activity
19952024
most citedNuclear weak-interaction processes in stars

547 citations · 2.3k across the 22 of their papers we have counts for

collaborators

22 papers

nucl-ex2024★ 22 cited

High-temperature Tl decay clarifies Pb dating in early Solar System

G. Leckenby, R. S. Sidhu, R. J. Chen +56

Radioactive nuclei with lifetimes on the order of millions of years can reveal the formation history of the Sun and active nucleosynthesis occurring at the time and place of its bi…

astro-ph.SR2024★ 22 cited

Solar fusion III: New data and theory for hydrogen-burning stars

B. Acharya, M. Aliotta, A. B. Balantekin +47

In stars that lie on the main sequence in the Hertzsprung-Russel diagram, like our sun, hydrogen is fused to helium in a number of nuclear reaction chains and series, such as the p…

astro-ph.SR2019★ 60 cited

Discovery of an Exceptionally Strong -Decay Transition of F and Implications for the Fate of Intermediate-Mass Stars

O. S. Kirsebom, S. Jones, D. F. Strömberg +21

A significant fraction of stars between 7-11 solar masses are thought to become supernovae, but the explosion mechanism is unclear. The answer depends critically on the rate of ele…

astro-ph.HE2019★ 41 cited

The -process with fully time-dependent supernova neutrino emission spectra

Andre Sieverding, Gabriel Martínez-Pinedo, Karlheinz Langanke +3

The neutrino process that occurs in the outer stellar shells during a supernova explosion and involves neutrino-nucleus reactions produces a range of rare, stable and radioactive i…

nucl-th2015★ 89 cited

Neutrino-nucleus reactions and their role for supernova dynamics and nucleosynthesis

K. G. Balasi, K. Langanke, G. Martínez-Pinedo

The description of nuclear reactions induced by supernova neutrinos has witnessed significant progress during the recent years. At the energies and momentum transfers relevant for…

nucl-th2011★ 101 cited

Fission properties for r-process nuclei

J. Erler, K. Langanke, H. P. Loens +2

We present a systematics of fission barriers and fission lifetimes for the whole landscape of super-heavy elements (SHE), i.e. nuclei with Z>100. The fission lifetimes are also com…