activity
20152026
most citedNeutron Star Mergers and Nucleosynthesis of Heavy Elements

356 citations · 943 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

Early galactic heavy element production - a phenomenological approach

B. Wehmeyer, D. Blaschke, F. K. Röpke +1

The high abundances of heavy elements in early, extremely metal-poor stars is still an unsolved issue in Galactic Chemical Evolution (GCE). Standard approaches, such as mergers of…

astro-ph.GA2023★ 19 cited

Inhomogeneous enrichment of radioactive nuclei in the Galaxy: Deposition of live Mn-53, Fe-60, Hf-182, and Pu-244 into deep-sea archives. Surfing the wave?

Benjamin Wehmeyer, Andrés Yagüe López, Benoit Côté +3

While modelling the galactic chemical evolution (GCE) of stable elements provides insights to the formation history of the Galaxy and the relative contributions of nucleosynthesis…

astro-ph.SR2022★ 4 cited

Origin of Plutonium-244 in the Early Solar System

Maria Lugaro, Andrés Yagüe López, Benjámin Soós +5

We investigate the origin in the early Solar System of the short-lived radionuclide 244Pu (with a half life of 80 Myr) produced by the rapid (r) neutron-capture process. We conside…

nucl-ex2022★ 51 cited

Horizons: Nuclear Astrophysics in the 2020s and Beyond

H. Schatz, A. D. Becerril Reyes, A. Best +162

Nuclear Astrophysics is a field at the intersection of nuclear physics and astrophysics, which seeks to understand the nuclear engines of astronomical objects and the origin of the…

astro-ph.SR2020★ 58 cited

129I and 247Cm in Meteorites Constrain the Last Astrophysical Source of Solar r-process Elements

Benoit Côté, Marius Eichler, Andrés Yagüe +12

The composition of the early Solar System can be inferred from meteorites. Many elements heavier than iron were formed by the rapid neutron-capture process (r process), but the ast…

astro-ph.HE2020★ 69 cited

Core-collapse Supernova Explosions Driven by the Hadron-quark Phase Transition as a Rare -process Site

Tobias Fischer, Meng-Ru Wu, Benjamin Wehmeyer +3

Supernova explosions of massive stars are one of the primary sites for the production of the elements in the universe. Up to now, stars with zero-age main-sequence masses in the ra…