Abstract
using the nuclear equation of states for a large variety of relativistic and non-relativistic force parameters, we calculate the static and rotating masses and radii of neutron stars. From these equation of states, we evaluate the properties of rotating neutron stars, such as rotational frequencies, moment of inertia, quadrupole deformation parameter, rotational ellipticity and gravitational wave strain amplitude. The estimated gravitational wave strain amplitude of the star is found to be~sim 10.
Highlights
Nuclei having very different N/Z ratio compared to stable nuclei with the same A, large radial cut-off, high momentum distribution are generally known as drip-line nuclei
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 neutronrich nuclei, experimental mapping of the nuclear shell structure near and far from stability
Summary
Nuclei having very different N/Z ratio compared to stable nuclei with the same A, large radial cut-off, high momentum distribution are generally known as drip-line nuclei. 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 neutronrich nuclei, experimental mapping of the nuclear shell structure near and far from stability. 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.
Sign-in/Register to view highlights & summary Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callMore From: Journal of Nuclear Physics, Material Sciences, Radiation and Applications
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
