References quoted in the XUNDL dataset: 26MG 26MG(POL G,G'):XUNDL-6

3 references found.

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2002KO57

Phys.Rev. C 66, 055805 (2002)

P.E.Koehler

Constraints on the ²²Ne(α, n)²⁵Mg s-process neutron source from analysis of ^natMg+n total and ²⁵Mg(n, γ) cross sections

NUCLEAR REACTIONS Mg(n, X), ²⁵Mg(n, γ), E < 500 MeV; analyzed data; deduced resonance parameters. ²²Ne(α, n), E=low; deduced astrophysical reaction rate uncertainties.

doi: 10.1103/PhysRevC.66.055805

2009LO06

Phys.Rev. C 80, 055803 (2009)

R.Longland, C.Iliadis, G.Rusev, A.P.Tonchev, R.J.de Boer, J.Gorres, M.Wiescher

Photoexcitation of astrophysically important states in ²⁶Mg

NUCLEAR REACTIONS ²⁶Mg(polarized γ, γ'), E=10.8, 11.0, 11.2, 11.4 MeV; measured Eγ, Iγ, and γγ(θ) at TUNL HIγS facility. ²⁶Mg; deduced levels, J, π, and branching ratios. Comparison with Monte Carlo simulations. Implications for the reaction rates for ²²Ne(α, γ)²⁶Mg of astrophysical interest.

doi: 10.1103/PhysRevC.80.055803

2010DE29

Phys.Rev. C 82, 025802 (2010)

R.J.de Boer, M.Wiescher, J.Gorres, R.Longland, C.Iliadis, G.Rusev, A.P.Tonchev

Photoexcitation of astrophysically important states in ²⁶Mg. II. Ground-state-transition partial widths

NUCLEAR REACTIONS ²⁶Mg(γ, γ'), E=10.5-11.7 MeV; measured Eγ, Iγ; deduced levels, J, π, resonances, branching ratios, total widths, partial widths. GEANT4 Monte-Carlo simulation of γ-ray spectra. Relevance to predictions of neutron production for the s-process in nucleosynthesis.

doi: 10.1103/PhysRevC.82.025802