Simulations demonstrate non-monotonic guide-field regulation of reconnection efficiency via balance between drift-kink suppression and tearing-mode hindrance in 3D relativistic current sheets.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 4roles
background 1polarities
unclear 1representative citing papers
End-to-end CTAO simulations show that 50h observations will detect Geminga and Monogem TeV halos at 13–30σ and constrain injection index to Δγ₁≈0.2, magnetic field to ΔB≈2μG, and SDZ size for Monogem.
Multi-telescope spectral modeling of HESS J1825-137 using Naima and MCMC shows leptonic dominance for existing GeV-TeV data but lepto-hadronic preference when adding simulated CTAO or LHAASO UHE points.
SKAO will enable detection of synchrotron emission from prestellar cores to probe their magnetic field properties in nearby star-forming regions.
citing papers explorer
-
Guide-Field-mediated Multiscale Instabilities in Relativistic Reconnection
Simulations demonstrate non-monotonic guide-field regulation of reconnection efficiency via balance between drift-kink suppression and tearing-mode hindrance in 3D relativistic current sheets.
-
Geminga and Monogem in the CTAO Era: Probing TeV Halos and Cosmic-Ray Transport
End-to-end CTAO simulations show that 50h observations will detect Geminga and Monogem TeV halos at 13–30σ and constrain injection index to Δγ₁≈0.2, magnetic field to ΔB≈2μG, and SDZ size for Monogem.
-
Constraining leptonic and hadronic gamma-ray emission from HESS J1825-137 and its environment
Multi-telescope spectral modeling of HESS J1825-137 using Naima and MCMC shows leptonic dominance for existing GeV-TeV data but lepto-hadronic preference when adding simulated CTAO or LHAASO UHE points.
-
Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds
SKAO will enable detection of synchrotron emission from prestellar cores to probe their magnetic field properties in nearby star-forming regions.