Effects of the symmetry energy slope on the axial oscillations of neutron stars

• Published in: Chinese physics B Vol. 22; no. 8; pp. 298 - 301
• Main Author: 文德华 周颖
• Format: Journal Article
• Language: English
• Published: 01.08.2013
• Subjects: Damping; Density; Energy (nuclear); Neutron stars; Oscillations; Saturation; Slopes; Stellar mass; Symmetry; 中子星; 对称核物质; 对称能; 性能; 振荡; 轴向; 阻尼时间; 饱和密度

The impact of symmetry energy slope L on the axial w-mode oscillations is explored, where the range of the con- strained slope L of symmetry energy at saturation density is adopted from 25 MeV to 115 MeV while keeping the equation of state （EOS） of symmetric nuclear matter fixed. Based on the range...