Skip Nav Destination
Relativistic Plasma in Supercritical Electromagnetic Fields
For plasmas in which the electromagnetic fields exceed a critical field strength, as defined by an invariant parameter in quantum electrodynamics, prolific production of high energy photons, electrons and positrons can cause complex new plasma interactions to occur. The physics of such plasmas in strong fields is critical to future high-intensity laser driven relativistic plasma physics, relativistic intense beam-beam interactions and is also relevant to early universe conditions, extreme astrophysical objects such as neutron star atmospheres and black hole environments. Papers for this Special Topic should relate to the physics of these environments.
Guest Editors: Alec Thomas and Stepan Bulanov
Plasma-Based Accelerators, Beams, Radiation Generation
Brandon K. Russell; Paul T. Campbell; Qian Qian; Jason A. Cardarelli; Stepan S. Bulanov; Sergei V. Bulanov; Gabriele M. Grittani; Daniel Seipt; Louise Willingale; Alexander G. R. Thomas
10.1063/5.0163392
Numerical Methods, Verification and Validation in Plasma Physics
T. G. Blackburn; B. King; S. Tang
10.1063/5.0159963
Plasma-Based Accelerators, Beams, Radiation Generation
P. Hadjisolomou; T. M. Jeong; D. Kolenaty; A. J. Macleod; V. Olšovcová; R. Versaci; C. P. Ridgers; S. V. Bulanov
10.1063/5.0158264
Plasma-Based Accelerators, Beams, Radiation Generation
Daniel Seipt; Alec G. R. Thomas
10.1063/5.0165836
Basic Plasma Phenomena, Waves, Instabilities
A. Longman; S. Ravichandran; L. Manzo; C. Z. He; R. Lera; N. McLane; M. Huault; G. Tiscareno; D. Hanggi; P. Spingola; N. Czapla; R. L. Daskalova; L. Roso; R. Fedosejevs; W. T. Hill, III
10.1063/5.0160195
Radiation: Emission, Absorption, Transport
Kinematically boosted pairs from the nonlinear Breit–Wheeler process in small-angle laser collisions
Pisin Chen; Lance Labun
10.1063/5.0157495
Plasma-Based Accelerators, Beams, Radiation Generation
Bing-Jun Li; Yan-Fei Li; Yue-Yue Chen; Xiu-Feng Weng; Xin-Jian Tan; Xin-Jie Ma; Liang Sheng; Hua-Si Hu
10.1063/5.0158256