Add to ORKGThe cross section for the capture of protons by C13 at 129 kilovolts is σ=5±1×10^-33 cm^2. This measurement was made possible through the use of a scintillation counter that had an over-all detection efficiency of 8.7 percent, and a pulsed ion source that had a peak proton current capability of one milliampere. A rough analysis of the radiation shows that 80 percent is due to the transition to the ground state of N14, while the exact nature of the remaining 20 percent was not determined
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 reaction network in the neutron-deficient part of the nuclear chart around A ≈ 100 contains seve...
The cross section for the capture of protons by C13 at 129 kilovolts is σ=5±1×10^-33 cm^2. This meas...
A low voltage accelerator and high current ion source has been used to determine the cross section o...
The reaction ^(14)C(p, γ)^(15)N has been measured in the proton energy range of E_p = 250–740 keV. F...
A method has been developed for preparing thin films of carbon on tantalum, and the thick and thin ...
Experimental determination of the cross sections of proton capture on radioactive nuclei is extremel...
A feasibility study was undertaken for the measurement of the resonance at Er=545 keV in the N13(p,)...
The cross section for the astrophysically important 13N(p, γ) 14O reaction has been measured directl...
States in N14 in the region of excitation energy between 10.6 and 12.2 Mev have been studied by mean...
The cross sections of proton-capture reactions are extremely important to model explosive nucleosynt...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
Radioactivity induced by a 15-MeV proton beam extracted into air was studied at the beam transport l...
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 reaction network in the neutron-deficient part of the nuclear chart around A ≈ 100 contains seve...
The cross section for the capture of protons by C13 at 129 kilovolts is σ=5±1×10^-33 cm^2. This meas...
A low voltage accelerator and high current ion source has been used to determine the cross section o...
The reaction ^(14)C(p, γ)^(15)N has been measured in the proton energy range of E_p = 250–740 keV. F...
A method has been developed for preparing thin films of carbon on tantalum, and the thick and thin ...
Experimental determination of the cross sections of proton capture on radioactive nuclei is extremel...
A feasibility study was undertaken for the measurement of the resonance at Er=545 keV in the N13(p,)...
The cross section for the astrophysically important 13N(p, γ) 14O reaction has been measured directl...
States in N14 in the region of excitation energy between 10.6 and 12.2 Mev have been studied by mean...
The cross sections of proton-capture reactions are extremely important to model explosive nucleosynt...
Direct measurements of reaction cross-sections at astrophysical energies often require the use of so...
This research was sponsored by the National Science Foundation Grant NSF PHY 87-1440
Radioactivity induced by a 15-MeV proton beam extracted into air was studied at the beam transport l...
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 reaction network in the neutron-deficient part of the nuclear chart around A ≈ 100 contains seve...