The model predicts a diffuse neutrino flux from AGN coronal current sheets that matches IceCube observations when the proton magnetization is fixed at 10^5.
Comisso,Concurrent Particle Acceleration and Pitch-angle Anisotropy Driven by Magnetic Reconnection: Ion-electron Plasmas, ApJ 972 (2024) 9 [2405.18227]
3 Pith papers cite this work. Polarity classification is still indexing.
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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.
A hadronic model with two free parameters shows proton-photon interactions can supply enough pairs for observed coronal optical depths above a critical Eddington ratio, with neutrino luminosity scaling as L_X^2/L_Edd below and L_X above that threshold.
citing papers explorer
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Diffuse neutrino flux from coronal magnetospheric current sheets of accreting black holes
The model predicts a diffuse neutrino flux from AGN coronal current sheets that matches IceCube observations when the proton magnetization is fixed at 10^5.
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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.
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Neutrino and pair creation in reconnection-powered coronae of accreting black holes
A hadronic model with two free parameters shows proton-photon interactions can supply enough pairs for observed coronal optical depths above a critical Eddington ratio, with neutrino luminosity scaling as L_X^2/L_Edd below and L_X above that threshold.