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Publications (13)
- CORRIGENDUM: Equation of state of hot neutron star matter using finite range simple effective interaction (2024 J. Phys. G: Nucl. Part. Phys. 51 085203) Save
- Calculation of bulk viscosity in oscillating hot neutron star matter of n+p+e+μ composition using a fully self-consistent evaluation procedure Save
- Equation of state of hot neutron star matter using finite range simple effective interaction Save
- Nuclear Matter Properties and Neutron Star Phenomenology Using the Finite Range Simple Effective Interaction Save
- Nuclear Matter Properties and Neutron Star Phenomenology Using the Finite Range Simple Effective Interaction Save
- Correlations between charge radii differences of mirror nuclei and stellar observables Save
- Finite-range simple effective interaction including tensor terms Save
- Reexamination of the N=50 and Z=28 shell closure Save
- Influence of direct Urca on the r-mode spin down features of newborn neutron star pulsars Save
- Nuclear symmetry energy parameters from neutron skin thickness in 208Pb and electric dipole polarizability in 68Ni , 120Sn and 208Pb Save