RMF calculations identify a shell/sub-shell closure at N=154 in Es isotopes using the NL-SH parameter set, along with estimates of alpha, beta, and cluster decay half-lives.
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Relativistic mean-field models provide a unified framework for describing bulk nuclear properties and the equation of state of dense neutron-rich matter in neutron stars.
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The Ground State Aspects and the Impact of Shell Structures on the Stability of Es-Isotopes
RMF calculations identify a shell/sub-shell closure at N=154 in Es isotopes using the NL-SH parameter set, along with estimates of alpha, beta, and cluster decay half-lives.
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Relativistic mean-field models of neutron-rich matter
Relativistic mean-field models provide a unified framework for describing bulk nuclear properties and the equation of state of dense neutron-rich matter in neutron stars.