The reaction ^(14)C(p, γ)^(15)N has been measured in the proton energy range of E_p = 250–740 keV. Five resonances have been observed and their strengths were determined. Additionally, 5 nonresonant γ-rays were found to the states at E_x = 0.0, 5.27, 5.30, 6.32 and 9.05 MeV. The energy dependence of their cross sections can be described by the direct capture process and the low-energy tails of the broad resonances at E_R= 1319 and 1509 keV
Background: The reaction 17O(p,γ)18F influences hydrogen-burning nucleosynthesis in several stellar ...
Spectroscopic factors and asymptotic normalization coefficients (ANCs) have been determined for boun...
To estimate the production rate of long-lived radio-nuclides during the controlled thermonuclear bur...
The reaction ^(14)C(p, γ)^(15)N has been measured in the proton energy range of E_p = 250–740 keV. F...
The reaction ^(14)C(α, γ)^(18)O has been measured in the alpha energy range of E_α = 1.14−2.33 MeV. ...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
The cross section for the capture of protons by C13 at 129 kilovolts is σ=5±1×10^-33 cm^2. This meas...
The 13C(7Li, 6He) 14 N0,1 reactions were measured at E (7Li) = 34 MeV with the Q3D magnetic spectrom...
The Bethe-Weizsäcker cycle consists of a set of nuclear reactions that convert hydrogen into helium ...
Total cross section measurements have been made for the ^(14)N(α,γ)^(18)F reaction for 0.5 ≦ E_α ≦ 1...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,\u...
The 14N(p, γ)15O reaction regulates the rate of energy production for stars slightly more massive th...
We present the first direct measurement of an astrophysical reaction using a radioactive beam of iso...
A low voltage accelerator and high current ion source has been used to determine the cross section o...
Nucleon resonances beyond the Δ(1232) have been observed in complex nuclei. Measurements of the (e,e...
Background: The reaction 17O(p,γ)18F influences hydrogen-burning nucleosynthesis in several stellar ...
Spectroscopic factors and asymptotic normalization coefficients (ANCs) have been determined for boun...
To estimate the production rate of long-lived radio-nuclides during the controlled thermonuclear bur...
The reaction ^(14)C(p, γ)^(15)N has been measured in the proton energy range of E_p = 250–740 keV. F...
The reaction ^(14)C(α, γ)^(18)O has been measured in the alpha energy range of E_α = 1.14−2.33 MeV. ...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,γ ...
The cross section for the capture of protons by C13 at 129 kilovolts is σ=5±1×10^-33 cm^2. This meas...
The 13C(7Li, 6He) 14 N0,1 reactions were measured at E (7Li) = 34 MeV with the Q3D magnetic spectrom...
The Bethe-Weizsäcker cycle consists of a set of nuclear reactions that convert hydrogen into helium ...
Total cross section measurements have been made for the ^(14)N(α,γ)^(18)F reaction for 0.5 ≦ E_α ≦ 1...
The rate of the carbon-nitrogen-oxygen (CNO) cycle of hydrogen burning is controlled by the 14N(p,\u...
The 14N(p, γ)15O reaction regulates the rate of energy production for stars slightly more massive th...
We present the first direct measurement of an astrophysical reaction using a radioactive beam of iso...
A low voltage accelerator and high current ion source has been used to determine the cross section o...
Nucleon resonances beyond the Δ(1232) have been observed in complex nuclei. Measurements of the (e,e...
Background: The reaction 17O(p,γ)18F influences hydrogen-burning nucleosynthesis in several stellar ...
Spectroscopic factors and asymptotic normalization coefficients (ANCs) have been determined for boun...
To estimate the production rate of long-lived radio-nuclides during the controlled thermonuclear bur...