English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Asymptotic normalization coefficients (ANCs) are fundamental nuclearconstants playing important role in nuclear reactions, nuclear structure andnuclear astrophysics. In this paper the physical reasons of the Coulombrenormalization of the ANC are addressed. Using Pinkston-Satchler equation theratio for the proton and neutron ANCs of mirror nuclei is obtained in terms ofthe Wronskians from the radial overlap functions and regular solutions of thetwo-body Schr\"odinger equation with the short-range interaction excluded. Thisratio allows one to use microscopic overlap functions for mirror nuclei in theinternal region, where they are the most accurate, to correctly predict theratio of the ANCs for mirror nuclei, which determine the amplitudes of thetails of the overlap functions. Calculations presented for different nucleidemonstrate the Coulomb renormalization effects and independence of the ratioof the nucleon ANCs for mirror nuclei on the channel radius. This ratio isvalid both for bound states and resonances. One of the goals of this paper isto draw attention on the possibility to use the Coulomb renormalized ANCsrather than the standard ones especially when the standard ANCs are too large.

Coulomb renormalization and ratio of proton and neutron asymptotic normalization coefficients for mirror nuclei