The 6Li(p,alpha )3He bare nucleus cross-section at astrophysical energies has been indirectly measured in the framework of the Trojan-Horse Method. This constitutes an important step to address the astrophysical problem of 6Li (and more generally of light elements) surface abundance in stars. The agreement between results from direct and indirect methods is discussed in the context of the surface lithium abundances in stars.

The 6Li(p,alpha )3He bare nucleus astrophysical S(E)-factor and its astrophysical implications

DEGL'INNOCENTI, SCILLA;
2006

Abstract

The 6Li(p,alpha )3He bare nucleus cross-section at astrophysical energies has been indirectly measured in the framework of the Trojan-Horse Method. This constitutes an important step to address the astrophysical problem of 6Li (and more generally of light elements) surface abundance in stars. The agreement between results from direct and indirect methods is discussed in the context of the surface lithium abundances in stars.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11568/107298
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