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Equation of state of strongly magnetized matter with hyperons and $\Delta$-resonances
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abstract
We construct a new equation of state for the baryonic matter under an intense magnetic field within the framework of covariant density functional theory. The composition of matter includes hyperons as well as $ \Delta$-resonances. The extension of the nucleonic functional to the hypernuclear sector is constrained by the experimental data on $\Lambda$ and $\Xi$-hypernuclei. We find that the equation of state stiffens with the inclusion of the magnetic field, which increases the maximum mass of neutron star compared to the non-magnetic case. In addition, the strangeness fraction in the matter is enhanced. Several observables, like the Dirac effective mass, particle abundances, etc show typical oscillatory behavior as a function of the magnetic field and/or density which is traced back to the occupation pattern of Landau levels.
Forward citations
Cited by 1 Pith paper
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Investigating Universal Relations in Compact Stars featuring $\Delta-$Admixed Exotic Dense Matter
Delta-admixed hypernuclear stars follow the I-Love-Q universal relations and a tight f-mode tidal relation, while the p-mode relation is much more composition-sensitive.
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