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NSR database version of April 29, 2024.

Search: Author = I.Baraffe

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2001HE20      Nucl.Phys. A688, 197c (2001)

A.Heger, I.Baraffe, C.L.Fryer, S.E.Woosley

Evolution and Nucleosynthesis of Very Massive Primordial Stars

doi: 10.1016/S0375-9474(01)00697-2
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1990DE21      Nucl.Phys. A514, 66 (1990)

P.Descouvemont, I.Baraffe

Microscopic Cluster Study of the ¹²B and ¹²N Systems and Application to a Hot pp Chain in Zero-Metal Stars

NUCLEAR STRUCTURE ¹²B; calculated levels, μ, quadrupole moments, B(λ), rms radius. ¹²N; calculated levels, B(λ), reduced widths. Microscopic cluster approach.

NUCLEAR REACTIONS ¹¹B(n, n), E ≤ 5 MeV; calculated σ(E). ⁸Li(α, n), E ≤ 2 MeV; ⁸B(α, p), E < 3 MeV; ¹¹C(p, γ), E ≤ 1 MeV; calculated S-factor. Microscopic cluster approach.

doi: 10.1016/0375-9474(90)90332-G
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