The r-process involves neutron-rich nuclei far off stability for which no experimental cross sections are known. Therefore, one has to rely on theory which might be prone to considerable uncertainties far off stability. To investigate the impact of such uncertainties, nucleosynthesis in hot bubble models followed completely from high-temperature NSE to low-temperature neutron capture freeze-out were calculated with largely varied rates. Due to the (n,gamma)-(gamma,n) equilibrium established at the onset of the r-process, only late-time neutron captures are important which mainly modify the abundances around the third r-process peak
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
We assess the prospects for attaining steady nuclear-flow equilibrium in expanding r-process environ...
The r-process involves neutron-rich nuclei far off stability for which no experimental cross section...
The r-process involves neutron-rich nuclei far off stability for which no experimental cross section...
Nucleosynthesis of elements beyond the iron peak requires reactions with neutrons due to the high Co...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
About half of the nuclei heavier than iron observed in nature are produced by the socalled rapid neu...
We explore changes in abundance patterns that occur late in the r process. As the neutrons available...
About half of the nuclei heavier than iron observed in nature are produced by the so-called rapid ne...
Recent works show that the r-process can proceed by competition between neutron capture and β-decay ...
also follow the freeze-out of reactions with declining temperatures and densities explicitely. We co...
The r-process is supposed to be a primary process which assembles heavy nuclei from a photo-dissocia...
The rapid neutron capture nucleosynthesis (r-process) is responsible for producing about half of the...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
We assess the prospects for attaining steady nuclear-flow equilibrium in expanding r-process environ...
The r-process involves neutron-rich nuclei far off stability for which no experimental cross section...
The r-process involves neutron-rich nuclei far off stability for which no experimental cross section...
Nucleosynthesis of elements beyond the iron peak requires reactions with neutrons due to the high Co...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
About half of the nuclei heavier than iron observed in nature are produced by the socalled rapid neu...
We explore changes in abundance patterns that occur late in the r process. As the neutrons available...
About half of the nuclei heavier than iron observed in nature are produced by the so-called rapid ne...
Recent works show that the r-process can proceed by competition between neutron capture and β-decay ...
also follow the freeze-out of reactions with declining temperatures and densities explicitely. We co...
The r-process is supposed to be a primary process which assembles heavy nuclei from a photo-dissocia...
The rapid neutron capture nucleosynthesis (r-process) is responsible for producing about half of the...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
We assess the prospects for attaining steady nuclear-flow equilibrium in expanding r-process environ...