Energy-dependent electron escape in evolving supernova remnants produces log-parabola distributions whose photon spectra are consistent with observations of RX J1713.7-3946 and SN 1006.
G., Bazer-Bachi, A
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
years
2026 3verdicts
UNVERDICTED 3roles
background 1polarities
background 1representative citing papers
Oblique shocks in massive star clusters accelerate cosmic rays to multi-PeV energies, reproducing the LHAASO-observed knee as a sequence of rigidity-dependent cutoffs from combined supernova and wind shocks.
A scaling law for nonthermal power-law tails in magnetized turbulent plasmas is derived from particle transport principles and confirmed by PIC simulations with escape, with applications to black hole coronae.
citing papers explorer
-
Cosmic Ray Electron Evolution in Supernova Remnants: Log-Parabola Distribution
Energy-dependent electron escape in evolving supernova remnants produces log-parabola distributions whose photon spectra are consistent with observations of RX J1713.7-3946 and SN 1006.
-
Oblique Shocks at Supernova Remnants in Massive Star Clusters: A Model for the Cosmic-Ray Knee Observed by LHAASO
Oblique shocks in massive star clusters accelerate cosmic rays to multi-PeV energies, reproducing the LHAASO-observed knee as a sequence of rigidity-dependent cutoffs from combined supernova and wind shocks.
-
On The Nonthermal Power Laws In Magnetized Turbulent Plasmas
A scaling law for nonthermal power-law tails in magnetized turbulent plasmas is derived from particle transport principles and confirmed by PIC simulations with escape, with applications to black hole coronae.