Machine Learning beta-decay Half-lives and Their Application to r-Process Observables
astro-ph.HE, nucl-th
Submitted: 2026-09-24
Updated: 2026-09-24
Terminology
Sources
- Adam: A Method for Stochastic Optimization
- r-Process Nucleosynthesis With Ab Initio Nuclear Masses Around The N=82 Shell Closure
- A Unified Approach to Interpreting Model Predictions
- Large-Scale Calculations of $\beta$-Decay Rates and Implications for $r$-Process Nucleosynthesis
- The N=126 Factory: A New Multi-Nucleon Transfer Reaction Facility
Related papers
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
- Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion