We report on our latest experimental study of the 2H(ρ,γ)3He reaction in the energy range of interest for big-bang nucleosynthesis. The differential cross section at 135° and γ)-ray angular distributions were measured and compared with the results deduced from the latest ab-initio calculation. The astrophysical S-factor for the 2H(ρ,γ)3He reaction was obtained in the center-of-mass energy range E = 97-210 keV, and it is found to be in reasonable agreement with that predicted by the ab-initio calculation
We have calculated the cross sections for the charge symmetric reactions He-3(He-3,2p)He-4 and He-3(...
The reaction cross section and the energy, at which this value is obtained, are extremely important ...
We have measured for the first time the cross section of the 2H(n,γ)3H reaction at an energy relevan...
We report on our latest experimental study of the 2H(ρ,γ)3He reaction in the energy range of interes...
The astrophysical S-factor for the 3He(α,γ)7Be reaction plays an important role in the Solar Standar...
The astrophysical S-factor for the 3He(α,γ)7Be reaction plays an important role in the Solar Standar...
Recent astronomical data have provided the primordial deuterium abundance with percent precision. As...
The cross section and angular distribution of the ^2H(d,γ) ^4He reaction have been measured from E^(...
The cross sections of the 2H(d,p)3H and 2H(d,n)3He reactions have been measured via the Trojan Horse...
The astrophysical S factor for the radiative capture d(p,γ)He3 in the energy range of interest for b...
The process is a key reaction in both Big-Bang nucleosynthesis and p–p chain of Hydrogen Burning in...
For about 20 years now, observations of 6Li in several old metal-poor stars inside the halo of our g...
The cross section of the [Formula Presented] reaction was determined by in-beam measurements at ener...
In order to understand primordial and stellar nucleosynthesis, we have studied H-2(d,p)H-3 reaction ...
The 10B(p,α0)7Be reaction has been studied by applying the Trojan Horse method to the 2H(10B,α0 7Be)...
We have calculated the cross sections for the charge symmetric reactions He-3(He-3,2p)He-4 and He-3(...
The reaction cross section and the energy, at which this value is obtained, are extremely important ...
We have measured for the first time the cross section of the 2H(n,γ)3H reaction at an energy relevan...
We report on our latest experimental study of the 2H(ρ,γ)3He reaction in the energy range of interes...
The astrophysical S-factor for the 3He(α,γ)7Be reaction plays an important role in the Solar Standar...
The astrophysical S-factor for the 3He(α,γ)7Be reaction plays an important role in the Solar Standar...
Recent astronomical data have provided the primordial deuterium abundance with percent precision. As...
The cross section and angular distribution of the ^2H(d,γ) ^4He reaction have been measured from E^(...
The cross sections of the 2H(d,p)3H and 2H(d,n)3He reactions have been measured via the Trojan Horse...
The astrophysical S factor for the radiative capture d(p,γ)He3 in the energy range of interest for b...
The process is a key reaction in both Big-Bang nucleosynthesis and p–p chain of Hydrogen Burning in...
For about 20 years now, observations of 6Li in several old metal-poor stars inside the halo of our g...
The cross section of the [Formula Presented] reaction was determined by in-beam measurements at ener...
In order to understand primordial and stellar nucleosynthesis, we have studied H-2(d,p)H-3 reaction ...
The 10B(p,α0)7Be reaction has been studied by applying the Trojan Horse method to the 2H(10B,α0 7Be)...
We have calculated the cross sections for the charge symmetric reactions He-3(He-3,2p)He-4 and He-3(...
The reaction cross section and the energy, at which this value is obtained, are extremely important ...
We have measured for the first time the cross section of the 2H(n,γ)3H reaction at an energy relevan...