NACRE, the 'nuclear astrophysics compilation of reaction rates', has been widely utilized in stellar evolution and nucleosynthesis studies. Its update and extension programme started within a Konan-Université Libre de Bruxelles (ULB) collaboration. At the present moment, experimental data in refereed journals have been collected, and their theoretical extrapolations are being performed using the R-matrix or potential models. For the 3H(d,n) 4He and 2H(p,γ)3He reactions, we present preliminary results that could well reproduce the experimental data. © 2006 American Institute of Physics.SCOPUS: cp.pInternational Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology; Tokyo; Japan; 8 Nov...
Although important effort has been devoted in the last decades to measure decay half-lives and react...
The NACRE-II project, which aims at an update and extension of the previous NACRE compilation [1] of...
We present applications of microscopic models to nuclear reactions of astrophysical interest, and we...
NACRE, the 'nuclear astrophysics compilation of reaction rates', has been widely utilized in stellar...
We review different models used in nuclear astrophysics. Definitions of the relevant cross sections ...
A multi-channel R-matrix code has been developed and used to analyse two key reactions in the CNO cy...
We report on the program and results of the NACRE network (Nuclear Astrophysics Compilation of REact...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
We briefly report on the program and present results of the European network for the evaluation and ...
We report on the status of a new evaluation of the rates in astrophysical conditions of 19 capture a...
40 pages, accepted for publication at ADNDT, web site at http://pntpm3.ulb.ac.be/bigbangWe use the R...
The focus of this seminar are exotic nuclei that participate in the nucleosynthesis. Half of the hea...
We use the R-matrix theory to fit S-factor data on nuclear reactions involved in Big Bang nucleosynt...
Background. The R-Matrix formalism is a crucial tool in the study of nuclear astrophysics reactions,...
Although important effort has been devoted in the last decades to measure decay half-lives and react...
The NACRE-II project, which aims at an update and extension of the previous NACRE compilation [1] of...
We present applications of microscopic models to nuclear reactions of astrophysical interest, and we...
NACRE, the 'nuclear astrophysics compilation of reaction rates', has been widely utilized in stellar...
We review different models used in nuclear astrophysics. Definitions of the relevant cross sections ...
A multi-channel R-matrix code has been developed and used to analyse two key reactions in the CNO cy...
We report on the program and results of the NACRE network (Nuclear Astrophysics Compilation of REact...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
An update of a previous description of the BRUSLIB + NACRE package of nuclear data for astrophysics ...
We briefly report on the program and present results of the European network for the evaluation and ...
We report on the status of a new evaluation of the rates in astrophysical conditions of 19 capture a...
40 pages, accepted for publication at ADNDT, web site at http://pntpm3.ulb.ac.be/bigbangWe use the R...
The focus of this seminar are exotic nuclei that participate in the nucleosynthesis. Half of the hea...
We use the R-matrix theory to fit S-factor data on nuclear reactions involved in Big Bang nucleosynt...
Background. The R-Matrix formalism is a crucial tool in the study of nuclear astrophysics reactions,...
Although important effort has been devoted in the last decades to measure decay half-lives and react...
The NACRE-II project, which aims at an update and extension of the previous NACRE compilation [1] of...
We present applications of microscopic models to nuclear reactions of astrophysical interest, and we...