Cluster emission and its impact on the r-process nucleosynthesis

arXiv:2608.24499 · nucl-ex, astro-ph.HE · Submitted 2026-08-25 · Read on arXiv

nucl-ex, astro-ph.HE

Submitted: 2026-08-25

Updated: 2026-08-25

Comments: 21 pages, 5 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Abundance — 14× in this paper · explained in 1 episode
• Adam — 5× in this paper · explained in 2 episodes
• alpha — 4× in this paper · explained in 1 episode
• Calibration — 3× in this paper · explained in 7 episodes
• Core — 2× in this paper · explained in 2 episodes
• Universal Decay Law — 2× in this paper
• Accuracy — 1× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Elias — 1× in this paper · explained in 2 episodes
• Generalized Liquid Drop Model — 1× in this paper

Sources

• The r-process nucleosynthesis: a continued challenge for nuclear physics and astrophysics
• Electron-capture supernovae as the origin of elements beyond iron
• Mass ejection in neutron star mergers
• Multi-messenger Observations of a Binary Neutron Star Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
• Identification of strontium in the merger of two neutron stars
• Modelling the spectra of the kilonova AT2017gfo -- I: The photospheric epochs

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