The relevant astrophysical reaction rates which are derived from the reaction cross sections are necessary input to the reaction network. In this work, we analyse several theoretical models of the nuclear potential which give better prediction of the cross sections for some selected reactions
The primary aim of experimental nuclear astrophysics is to determine the rates of nuclear reactions ...
Astrophysical reaction rates, which are mostly derived from theoretical cross sections, are necessar...
The probability of a nuclear reaction occurrence is defined as cross-section which can be ob- tained...
In a previous publication (ATOMIC DATA AND NUCLEAR DATA TABLES 75, 1 (2000)), we gave seven-paramete...
Although important effort has been devoted in the last decades to measure reaction cross sections, m...
We review different models used for reactions involved in nuclear astrophysics. The reaction rate is...
We review different models used for reactions involved in nuclear astrophysics. The reaction rate is...
The increasing need for cross sections far from the valley of stability poses a challenge for nuclea...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
During the last 10 years, in the general context of nuclear energy applications and future reactors ...
The need for cross sections far from the valley of stability, for applications such as nuclear astro...
The increasing need for cross sections far from the valley of stability, especially for applications...
Nuclear reaction rates for astrophysics applications are traditionally determined on the basis of Ha...
Abstract. Nuclear reaction rates for astrophysics applications are traditionally determined on the b...
Nuclear reaction rates determine the abundances of isotopes in stellar burning pro-cesses. A multitu...
The primary aim of experimental nuclear astrophysics is to determine the rates of nuclear reactions ...
Astrophysical reaction rates, which are mostly derived from theoretical cross sections, are necessar...
The probability of a nuclear reaction occurrence is defined as cross-section which can be ob- tained...
In a previous publication (ATOMIC DATA AND NUCLEAR DATA TABLES 75, 1 (2000)), we gave seven-paramete...
Although important effort has been devoted in the last decades to measure reaction cross sections, m...
We review different models used for reactions involved in nuclear astrophysics. The reaction rate is...
We review different models used for reactions involved in nuclear astrophysics. The reaction rate is...
The increasing need for cross sections far from the valley of stability poses a challenge for nuclea...
The majority of nuclear reactions in astrophysics involve unstable nuclei which are not fully access...
During the last 10 years, in the general context of nuclear energy applications and future reactors ...
The need for cross sections far from the valley of stability, for applications such as nuclear astro...
The increasing need for cross sections far from the valley of stability, especially for applications...
Nuclear reaction rates for astrophysics applications are traditionally determined on the basis of Ha...
Abstract. Nuclear reaction rates for astrophysics applications are traditionally determined on the b...
Nuclear reaction rates determine the abundances of isotopes in stellar burning pro-cesses. A multitu...
The primary aim of experimental nuclear astrophysics is to determine the rates of nuclear reactions ...
Astrophysical reaction rates, which are mostly derived from theoretical cross sections, are necessar...
The probability of a nuclear reaction occurrence is defined as cross-section which can be ob- tained...
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