D. N. Binh

First application of the Trojan horse method with a radioactive ion beam: Study of the 18 F(p,α)15 O reaction at astrophysical energies

Measurement of nuclear cross sections at astrophysical energies involving unstable species is one of the most challenging tasks in experimental nuclear physics. The use of indirect methods is often unavoidable in this scenario. In this paper the Trojan Horse Method is applied for the first time to a radioactive ion beam induced reaction studying the

α-Resonance structure in 11C studied via resonant scattering of 7Be+α and with the 7Be(α,p) reaction

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Active target studies of the αp-process at CRIB

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First direct measurement of the C 11 (α,p) N 14 stellar reaction by an extended thick-target method

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Determination of the astrophysical12N(p,γ)13O reaction rate from the2H(12N,13O)nreaction and its astrophysical implications

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Nuclear structure of 30 S and its implications for nucleosynthesis in classical novae

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First measurement of S 30 +α resonant elastic scattering for the S 30 (α,p) reaction rate

O process at low energies relevant to astrophysics via the three body reaction

30S Beam Development and X‐ray Bursts

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Indirect studies on astrophysical reactions at the low-energy RI beam separator CRIB

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First results of Trojan horse method using radioactive ion beams: 18F(p,α) at astrophysical energies

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