Add to ORKGIntense /sup 13/N radioactive ion beams have been produced by the two-accelerator method. They have been used to investigate the /sup 13/N(/b p/, gamma )/sup 14/O reaction, in particular to measure directly its cross section in the energy region of interest in nuclear astrophysics. The results of a complete set of experiments thereby carried out on this reaction allowed the determining of the stellar conditions under which the cold and hot CNO cycles, for the nuclear `burning' of hydrogen and its transformation into helium, dominate.Anglai
A feasibility study was undertaken for the measurement of the resonance at Er=545 keV in the N13(p,)...
Stellar evolution and nucleosynthesis are interconnected by a wide network of nuclear reactions: the...
Low-energy post-accelerated radioactive ion beams have been used to study nuclear reactions addressi...
Intense N13 radioactive ion beams have been produced by the two-accelerator method. They have been u...
The results of a complete set of experiments dealing with the (N(p, gamma)O)-N-13-O-14 reaction and ...
The results of a complete set of experiments dealing with the 13N(p, γ)14O reaction and using 13N ra...
An intense beam (1.5*10/sup 8/ particles/sec) of radioactive /sup 13/N/sup 1+/ ions (half-life: /b T...
An intense beam (1.5×108 particles/sec) of radioactive N1+13 ions (half-life: T1/2=10 min) has been ...
The cross section for the astrophysically important 13N(p, γ) 14O reaction has been measured directl...
The total cross section for the N-13(d, n)O-14g.s. reaction has been measured with N-13 radioactive ...
The Daresbury Recoil Separator (DRS) and Silicon Detector Array (SIDAR) have been installed at Oak R...
In stars with temperatures above 20*106K, hydrogen burning is dominated by the CNO cycle. Its rate i...
The authors report on first operational results obtained with the two-cyclotron concept for the prod...
In stars with temperatures above 20*10^6 K, hydrogen burning is dominated by the CNO cycle. Its rate...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
A feasibility study was undertaken for the measurement of the resonance at Er=545 keV in the N13(p,)...
Stellar evolution and nucleosynthesis are interconnected by a wide network of nuclear reactions: the...
Low-energy post-accelerated radioactive ion beams have been used to study nuclear reactions addressi...
Intense N13 radioactive ion beams have been produced by the two-accelerator method. They have been u...
The results of a complete set of experiments dealing with the (N(p, gamma)O)-N-13-O-14 reaction and ...
The results of a complete set of experiments dealing with the 13N(p, γ)14O reaction and using 13N ra...
An intense beam (1.5*10/sup 8/ particles/sec) of radioactive /sup 13/N/sup 1+/ ions (half-life: /b T...
An intense beam (1.5×108 particles/sec) of radioactive N1+13 ions (half-life: T1/2=10 min) has been ...
The cross section for the astrophysically important 13N(p, γ) 14O reaction has been measured directl...
The total cross section for the N-13(d, n)O-14g.s. reaction has been measured with N-13 radioactive ...
The Daresbury Recoil Separator (DRS) and Silicon Detector Array (SIDAR) have been installed at Oak R...
In stars with temperatures above 20*106K, hydrogen burning is dominated by the CNO cycle. Its rate i...
The authors report on first operational results obtained with the two-cyclotron concept for the prod...
In stars with temperatures above 20*10^6 K, hydrogen burning is dominated by the CNO cycle. Its rate...
In stars, four hydrogen nuclei are converted into a helium nucleus by two competing nuclear fusion p...
A feasibility study was undertaken for the measurement of the resonance at Er=545 keV in the N13(p,)...
Stellar evolution and nucleosynthesis are interconnected by a wide network of nuclear reactions: the...
Low-energy post-accelerated radioactive ion beams have been used to study nuclear reactions addressi...