In the mean field approximation of nonlinear relativistic a-ω-p model, we have studied the influence of density-dependent coupling constants between nucleons and mesons on the equation of state (EOS) of infinite sy...In the mean field approximation of nonlinear relativistic a-ω-p model, we have studied the influence of density-dependent coupling constants between nucleons and mesons on the equation of state (EOS) of infinite symmetric nuclear matter in different conditions. We find that the EOS of nuclear matter will become stiffer as e, d in the self- interaction of σ meson increase when the coeffcients except aω in Гω, in which the opposite occurs, are fixed. On the other hand, greater values of aσ, bσ, cσ, aω, dω and smaller values of dσ, bω, cω will lead to stiffer EOS ifc and d are fixed. Besides, greater values of Гω lead to stiffer EOS in high density region for the EOS with same incompressibility coefficient at saturation density.展开更多
为了研究自然杂化轨道计算结果与核自旋偶合常数的相关性 ,本文进行了从头算级别的自然杂化轨道计算。采用STO 3G基组 ,利用Lowdin正交化原子轨道基组下的密度矩阵 ,得到了分子中各原子的杂化轨道、净电荷与13 C H、13 C 13 C键自旋偶...为了研究自然杂化轨道计算结果与核自旋偶合常数的相关性 ,本文进行了从头算级别的自然杂化轨道计算。采用STO 3G基组 ,利用Lowdin正交化原子轨道基组下的密度矩阵 ,得到了分子中各原子的杂化轨道、净电荷与13 C H、13 C 13 C键自旋偶合常数1JCH和1JCC之间关系式。展开更多
基金Supported by the National Natural Science Foundation of China under Grant No.11275073
文摘In the mean field approximation of nonlinear relativistic a-ω-p model, we have studied the influence of density-dependent coupling constants between nucleons and mesons on the equation of state (EOS) of infinite symmetric nuclear matter in different conditions. We find that the EOS of nuclear matter will become stiffer as e, d in the self- interaction of σ meson increase when the coeffcients except aω in Гω, in which the opposite occurs, are fixed. On the other hand, greater values of aσ, bσ, cσ, aω, dω and smaller values of dσ, bω, cω will lead to stiffer EOS ifc and d are fixed. Besides, greater values of Гω lead to stiffer EOS in high density region for the EOS with same incompressibility coefficient at saturation density.