Nucleosynthesis in the fast ejecta of a neutron star merger
astro-ph.HE
Submitted: 2026-05-15
Updated: 2026-05-15
Sources
- Robustness of Magnetic Field Amplification in Neutron Star Mergers
- Binary neutron star mergers with SPHINCS_BSSN: temperature-dependent equations of state and damping of constraint violations
- Magnetic Field Configurations in Binary Neutron Star Mergers II: Inspiral, Merger and Ejecta
- Complete survey of r-process conditions: the (un-)robustness of the r-process(-es)
- Non-thermal emission from mildly relativistic dynamical ejecta of neutron star mergers: spectrum and sky image
- The r-Process: History, Required Conditions, Astrophysical Sites, and Observations
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