Add to ORKGThe reaction ^(14)C(α, γ)^(18)O has been measured in the alpha energy range of E_α = 1.14−2.33 MeV. The resonance strengths of the 4^+ resonance at E_α = 1.14 MeV and of the 1^− resonance at E_α = 1.79 MeV have been measured relative to the ^(14)C(p, γ)^(15)N resonance at E_p=0.528 MeV. Additionally, two nonresonant γ-transitions to the ground state and to the first excited state of ^(18)O were found. The energy dependence of their cross sections can be described by the direct capture process and its interference with the two 1^− resonances at E_α = 1.79 and 2.33 MeV
The alpha and neutron capture reactions on ^(14)C, important in a nonstandard big bang scenario, hav...
The low energy part of the beta delayed, alpha spectrum of ^(16)N can be used to determine the p-wav...
The 17O(p,α)14N reaction plays a key role in various astrophysical scenarios, from asymptotic giant ...
The reaction ^(14)C(α, γ)^(18)O has been measured in the alpha energy range of E_α = 1.14−2.33 MeV. ...
The reaction ^(14)C(p, γ)^(15)N has been measured in the proton energy range of E_p = 250–740 keV. F...
Total cross section measurements have been made for the ^(14)N(α,γ)^(18)F reaction for 0.5 ≦ E_α ≦ 1...
International audienceThe radiative capture reaction 12 C(α, γ) 16 O plays an important role in heli...
International audienceThe 18O(p,α)15N and 17O(p,α)14N reactions are of primary importance in several...
In this dissertation, proton, two proton, and emission from the 14O + a interactions were studied w...
The 18O(p, α)15N reaction is of primary importance to pin down the uncertainties, due to nuclear phy...
A search was made for a resonant, final-state interaction between carbon ions produced in the reacti...
AbstractThe cross sections of the Er162(α,γ)Yb166 and Er162(α,n)Yb165 reactions have been measured f...
The observation of oxygen isotopes in giant stars sheds light on mixing processes operating in their...
The $^{17}O(p,\alpha)^{14}N$ and $^{17}O(p,\gamma)^{18}F$ reactions are of major importance to hydro...
International audienceThe O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthe...
The alpha and neutron capture reactions on ^(14)C, important in a nonstandard big bang scenario, hav...
The low energy part of the beta delayed, alpha spectrum of ^(16)N can be used to determine the p-wav...
The 17O(p,α)14N reaction plays a key role in various astrophysical scenarios, from asymptotic giant ...
The reaction ^(14)C(α, γ)^(18)O has been measured in the alpha energy range of E_α = 1.14−2.33 MeV. ...
The reaction ^(14)C(p, γ)^(15)N has been measured in the proton energy range of E_p = 250–740 keV. F...
Total cross section measurements have been made for the ^(14)N(α,γ)^(18)F reaction for 0.5 ≦ E_α ≦ 1...
International audienceThe radiative capture reaction 12 C(α, γ) 16 O plays an important role in heli...
International audienceThe 18O(p,α)15N and 17O(p,α)14N reactions are of primary importance in several...
In this dissertation, proton, two proton, and emission from the 14O + a interactions were studied w...
The 18O(p, α)15N reaction is of primary importance to pin down the uncertainties, due to nuclear phy...
A search was made for a resonant, final-state interaction between carbon ions produced in the reacti...
AbstractThe cross sections of the Er162(α,γ)Yb166 and Er162(α,n)Yb165 reactions have been measured f...
The observation of oxygen isotopes in giant stars sheds light on mixing processes operating in their...
The $^{17}O(p,\alpha)^{14}N$ and $^{17}O(p,\gamma)^{18}F$ reactions are of major importance to hydro...
International audienceThe O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthe...
The alpha and neutron capture reactions on ^(14)C, important in a nonstandard big bang scenario, hav...
The low energy part of the beta delayed, alpha spectrum of ^(16)N can be used to determine the p-wav...
The 17O(p,α)14N reaction plays a key role in various astrophysical scenarios, from asymptotic giant ...