AbstractA big part in understanding the nucleosynthesis of heavy nuclei is a proper description of the effective interaction between an α-particle and a target nucleus. Information about the so-called α+nucleus optical-model potential is achieved by precise cross-section measurements at sub-Coulomb energies aiming to constrain the theoretical models for the nuclear physics input-parameters. The cross sections of the 108Cd(α,γ) and 108Cd(α,n) reaction have been measured for the first time close to the astrophysically relevant energy region via the in-beam method at the high-efficiency γ-ray spectrometer HORUS and via the activation technique at the Cologne Clover Counting Setup at the Institute for Nuclear Physics in Cologne, Germany. Compar...
Background: Deviations between experimental data of charged-particle-induced reactions and calculati...
AbstractDifferential and total cross sections for coherent π0-photoproduction from 12C, 40Ca, 93Nb a...
In this paper we present the ongoing experiments at ATOMKI related to our systematic γ-process studi...
AbstractA big part in understanding the nucleosynthesis of heavy nuclei is a proper description of t...
A big part in understanding the nucleosynthesis of heavy nuclei is a proper description of the effec...
In the model calculations of heavy element nucleosynthesis processes the nuclear reaction rates are ...
Background: Astrophysical reaction rates,which are mostly derived from theoretical cross sections, a...
Starting from a recent model of the η′N interaction, we evaluate the η ′-nucleus optical potential, ...
Background: α-nucleus potentials play an essential role for the calculation of α-induced reaction cr...
© 2017 The Authors. Published by Elsevier B. V. This is an Open Access article distributed under the...
© 2017 The Authors. Published by Elsevier B. V. This is an Open Access article distributed under the...
The γ-process in core-collapse and/or type Ia supernova explosions is thought to explain the origin...
This document is the Accepted Manuscript version of the following article: Z. Korkulu, et al, ‘Inves...
Many nuclear astrophysics applications involve radiative α-particle captures, α decays and α-particl...
Background: Deviations between experimental data of charged-particle-induced reactions and calculati...
Background: Deviations between experimental data of charged-particle-induced reactions and calculati...
AbstractDifferential and total cross sections for coherent π0-photoproduction from 12C, 40Ca, 93Nb a...
In this paper we present the ongoing experiments at ATOMKI related to our systematic γ-process studi...
AbstractA big part in understanding the nucleosynthesis of heavy nuclei is a proper description of t...
A big part in understanding the nucleosynthesis of heavy nuclei is a proper description of the effec...
In the model calculations of heavy element nucleosynthesis processes the nuclear reaction rates are ...
Background: Astrophysical reaction rates,which are mostly derived from theoretical cross sections, a...
Starting from a recent model of the η′N interaction, we evaluate the η ′-nucleus optical potential, ...
Background: α-nucleus potentials play an essential role for the calculation of α-induced reaction cr...
© 2017 The Authors. Published by Elsevier B. V. This is an Open Access article distributed under the...
© 2017 The Authors. Published by Elsevier B. V. This is an Open Access article distributed under the...
The γ-process in core-collapse and/or type Ia supernova explosions is thought to explain the origin...
This document is the Accepted Manuscript version of the following article: Z. Korkulu, et al, ‘Inves...
Many nuclear astrophysics applications involve radiative α-particle captures, α decays and α-particl...
Background: Deviations between experimental data of charged-particle-induced reactions and calculati...
Background: Deviations between experimental data of charged-particle-induced reactions and calculati...
AbstractDifferential and total cross sections for coherent π0-photoproduction from 12C, 40Ca, 93Nb a...
In this paper we present the ongoing experiments at ATOMKI related to our systematic γ-process studi...