论文标题
超强磁场中的物理
Physics in Ultra-Strong Magnetic Fields
论文作者
论文摘要
中子星的几个种群的表面磁场高于4.4 x 10^{13} g的临界强度，其中电子回旋器能量等于其剩余的质量能。这些包括高场旋转驱动的脉冲星，X射线昏暗的隔离中子星（XDIN）和磁铁。在这样的超强田中，在物理过程中的量子效应以及仅在这些高磁场强度下发生的其他外来量子电动力学过程对发射的辐射有重大影响。尽管非常强的磁场在中子恒星的内部和外部都起着至关重要的作用，但我将审查主要在中子恒星磁层中运行的过程以及它们如何影响观察到的辐射。
Several populations of neutron stars have surface magnetic fields above the critical strength of 4.4 x 10^{13} G where the electron cyclotron energy equals its rest mass energy. These include high-field rotation-powered pulsars, X-ray dim isolated neutron stars (XDIN), and magnetars. In such ultra-strong fields, quantum effects in physical processes as well as additional exotic Quantum Electrodynamic processes only occurring at these high field strengths have a significant influence on the emitted radiation. Although very strong magnetic fields play a critical role both inside and outside of neutron stars, I will review primarily processes that operate in the neutron star magnetospheres and how they influence the observed radiation.
