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- W3100169267 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 $Delta$ 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 $Delta$ isobars. We analyze available empirical information to put constraints on coupling constants of $Delta$s to mesonic mean fields. We show that the resulting equation of state satisfies majority of presently known experimental constraints." @default.
- W3100169267 created "2020-11-23" @default.
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- W3100169267 date "2017-01-01" @default.
- W3100169267 modified "2023-09-24" @default.
- W3100169267 title "The effect of inclusion of Δ resonances in relativistic mean-field model with scaled hadron masses and coupling constants" @default.
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- W3100169267 doi "https://doi.org/10.1088/1742-6596/798/1/012070" @default.
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