Comprehensive Study of Mass Ejection and Nucleosynthesis in Binary Neutron Star Mergers Leaving Short-lived Massive Neutron Stars
Sho Fujibayashi et al 2023 ApJ 942 39
General relativistic hydrodynamics simulations show that the more asymmetric the merger of two neutron stars, the heavier the r-process elements that are synthesized in the aftermath of the collision.