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

G. Singh; M. Dan; M. Kimura; R. Chatterjee; Shubhchintak; V. Choudhary; W. Horiuchi

REVIEW

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

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2302.06986 v1 pith:DJVF33XN submitted 2023-02-14 nucl-th

V. Choudhary , M. Dan , R. Chatterjee , M. Kimura , W. Horiuchi , Shubhchintak , G. Singh This is my paper · ORCID

classification nucl-th

keywords approachbubblecapturegammanaturerateanalyseantisymmetrized

verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments

abstract

We aim to explore the bubble nature of the exotic nucleus $^{20}$N 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 $^{20}$N as an indirect approach to estimate the $^{19}$N$(n,\gamma)^{20}$N radiative capture rate.

Discussion (0). Continue with ORCID to comment.

Pith tools