Cross sections and reaction rates of (gamma,n) reactions have been measured close above threshold with the photoactivation technique. The experimental data for W-186,Pt-190,Pt-192,Pt-198, Hg-196,Hg-198,Hg-204, Au-197, and Pb-204 show good agreement with theoretical predictions.Peer reviewe
Photon-induced reactions play a key role in the nucleosynthesis of rare neutron-deficient p -nuclei....
The majority of the light elements up to iron (Fe) are formed by successive rounds of ther- monuclea...
The majority of the light elements up to iron (Fe) are formed by successive rounds of ther- monuclea...
The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon bath at the temperatures r...
The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon bath at the temperatures r...
Photon-induced reactions during the astrophysical p- (or gamma-) process occur at typical temperatur...
Total cross section measurements for the Pd-102(p, gamma)Ag-103 and Sn-116(p, gamma)Sb-117 reactions...
The reaction Pr-141(alpha, n)Pm-144 was investigated between E-alpha = 11 MeV and 15 MeV with the ac...
This thesis deals with the systematic study of photoneutron reactions in the astrophysically relevan...
The primary aim of experimental nuclear astrophysics is to determine the rates of nuclear reactions ...
Photodisintegration reaction rates involving charged particles are relevant to the p-process nucleos...
Cross sections for the photon-induced particle-emission reactions (gamma,n), (gamma,p), and (gamma,a...
Abstract. Nuclear reaction rates for astrophysics applications are traditionally determined on the b...
The majority of the light elements up to iron (Fe) are formed by successive rounds of thermonuclear ...
Nuclear reaction rates for astrophysics applications are traditionally determined on the basis of Ha...
Photon-induced reactions play a key role in the nucleosynthesis of rare neutron-deficient p -nuclei....
The majority of the light elements up to iron (Fe) are formed by successive rounds of ther- monuclea...
The majority of the light elements up to iron (Fe) are formed by successive rounds of ther- monuclea...
The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon bath at the temperatures r...
The nucleosynthesis of heavy neutron-deficient nuclei in a stellar photon bath at the temperatures r...
Photon-induced reactions during the astrophysical p- (or gamma-) process occur at typical temperatur...
Total cross section measurements for the Pd-102(p, gamma)Ag-103 and Sn-116(p, gamma)Sb-117 reactions...
The reaction Pr-141(alpha, n)Pm-144 was investigated between E-alpha = 11 MeV and 15 MeV with the ac...
This thesis deals with the systematic study of photoneutron reactions in the astrophysically relevan...
The primary aim of experimental nuclear astrophysics is to determine the rates of nuclear reactions ...
Photodisintegration reaction rates involving charged particles are relevant to the p-process nucleos...
Cross sections for the photon-induced particle-emission reactions (gamma,n), (gamma,p), and (gamma,a...
Abstract. Nuclear reaction rates for astrophysics applications are traditionally determined on the b...
The majority of the light elements up to iron (Fe) are formed by successive rounds of thermonuclear ...
Nuclear reaction rates for astrophysics applications are traditionally determined on the basis of Ha...
Photon-induced reactions play a key role in the nucleosynthesis of rare neutron-deficient p -nuclei....
The majority of the light elements up to iron (Fe) are formed by successive rounds of ther- monuclea...
The majority of the light elements up to iron (Fe) are formed by successive rounds of ther- monuclea...
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