With simple cluster wave functions describing the colliding nuclei, the resonating-group method allows treating collisions realistically with full account of antisymmetrization and of good quantum numbers. The introduction of generator coordinates leads to a striking simplification by allowing the systematic use of Slater determinants. Reactions involving bound and scattering states simultaneously, such as radiative-capture reactions in nuclear astrophysics, are a particularly rich field of applications. In recent years, the microscopic cluster model has evolved to the study of three-body scattering which appears as a final state in a number of processes. The challenge is now to extend microscopic descriptions of collisions to ab initio cal...
Nuclei feature a rich variety of many-body phenomena. Especially the clustering of nucleons, which l...
Clusters are quite important at various situations in heavy-ion collisions. Antisymmetrized molecula...
important role in astrophysical scenarios. Experimental data are usually only available for higher e...
The exact treatment of nuclei starting from the constituent nucleons and the fun...
We propose an extension of the continuum discretized coupled channels (CDCC) method, where the proje...
We present different reaction models commonly used in nuclear astrophysics, in particular for the nu...
Clusters are quite important at various situations in heavy-ion collisions and in excited low-densit...
The aim of nuclear astrophysics is to understand the formation of the elements and the role played b...
Low-energy nuclear reactions play an important role in many astrophysical scenarios. In many cases e...
We review different models used in nuclear astrophysics. Definitions of the relevant cross sections ...
We reduce the many-body problem to a multi-channel few-body problem by the AGS method. The channels ...
Microscopic approaches enable one to study nuclear bound states as well as nuclear collisions in a u...
Clustering plays an important role in the structure of nuclei, especially for light nuclei in the $p...
We present different models used in nuclear astrophysics. In particular the role of microscopic clus...
The elastic phase shifts for the α + α and α + 3He collisions are calculated in a cluster approach b...
Nuclei feature a rich variety of many-body phenomena. Especially the clustering of nucleons, which l...
Clusters are quite important at various situations in heavy-ion collisions. Antisymmetrized molecula...
important role in astrophysical scenarios. Experimental data are usually only available for higher e...
The exact treatment of nuclei starting from the constituent nucleons and the fun...
We propose an extension of the continuum discretized coupled channels (CDCC) method, where the proje...
We present different reaction models commonly used in nuclear astrophysics, in particular for the nu...
Clusters are quite important at various situations in heavy-ion collisions and in excited low-densit...
The aim of nuclear astrophysics is to understand the formation of the elements and the role played b...
Low-energy nuclear reactions play an important role in many astrophysical scenarios. In many cases e...
We review different models used in nuclear astrophysics. Definitions of the relevant cross sections ...
We reduce the many-body problem to a multi-channel few-body problem by the AGS method. The channels ...
Microscopic approaches enable one to study nuclear bound states as well as nuclear collisions in a u...
Clustering plays an important role in the structure of nuclei, especially for light nuclei in the $p...
We present different models used in nuclear astrophysics. In particular the role of microscopic clus...
The elastic phase shifts for the α + α and α + 3He collisions are calculated in a cluster approach b...
Nuclei feature a rich variety of many-body phenomena. Especially the clustering of nucleons, which l...
Clusters are quite important at various situations in heavy-ion collisions. Antisymmetrized molecula...
important role in astrophysical scenarios. Experimental data are usually only available for higher e...