Nuclei Near and Far From β-Stability Line

  • R.L. Nayak Department of physics, VSS University of Technology, Burla, Odisha, India
  • T. Sahoo Department of physics, VSS University of Technology, Burla, Odisha, India
  • A. Acharya Department of physics, VSS University of Technology, Burla, Odisha, India
Keywords: Neutron and proton drip line nuclei, β stability line, n- and p- skin

Abstract

Proton to neutron ratio around β-stability line presents an open challenge to the nuclear physicists. The prominent milestone in this regard is the discovery of the super heavy elements, nuclear halos in the lightest neutron-rich nuclei, experimental mapping of the nuclear shell structure near and far from stability. In this present paper, the behavior of the p- and n- halo nuclei near the β-stability line are discussed considering the variation of radius with respect to the mass number and N~Z for different nuclei. Our aim is to study the nuclear properties through neutron and proton skin. The isospin symmetry breaking is for heavy halo nuclei of strong interest.

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References

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Published
2015-08-03
How to Cite
R.L. Nayak, T. Sahoo, & A. Acharya. (2015). Nuclei Near and Far From β-Stability Line. Journal of Nuclear Physics, Material Sciences, Radiation and Applications, 3(1), 1-4. https://doi.org/10.15415/jnp.2015.31001
Section
Articles