Boron abundances in stellar atmospheres , as well as berillium and lithium ones, can give useful hints for nonstandard transport processes discrimination in stars. They can also be relevant for understanding several astrophysical processes (e.g. primordial nucleosynthesis and spallation reactions in ISM). A comprehensive study of Li Be B abundances can therefore confirm or not the presence of non-standard mixing processes in stellar envelopes. For this reason nuclear processes producing or depleting boron isotope abundance need to be studied at astrophysical energies. The ~(10)B(p,α)~7Be reaction has been studied by means of the Trojan Horse Method .The Trojan Horse Method was thus applied to the ~(10)B(d, α 7Be)n reaction, studied at 24 MeV. The obtained results will be discussed.
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