Research news on R-process

The r-process, or rapid neutron-capture process, as a research area focuses on understanding the nucleosynthesis of roughly half of the elements heavier than iron through environments with extremely high neutron fluxes. It integrates nuclear physics, astrophysics, and computational modeling to study neutron-rich nuclei far from stability, their capture cross-sections, β-decay rates, fission properties, and the hydrodynamic and thermodynamic conditions in candidate astrophysical sites such as neutron star mergers or certain core-collapse supernovae. Research aims to reproduce observed solar and stellar abundance patterns, constrain the nuclear equation of state, and link electromagnetic and gravitational-wave observations to heavy-element production.

NASA finds extreme star collision in unlikely spot

A fleet of NASA missions has likely uncovered a collision between two ultradense stars in a tiny galaxy buried in a huge stream of gas. Astronomers have never seen this type of explosive event in an environment like this ...

Heaviest tin isotopes provide insights into element synthesis

An international team of researchers, led by scientists from GSI/FAIR in Darmstadt, Germany, has studied r-process nucleosynthesis in measurements conducted at the Canadian research center TRIUMF in Vancouver. At the center ...