The total cross-section of 12C(α,γ)16O was measured for the first time by a direct and ungated detection of the 16O recoils. This measurement in inverse kinematics using the recoil mass separator ERNA in combination with a windowless He gas target allowed to collect data with high precision in the energy range E = 1.9 to 4.9 MeV. The data represent new information for the determination of the astrophysical S(E) factor.

First direct measurement of the total cross-section of C-12(alpha,gamma)O-16

L. GIALANELLA;A, D'ONOFRIO;LUBRITTO, Carmine;TERRASI, Filippo;
2005

Abstract

The total cross-section of 12C(α,γ)16O was measured for the first time by a direct and ungated detection of the 16O recoils. This measurement in inverse kinematics using the recoil mass separator ERNA in combination with a windowless He gas target allowed to collect data with high precision in the energy range E = 1.9 to 4.9 MeV. The data represent new information for the determination of the astrophysical S(E) factor.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11591/187642
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