2010/11/25 by David A. Burton, D. A. Burton, H. Wen +3
Earth and Planetary Sciences · Mathematics · Physics and Astronomy · #Acceleration #Amplitude #Atomic physics #Born–Infeld model #Classical mechanics #Computational physics #Electron #High-pressure geophysics and materials #Laser-Plasma Interactions and Diagnostics #Magnetic field #Physics #Plasma #Quantum electrodynamics #Quantum mechanics #Solar and Space Plasma Dynamics #Waves in plasmas #math-ph #math.MP #physics.acc-ph #physics.plasm-ph
paper · pdf · doi:10.1063/1.3599131
published in AIP conference proceedings, 87-92 (American Institute of Physics) · 6 pages, 1 figure. Developed from a talk given at the 19th International Fall Workshop on Geometry and Physics, Sep 6-9 2010, Porto, Portugal
arxiv created 2010/11/25 · openalex publication_date 2011/01/01 · arxiv updated 2011/07/28 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Motivated by the suggestion that Born-Infeld plasmas could have significance for electron acceleration in neutron star crusts, we obtain an upper bound on the amplitude of electrostatic waves propagating parallel to a longitudinal magnetic field in a Born-Infeld plasma.