Add to ORKGA direct test of nova explosion models comes from the observation of γ rays created in the decay of radioactive isotopes produced in the nova. One such isotope, 18F, is believed to be the main source of observable γ rays at and below 511 keV. The main destruction mechanism of 18F is thought to be the 18F(p,α)15O reaction, and uncertainties in the reaction rate arise from uncertainties in the energies, spins, and parities of the nuclear levels in 19Ne above the 18F+p threshold. To measure the properties of these levels, the 19F(3He,t)19Ne-(γ) reaction was studied at Argonne National Laboratory and the Nuclear Science Laboratory at the University of Notre Dame
Background: The 17O(p,\u3b3 )18F reaction affects the production of key isotopes (e.g., 18F and 18O)...
Gamma ray astronomy has made big strides in the last decades paving the way to a better understandin...
The 18F(p,α)15O reaction is the predominant destruction mechanism in novae of the radionuclide F18, ...
Detection of nuclear-decay γ rays provides a sensitive thermometer of nova nucleosynthesis. The most...
The detection of γ-rays from explosive astrophysical scenarios such as novae provides an excellent ...
The 15O(α,γ)19Ne reaction is an important trigger reaction leading to the rapid proton (rp) capture ...
Classical novae are the most common astrophysical thermonuclear explosion and are thought to contrib...
A good understanding of the level structure of 19Ne around the proton threshold is critical to estim...
The rate of destruction of 18F via the 18F + p reactions is of importance in both novae and X-ray b...
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
The 18F(p,α)15O reaction plays a crucial role in understanding γ-ray emission from novae. Because of...
The 17F(p, γ)18 reaction is important in stellar explosions, but its rate has been uncertain because...
The $^{18}$F(p, $\alpha$)$^{15}$O reaction is key to determining the $^{18}$F abundance in classical...
The 29P(p,γ)30S reaction plays an important role in understanding the Si isotopic abundances in pres...
The F18(p,α)O15 reaction rate is crucial for constraining model predictions of the γ-ray observable ...
Background: The 17O(p,\u3b3 )18F reaction affects the production of key isotopes (e.g., 18F and 18O)...
Gamma ray astronomy has made big strides in the last decades paving the way to a better understandin...
The 18F(p,α)15O reaction is the predominant destruction mechanism in novae of the radionuclide F18, ...
Detection of nuclear-decay γ rays provides a sensitive thermometer of nova nucleosynthesis. The most...
The detection of γ-rays from explosive astrophysical scenarios such as novae provides an excellent ...
The 15O(α,γ)19Ne reaction is an important trigger reaction leading to the rapid proton (rp) capture ...
Classical novae are the most common astrophysical thermonuclear explosion and are thought to contrib...
A good understanding of the level structure of 19Ne around the proton threshold is critical to estim...
The rate of destruction of 18F via the 18F + p reactions is of importance in both novae and X-ray b...
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
The 18F(p,α)15O reaction plays a crucial role in understanding γ-ray emission from novae. Because of...
The 17F(p, γ)18 reaction is important in stellar explosions, but its rate has been uncertain because...
The $^{18}$F(p, $\alpha$)$^{15}$O reaction is key to determining the $^{18}$F abundance in classical...
The 29P(p,γ)30S reaction plays an important role in understanding the Si isotopic abundances in pres...
The F18(p,α)O15 reaction rate is crucial for constraining model predictions of the γ-ray observable ...
Background: The 17O(p,\u3b3 )18F reaction affects the production of key isotopes (e.g., 18F and 18O)...
Gamma ray astronomy has made big strides in the last decades paving the way to a better understandin...
The 18F(p,α)15O reaction is the predominant destruction mechanism in novae of the radionuclide F18, ...