In order to extend the experimental database relevant for the astrophysical gamma-process towards the unexplored heavier mass region, the cross sections of the Eu-151(alpha, gamma)Tb-155 and Eu-151 (alpha, n)Tb-154 reactions have been measured at low energies between 12 and 17 MeV using the activation technique. The results are compared with the predictions of statistical model calculations and it is found that the calculations overestimate the cross sections by about a factor of 2. A sensitivity analysis shows that this discrepancy is caused by the inadequate description of the alpha+nucleus channel. A factor of 2 reduction of the reaction rate of Eu-151(alpha, gamma)Tb-155 in gamma-process network calculations with respect to theoretical ...
The reaction Pr-141(alpha, n)Pm-144 was investigated between E-alpha = 11 MeV and 15 MeV with the ac...
The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small ...
In this paper we present the ongoing experiments at ATOMKI related to our systematic γ-process studi...
The cross sections of (151)Eu(alpha, gamma)(155)Tb and (151)Eu(alpha,n)(154)Tb reactions have been m...
Background: The. process in core-collapse supernova explosions is thought to explain the origin of p...
The cross sections of the 162Er(α,γ)166Yband 162Er(α,n)165Ybreactions have been measured for the fir...
Background: The reaction rates used in gamma-process nucleosynthesis network calculations are mostly...
The stellar reaction rates of radiative alpha-capture reactions on heavy isotopes are of crucial imp...
Background: Statistical model calculations have to be used for the determination of reaction rates i...
The 106Cd(alpha,gamma)110Sn reaction cross section has been measured in the energy range of the Gamo...
Background: Astrophysical reaction rates,which are mostly derived from theoretical cross sections, a...
Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-S...
The Cd-106(alpha,gamma)Sn-110 reaction cross section has been measured in the energy range of the Ga...
The location of the (gamma,p)/(gamma,n) and (gamma,alpha)/(gamma,n) line at gamma process temperatur...
Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the act...
The reaction Pr-141(alpha, n)Pm-144 was investigated between E-alpha = 11 MeV and 15 MeV with the ac...
The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small ...
In this paper we present the ongoing experiments at ATOMKI related to our systematic γ-process studi...
The cross sections of (151)Eu(alpha, gamma)(155)Tb and (151)Eu(alpha,n)(154)Tb reactions have been m...
Background: The. process in core-collapse supernova explosions is thought to explain the origin of p...
The cross sections of the 162Er(α,γ)166Yband 162Er(α,n)165Ybreactions have been measured for the fir...
Background: The reaction rates used in gamma-process nucleosynthesis network calculations are mostly...
The stellar reaction rates of radiative alpha-capture reactions on heavy isotopes are of crucial imp...
Background: Statistical model calculations have to be used for the determination of reaction rates i...
The 106Cd(alpha,gamma)110Sn reaction cross section has been measured in the energy range of the Gamo...
Background: Astrophysical reaction rates,which are mostly derived from theoretical cross sections, a...
Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-S...
The Cd-106(alpha,gamma)Sn-110 reaction cross section has been measured in the energy range of the Ga...
The location of the (gamma,p)/(gamma,n) and (gamma,alpha)/(gamma,n) line at gamma process temperatur...
Cross sections of the 107Ag(α, γ)111In and 107Ag(α,n)110In reactions have been measured with the act...
The reaction Pr-141(alpha, n)Pm-144 was investigated between E-alpha = 11 MeV and 15 MeV with the ac...
The nucleosynthesis of elements beyond iron is dominated by the s and r processes. However, a small ...
In this paper we present the ongoing experiments at ATOMKI related to our systematic γ-process studi...