3D PIC simulations of relativistic turbulence show mirror interactions drive perpendicular momentum gains correlated with local magnetic-field strengthening, yielding anisotropic high-energy particle distributions and enhanced confinement.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
fields
astro-ph.HE 3roles
background 2polarities
background 2representative citing papers
3C403 is identified as a strong neutrino-emitting candidate radio galaxy from ANTARES data, with multiwavelength analysis of its stable jet and absorbed accretion suggesting possible production mechanisms.
citing papers explorer
-
Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence
3D PIC simulations of relativistic turbulence show mirror interactions drive perpendicular momentum gains correlated with local magnetic-field strengthening, yielding anisotropic high-energy particle distributions and enhanced confinement.
-
3C403: a candidate neutrino-emitting radio galaxy
3C403 is identified as a strong neutrino-emitting candidate radio galaxy from ANTARES data, with multiwavelength analysis of its stable jet and absorbed accretion suggesting possible production mechanisms.
- Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes