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We aim to explore the bubble nature of the exotic nucleus $^{20}$N within themicroscopic antisymmetrized molecular dynamics (AMD) approach. Constraining itsstructural parameters, we analyse its static properties. Subsequently, we usethe AMD infused finite-range distorted-wave Born approximation theory tocalculate the Coulomb breakup of $^{20}$N as an indirect approach to estimatethe $^{19}$N$(n,\gamma)^{20}$N radiative capture rate.

The $^{19}$N($n$,$\gamma)^{20}$N capture rate in light of the probable bubble nature of $^{20}$N