Studies of Compton scattering by relativistic electrons in a strong magnetic field have been restricted to either incident photon angles $θ'$ aligned along the magnetic field $B$ or incident photon energies $ω'$ below the first pair creation threshold $ω'_{PC}$. When these restrictions are relaxed there is a resonance in Compton scattering associated with pair creation (PC), that is analogous to but independent of known resonances associated with gyromagnetic absorption (GA). As with the GA resonances, that may be labeled by the Landau quantum numbers of the relevant states, there is a sequence of PC resonances where the scattering cross section diverges. In this paper, the lowest divergence is studied for incident photon energies satisfying ${ω'}^2\sin^2θ'/(2eB)\ll1$, assuming that the scattering electron is in its ground (Landau) state. This lowest resonance affects only parallel-polarized photons.
Impact of Resonant Compton Scattering on Magnetar X-Ray Polarization with QED Vacuum Resonance
School of Physics and Astronomy, Shanghai Jiao Tong University（上海交通大学物理与天文学院）；Tsung-Dao Lee Institute, Shanghai Jiao Tong University（上海交大李政道研究所）；Center for Astrophysics and Planetary Science, Department of Astronomy, Cornell University（康奈尔大学天文学系天体物理学与行星科学中心）
Department of Physics, McLennan Physical Labs, Toronto, ON M5S 1A7, Canada（多伦多大学物理系）；Canadian Institute for Theoretical Astrophysics, 60 St. George St., Toronto, ON M5S 3H8, Canada（加拿大理论天体物理研究所）
Neutrino and pair creation in reconnection-powered coronae of accreting black holes
National and Kapodistrian University of Athens（雅典国立卡波迪斯特里安大学）；Institute of Accelerating Systems & Applications（加速系统与应用研究所）；Deutsches Elektronen-Synchrotron DESY（德国电子同步加速器中心）；Columbia University（哥伦比亚大学）；Center for Computational Astrophysics, Flatiron Institute（纽约大学柯朗数学科学研究所计算天体物理中心）
Funnel Leakage of the Wien Fireball in the Early Nebula after a Binary Neutron Star Merger
College of Physics Science and Technology, Hebei University（河北大学物理科学与技术学院）；Institute of Astrophysics, Central China Normal University（华中师范大学天体物理研究所）；Institute for Frontier in Astronomy and Astrophysics, Beijing Normal University（北京师范大学天文与天体物理前沿研究院）；Department of Astronomy, Beijing Normal University（北京师范大学天文学系）
