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Constraining Nuclear Symmetry Energy parameters from Neutron skin thickness of Ca
S. K. Tripathy, D. Behera, T. R. Routray +1
In the present work, we use a finite range effective interaction to calculate the neutron skin thickness in Ca and correlate these quantities with the parameters of nuclear…
Constraints from GW170817 on the bulk viscosity of neutron star matter and the r-mode instability
T. R. Routray, S. P. Pattnaik, C. Gonzalez-Boquera +3
We perform a systematic study of the dependence of the r-mode phenomenology in normal fluid pulsar neutron stars on the symmetry energy slope parameter . An essential ingredient…
Nuclear Symmetry Energy and Neutron Skin Thickness of using a finite range effective interaction
D. Behera, S. K. Tripathy, T. R. Routray +1
We use a finite range simple effective interaction to construct nuclear equations of state for the study of the density dependence of the nuclear symmetry energy. The EoSs provide…
Simple effective interaction: Infinite nuclear matter and finite nuclei
B. Behera, X. Vinas, M. Bhuyan +3
The mean field properties and equation of state for asymmetric nuclear matter are studied by using a simple effective interaction which has a single finite range Gaussian term. The…