Bare-nucleus astrophysical factor of the 3He(d,p)4He reaction via the ``Trojan horse'' method

Details Bare-nucleus astrophysical factor of the 3He(d,p)4He reaction via the ``Trojan horse'' method Bare-nucleus astrophysical factor of the 3He(d,p)4He reaction via the ``Trojan horse'' method

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005phrvc..72f5802l&link_type=abstract

Physical Review C, vol. 72, Issue 6, id. 065802

Astronomy and Astrophysics

Astrophysics

19

Hydrostatic Stellar Nucleosynthesis, Single-Particle Levels And Strength Functions, Direct Reactions, Transfer Reactions

Scientific paper

The 3He(d,p)4He reaction has been studied from Ec.m.=600 keV down to astrophysical energies by means of the “Trojan horse” method using the 6Li(3He,pα)4He three-body reaction at Elab=5 and 6 MeV. Coincidence spectra were measured in kinematic conditions favoring the quasifree 3He+2H process. The bare astrophysical factor Sb(E) for the 3He(d,p)4He reaction was extracted from the three-body cross section in the modified plane-wave Born approximation. Comparison with the Sb extrapolation from the free two-body data is presented. The independent estimate of the screening potential as obtained with the present work seems to confirm the theoretical adiabatic limit.

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