The Bare Astrophysical S(E) Factor of the 7Li(p, α)α Reaction

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© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation M. Lattuada et al 2001 ApJ 562 1076 DOI 10.1086/323868

0004-637X/562/2/1076

Abstract

The astrophysically important 7Li(p, α)α reaction has been studied via the Trojan horse method in the energy range E = 10-400 keV. A new theoretical description, based on the distorted-wave Born approximation approach, allows one to extract information on the bare astrophysical S-factor, Sb(E), with Sb(0) = 55 ± 3 keV barns. The results are compared with direct experimental data leading to a model-independent value of the electron screening potential energy, Ue = 330 ± 40 eV, much higher than the adiabatic limit Uad = 175 eV.

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10.1086/323868