A new microscopic nucleon-nucleon interaction derived from relativistic mean field theory

Abstract

A new microscopic nucleon-nucleon (NN) interaction has been derived for the first time from the popular relativistic mean field theory (RMFT) Lagrangian. The NN interaction so obtained remarkably relate to the inbuilt fundamental parameters of RMFT. Furthermore, by folding it with the RMFT-densities of cluster and daughter nuclei to obtain the optical potential, it's application is also examined to study the exotic cluster radioactive decays, and results obtained found comparable with the successfully used M3Y phenomenological effective NN interactions. The presently derived NN-interaction can also be used to calculate a number of other nuclear observables.

4 Pages 2 Figures

References in corpus (3)

• Critical view of WKB decay widths
• Versatility of field theory motivated nuclear effective Lagrangian approach
• Folding model analysis of alpha radioactivity

Cited by in corpus (22)

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• The multidimensional model of cluster radioactivity
• Fusion cross section of the superheavy $Z$ = 120 nuclei within the relativistic mean-field formalism
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• Isospin dependent properties of the isotopic chain of Scandium and Titanium nuclei within the relativistic mean-field formalism
• Medium dependent relativistic NN potential: Application to the fusion dynamics
• Examining the stability of thermally fissile Th and U isotopes
• Ternary fission within the temperature dependent relativistic mean field approach
• Preformation Probability and Kinematics of Clusters Emission yielding Pb-daughters
• The effect of self interacting isoscalar-vector meson on finite nuclei and infinite nuclear matter
• Role of nuclear deformation and orientation about symmetry axis of target nucleus on heavy-ion fusion dynamics
• Nuclear incompressibility and its enduring impact on fusion cross-section
• Persistence of the N = 50 shell closure over the isotopic chains of Sc, Ti, V and Cr nuclei using relativistic energy density functional
• Fusion dynamics of ${}^{12}$C+${}^{12}$C reaction: An astrophysical interest within the relativistic mean-field approach
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• Effects of Pycnonuclear Reactions on White Dwarf Stellar Evolution
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• Unearthing radial independence for prediction of alpha-decay half-lives