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

被引:5
|
作者
Maslov, K. A. [1 ]
Kolomeitsev, E. E. [2 ]
Voskresensky, D. N. [1 ]
机构
[1] Natl Res Nucl Univ MEPhI, Moscow Engn Phys Inst, Kashirskoe Highway 31, Moscow 115409, Russia
[2] Matej Bel Univ, Tajovskeho 40, Banska Bystrica 97401, Slovakia
基金
俄罗斯基础研究基金会;
关键词
EQUATION;
D O I
10.1088/1742-6596/798/1/012070
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
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页数:5
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