标题： 具有 phenomenological three-nucleon force 的中子星计算 显示英文标题

标题： Neutron star calculations with the phenomenological three-nucleon force

摘要： 在这项工作中，我们研究了三体力对中子星结构的影响。在我们的计算中，我们将中子星物质视为β稳定核物质。我们已经将有关TBF效应的结果与两体结果以及其他使用乌尔巴纳v14势和核物质能量抛物线近似来近似不对称核物质问题的三体力计算进行了对比。因此，通过求解托尔曼-奥本海默-沃尔科夫方程，我们估算了中子星的宏观性质，并探讨了当前计算与预期的动力学稳定性条件的一致性。 显示英文摘要

摘要： In this work, we have studied the effect of three-nucleon interaction on the neutron stars structure. In our calculations, we have considered the neutron star matter as a beta-stable nuclear matter. We have put the results concerning the TBF effect in perspective against two-body results and other calculations of three-nucleon interactions, using the Urbana v14 potential and the parabolic approximation of the nuclear-matter energy for approximating the problem of asymmetric nuclear matter. As such, solving the Tolman-Oppenheimer-Volkoff equation, we have estimated bulk properties of neutron stars and investigated how the present calculations would agree with the expected dynamical-stability condition.