Properties Of Exotic Nuclei Using Effective Interactions Structure And Reaction Perspective

Abstract

There is currently a lot of interest in the characteristics of nuclei outside the valley of newlineand#946;-stability. Beginning with interacting nucleon and meson fields in a relativistic framework, newlinesignificant advancement has been achieved recently in comprehending various nuclear newlinefeatures at the microscopic level. The development of intermediate energy radioactive newlineion beams (RIB) makes it feasible to study the nuclear chart. The drip line of proton-rich newlineside is much better investigated than its neutron counterpart, but most of the area still newlineneeds to be resurveyed. These days, a lot of strange phenomena have been discovered, newlineand the ones around the drip-line particularly intrigue us a lot. Studying the nuclear newlineground-state properties is possible by the solutions of the relativistic mean field (RMF) newlineequations for nucleons and mesons (in the Relativistic Hartree-Fock approximation). This newlinemethod has a very good benefit that it provides an excellent result for binding energies as newlinewell other properties not only for spherical but also for deformed nuclei. For this proper newlinerelativistic kinematics is used and that the mesons and their properties are known or fixed newlineby the properties of a small number of finite nuclei. As a result, relativistic mean field newline(RMF) models can be used to analyse the binding energies and other bulk characteristics newlineof considered nuclei, and it would be intriguing to apply RMF calculations to nuclei that newlineare close to the neutron-drip line. Along with the pertinent structure data on masses, newlineinteraction cross sections, and the unusual halo and skin structures have also been studied. newlineAnother crucial aspect of nuclear structure is the shell structure of nuclei, which appears newlineas magic numbers. One of the key problems with the nuclear structural physics of unusual newlinenuclei, especially the light nuclei, is the disappearance of the conventional magic number(s) newlineand/or the introduction of a new magic number distant from the and#946;-stability line. Despite newlinebeing one of the oldest concepts in nuclear physics, the magic number pl