Nuclei Near and Far From β-Stability Line

Authors

  • 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

DOI:

https://doi.org/10.15415/jnp.2015.31001

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

Change of shell structure in nuclei towards neutron drip line by Ikuko Hamamoto, Division of mathematical physics, LTH, University of Lund, Sweden.

S.M. Wang, J.C. Pei and F.R. Xu, Phys. Rev. C 87, 014311 (2013). http://dx.doi.org/10.1103/PhysRevC.87.014311

G.R. Jansen, M. Hjorth-Jensen, G. Hagen and T. Papen brock, Phys. Rev. C 83, 054306 (2011). http://dx.doi.org/10.1103/PhysRevC.83.054306

Textbook on nuclear physics by B. L. Cohen.

Textbook on nuclear physics by Bohr and Mottelson.

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Published

2015-08-03

How to Cite

(1)
Nayak, R. L. .; Sahoo, T. .; Acharya, A. . Nuclei Near and Far From β-Stability Line. J. Nucl. Phy. Mat. Sci. Rad. A. 2015, 3, 1-4.

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