-MS evolution of low-mass stars.

Stellar Surface Abundance of Light Elements and Updated (p,α) Reaction�Rates

Lamia L.;Romano S.;Spitaleri C.;La Cognata M.
2019

Abstract

We present the progress in the measurements of the nuclear reaction rates for 6,7Li,9Be and 10B (p,α) burning channels derived using the Trojan Horse Method (THM). The effects on the predicted stellar surface abundances of such elements in pre-main sequence stars are evaluated using the Pisa up-to-date stellar evolutionary code. The present analysis is restricted to the pre-MS evolution of low-mass stars.
978-3-030-13875-2
978-3-030-13876-9
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/20.500.11769/373023
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