Several cross-section measurements of proton as well as α-particle capture reactions in the Se-Sb region have been carried out at sub-Coulomb energies with the aim to obtain global input parameters for Hauser-Feshbach (HF) calculations. Some of the results are compared with HF calculations using various optical model potentials and nuclear level densities. © 2005 IOP Publishing Ltd.SCOPUS: cp.jinfo:eu-repo/semantics/publishe
The cross sections of the 72Ge( α , γ)76Se and 1°7Ag(ρ, γ)1°8Cd reactions were measured at energies ...
International audienceThe abundance calculations of the p-nuclei produced in explosive stellar sites...
The cross sections for the 0¹⁶ (p,ɤ) F¹⁷ transitions to the ground d-state and to an excited s-state...
As a continuation of a systematic study of reactions relevant to the astrophysical p process, the cr...
Background: The nucleosynthesis of the neutron-deficient p nuclei remains an open question in nuclea...
As a continuation of a systematic study of reactions relevant to the astrophysical [Formula Presente...
As a continuation of a systematic study of reactions relevant to astrophysical p-process, the (p,γ) ...
Measurements have been made of the 96 Zr(p,fl) 97 Nb, 112 Sn(p,fl) 113 Sb, and 119 Sn(p,fl...
For nucleosynthesis networks of isotopes heavier than those in the iron-peak region, reaction rates ...
Background: Astrophysical models studying the origin of the neutron-deficient p nuclides require kno...
As a continuation of a systematic study of reactions relevant to astrophysical p-process, the (p,gam...
bInstitute for Applied Physics, Goethe-University Frankfurt am Main The accuracy of predicted isotop...
The γ process is assumed to play an important role in the nucleosynthesis of the majority of the p n...
Cross sections for the Yb-168(alpha,beta)Hf171- reactions were measured by means of the activation m...
The astrophysical p process unites all processes that have been introduced to explain the abundance ...
The cross sections of the 72Ge( α , γ)76Se and 1°7Ag(ρ, γ)1°8Cd reactions were measured at energies ...
International audienceThe abundance calculations of the p-nuclei produced in explosive stellar sites...
The cross sections for the 0¹⁶ (p,ɤ) F¹⁷ transitions to the ground d-state and to an excited s-state...
As a continuation of a systematic study of reactions relevant to the astrophysical p process, the cr...
Background: The nucleosynthesis of the neutron-deficient p nuclei remains an open question in nuclea...
As a continuation of a systematic study of reactions relevant to the astrophysical [Formula Presente...
As a continuation of a systematic study of reactions relevant to astrophysical p-process, the (p,γ) ...
Measurements have been made of the 96 Zr(p,fl) 97 Nb, 112 Sn(p,fl) 113 Sb, and 119 Sn(p,fl...
For nucleosynthesis networks of isotopes heavier than those in the iron-peak region, reaction rates ...
Background: Astrophysical models studying the origin of the neutron-deficient p nuclides require kno...
As a continuation of a systematic study of reactions relevant to astrophysical p-process, the (p,gam...
bInstitute for Applied Physics, Goethe-University Frankfurt am Main The accuracy of predicted isotop...
The γ process is assumed to play an important role in the nucleosynthesis of the majority of the p n...
Cross sections for the Yb-168(alpha,beta)Hf171- reactions were measured by means of the activation m...
The astrophysical p process unites all processes that have been introduced to explain the abundance ...
The cross sections of the 72Ge( α , γ)76Se and 1°7Ag(ρ, γ)1°8Cd reactions were measured at energies ...
International audienceThe abundance calculations of the p-nuclei produced in explosive stellar sites...
The cross sections for the 0¹⁶ (p,ɤ) F¹⁷ transitions to the ground d-state and to an excited s-state...