I. 脉冲星(高速旋转的中子星)基本的观测性质 II.有关凝聚态(超流与超导)的物理预备知识 III. 我们的有关研究背景 IV. 磁星超强磁场的物理本质 ─ 各向异性中子超流体3P2中子Cooper对的顺磁磁化现象 V. 强磁场下电子气体的Fermi能同磁场强度的相关性 VI. 磁星的活动性与高X-射线光度 VII. 年轻脉冲星Glitch的物理本质: 3P2 中子超流体 的相震荡模型
1Introduction 2Organization of This Paper 3Introduction to SVD and Waves—Sets of Point Sources and Receivers 4Introductory Example—Three Sources and Three Receivers 5Scalar Wave Examples with Point Sources and Receivers 6Mathematics of Continuous Functions, Operators, and Vector Spaces 7Communications Modes and Common Families of Functions 8Extending to Electromagnetic Waves 9Quantizing the Electromagnetic Field Using the M-Gauge 10Linear Scatterers and Optical Devices 11Mode-Converter Basis Sets as Fundamental Optical Descriptions 12Conclusions