The cross section for the astrophysically important 13N(p, γ) 14O reaction has been measured directly with an intense (3 × 108 particles/s) and pure (> 99%) 8.2-MeV 13N radioactive ion beam. The average value, for the 5.8-8.2-MeV 13N energy range, is 106(30) μb. The partial γ width of the resonance which occurs in this reaction at a center-of-mass energy of 0.545 MeV has been deduced to be 3.8(1.2) eV. It is compared with theoretical predictions and indirect determinations.SCOPUS: ar.jinfo:eu-repo/semantics/publishe
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
The 13C(7Li, 6He) 14 N0,1 reactions were measured at E (7Li) = 34 MeV with the Q3D magnetic spectrom...
A low voltage accelerator and high current ion source has been used to determine the cross section o...
A feasibility study was undertaken for the measurement of the resonance at Er=545 keV in the N13(p,)...
Intense N13 radioactive ion beams have been produced by the two-accelerator method. They have been u...
The total cross section for the N-13(d, n)O-14g.s. reaction has been measured with N-13 radioactive ...
The results of a complete set of experiments dealing with the 13N(p, γ)14O reaction and using 13N ra...
Intense /sup 13/N radioactive ion beams have been produced by the two-accelerator method. They have ...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
A feasibility study was undertaken for the measurement of the resonance at E(r) = 545 keV in the N-1...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of s...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
The 13C(7Li, 6He) 14 N0,1 reactions were measured at E (7Li) = 34 MeV with the Q3D magnetic spectrom...
A low voltage accelerator and high current ion source has been used to determine the cross section o...
A feasibility study was undertaken for the measurement of the resonance at Er=545 keV in the N13(p,)...
Intense N13 radioactive ion beams have been produced by the two-accelerator method. They have been u...
The total cross section for the N-13(d, n)O-14g.s. reaction has been measured with N-13 radioactive ...
The results of a complete set of experiments dealing with the 13N(p, γ)14O reaction and using 13N ra...
Intense /sup 13/N radioactive ion beams have been produced by the two-accelerator method. They have ...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
A feasibility study was undertaken for the measurement of the resonance at E(r) = 545 keV in the N-1...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of s...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
The 13C(7Li, 6He) 14 N0,1 reactions were measured at E (7Li) = 34 MeV with the Q3D magnetic spectrom...
A low voltage accelerator and high current ion source has been used to determine the cross section o...