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arXiv · 1611.02751

The effect of inclusion of $Δ$ resonances in relativistic mean-field model with scaled hadron masses and coupling constants

K. A. Maslov·E. E. Kolomeitsev·D. N. Voskresensky
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Abstract

Knowledge of the equation of state of the baryon matter plays a decisive role in the description of neutron stars. With an increase of the baryon density the filling of Fermi seas of hyperons and $Δ$ isobars becomes possible. Their inclusion into standard relativistic mean-field models results in a strong softening of the equation of state and a lowering of the maximum neutron star mass below the measured values. We extend a relativistic mean-field model with scaled hadron masses and coupling constants developed in our previous works and take into account now not only hyperons but also the $Δ$ isobars. We analyze available empirical information to put constraints on coupling constants of $Δ$s to mesonic mean fields. We show that the resulting equation of state satisfies majority of presently known experimental constraints.

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K. A. Maslov, E. E. Kolomeitsev, D. N. Voskresensky. 2016-11-08. The effect of inclusion of $Δ$ resonances in relativistic mean-field model with scaled hadron masses and coupling constants. https://doi.org/10.1088/1742-6596%2F798%2F1%2F012070

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