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- Institute of Physics, BhubaneshwarIN18 papers
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33 papers · 1 filter
Equation of State of Hot Neutron Star Matter using Finite Range Simple Effective Interaction
T. R. Routray, S. Sahoo, X. Viñas +2
The equation of state of hot neutron star matter of n+p+e+ composition in -equilibrium is studied for both neutrino-free isothermal and neutrino-trapped isentropic conditions…
Correlations between charge radii differences of mirror nuclei and stellar observables
P. Bano, S. P. Pattnaik, M. Centelles +2
The correlation between the charge radii differences in mirror nuclei pairs and the neutron skin thickness has been studied with the so-called finite range simple effective interac…
The finite range simple effective interaction including tensor terms
P. Bano, X. Viñas, T. R. Routray +3
The prediction of single particle level crossing phenomenon between and orbitals in - and -isotopic chains by the finite range simple effective intera…
The N=50 and Z=28 shell closure revisited
T. R. Routray, P. Bano, M. Anguiano +3
Recent experiments performed in neutron-rich copper isotopes have revealed a crossing in the nucleus Cu between the and levels, which correspond to the groun…
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…
Study of the core-crust transition in neutron stars with finite-range interactions: the dynamical method
C. Gonzalez-Boquera, M. Centelles, X. Viñas +1
The properties of the core-crust transition in neutron stars are investigated using effective nuclear forces of finite-range. Special attention is paid to the so-called dynamical m…