A phenomenological nonequilibrium freeze-out model with Lagrange parameters accounts for both the universal heavy r-process abundance pattern in stars and its observed variations.
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Universality and variability of the heavy r-process element abundance pattern from a nonequilibrium approach
A phenomenological nonequilibrium freeze-out model with Lagrange parameters accounts for both the universal heavy r-process abundance pattern in stars and its observed variations.
- Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors