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تسجيل مستخدم جديدEffective relativistic mean field model for finite nuclei and neutron stars
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New Relativistic mean field parameter set IOPB-I has been developed.
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New effective $Lambda N$ interactions are proposed for the density dependent relativistic mean field model. The multidimensionally constrained relativistic mean field model is used to calculate ground state properties of eleven known $Lambda$ hypernu
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A new parameter set is generated for finite and infinite nuclear system within the effective field theory motivated relativistic mean field (ERMF) formalism. The isovector part of the ERMF model employed in the present study includes the coupling of
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