The 19N(n,γ)20N capture rate in light of the probable bubble nature of 20N

Abstract

We aim to explore the bubble nature of the exotic nucleus 20N within the microscopic antisymmetrized molecular dynamics (AMD) approach. Constraining its structural parameters, we analyse its static properties. Subsequently, we use the AMD infused finite-range distorted-wave Born approximation theory to calculate the Coulomb breakup of 20N as an indirect approach to estimate the 19N(n,γ)20N radiative capture rate.

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