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Neutron spectroscopy of $^{26}$Mg states: constraining the stellar neutron source $^{22}$Ne($\alpha, n$)$^{25}$Mg
This work reports on accurate, high-resolution measurements of the 25 Mg( n,γ ) 26 Mg and 25 Mg( n,tot ) cross sections in the neutron energy range from thermal to about 300 keV, leading to a significantly improved 25 Mg( n,γ ) 26 Mg parametrization. The relevant resonances for n+25 Mg were characte...
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Lenguaje: | eng |
Publicado: |
2017
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2017.02.025 http://cds.cern.ch/record/2253417 |
Sumario: | This work reports on accurate, high-resolution measurements of the 25 Mg( n,γ ) 26 Mg and 25 Mg( n,tot ) cross sections in the neutron energy range from thermal to about 300 keV, leading to a significantly improved 25 Mg( n,γ ) 26 Mg parametrization. The relevant resonances for n+25 Mg were characterized from a combined R-matrix analysis of the experimental data. This resulted in an unambiguous spin/parity assignment of the corresponding excited states in 26 Mg. With this information experimental upper limits of the reaction rates for 22 Ne( α,n ) 25 Mg and 22 Ne( α,γ ) 26 Mg were established, potentially leading to a significantly higher (α,n)/(α,γ) ratio than previously evaluated. The impact of these results has been studied for stellar models in the mass range 2 to 25 M⊙ . |
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