Add to ORKGThe 15O(α,γ)19Ne reaction is an important trigger reaction leading to the rapid proton (rp) capture process in X-ray bursts. The primary uncertainty in determining its astrophysical rate is the uncertain α branching ratios of levels near Ex = 4.1 MeV in 19Ne. These states have been populated in a study of the 20Ne(p, d)19Ne reaction, and α branching ratios are reported in this manuscript
Astrophysical models that address stellar energy generation and nucleosynthesis require a considerab...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...
The 15O(α,γ)19Ne reaction is one of two routes for breakout from the hot CNO cycles into the rp proc...
The branching ratio Γα/Γγ of the 4.033 MeV 3/2+ state in 19Ne plays a crucial role in the breakout f...
The O15(α,γ)Ne19 reaction is responsible for breakout from the hot CNO cycle in type I x-ray bursts....
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
A good understanding of the level structure of 19Ne around the proton threshold is critical to estim...
A direct test of nova explosion models comes from the observation of γ rays created in the decay of ...
Certain astrophysical environments such as thermonuclear outbursts on accreting neutron stars (Type-...
Detection of nuclear-decay γ rays provides a sensitive thermometer of nova nucleosynthesis. The most...
The Ne19(p,γ)Na20 reaction is the second step of a reaction chain which breaks out from the hot CNO ...
The reaction 15 O(alpha; gamma) 19 Ne is one of the potential breakout reactions from the Hot CNO...
Background: Ne19 is an important isotope in nuclear astrophysics due to its role in both the F18(p,α...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...
Astrophysical models that address stellar energy generation and nucleosynthesis require a considerab...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...
The 15O(α,γ)19Ne reaction is one of two routes for breakout from the hot CNO cycles into the rp proc...
The branching ratio Γα/Γγ of the 4.033 MeV 3/2+ state in 19Ne plays a crucial role in the breakout f...
The O15(α,γ)Ne19 reaction is responsible for breakout from the hot CNO cycle in type I x-ray bursts....
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
A good understanding of the level structure of 19Ne around the proton threshold is critical to estim...
A direct test of nova explosion models comes from the observation of γ rays created in the decay of ...
Certain astrophysical environments such as thermonuclear outbursts on accreting neutron stars (Type-...
Detection of nuclear-decay γ rays provides a sensitive thermometer of nova nucleosynthesis. The most...
The Ne19(p,γ)Na20 reaction is the second step of a reaction chain which breaks out from the hot CNO ...
The reaction 15 O(alpha; gamma) 19 Ne is one of the potential breakout reactions from the Hot CNO...
Background: Ne19 is an important isotope in nuclear astrophysics due to its role in both the F18(p,α...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...
Astrophysical models that address stellar energy generation and nucleosynthesis require a considerab...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO ...