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.
48 Ring, P., Gambhir, Y
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 2
method 1
citation-polarity summary
verdicts
UNVERDICTED 3representative citing papers
Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.
A review of parity-doublet models in effective field theory that accommodate a chirally invariant mass m0 to describe baryons across vacuum, nuclear, and astrophysical densities.
citing papers explorer
-
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.
-
Dense Matter and Compact Stars in Strong Magnetic Fields
Strong magnetic fields in compact stars induce Landau quantization and magnetic-moment couplings that change the equation of state and allow additional degrees of freedom such as hyperons, Delta resonances, and quark matter.
-
Chiral, parity-doublet, effective-Lagrangian mean-field theories for nuclear and astrophysical phenomenology
A review of parity-doublet models in effective field theory that accommodate a chirally invariant mass m0 to describe baryons across vacuum, nuclear, and astrophysical densities.