Magnetic rigidity reveals the PeVatron acceleration region in SS433
Jie Liao, Wancheng Xu, Lang Cui, Pak-Hin Thomas Tam, Xi Yan, Linuo Yang, Ruo-yu Liu, Liang Chen, Ning Chang, Yong-Feng Huang, Long Ji, Ashutosh Tripathi, Felix Aharonian
astro-ph.HE
Submitted: 2026-08-16
Updated: 2026-08-18
Comments: 37 pages, 10 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Origin of Galactic Cosmic Rays
- Particle acceleration and multi-messenger radiation from Ultra-Luminous X-ray Sources: A new class of Galactic PeVatrons
- Galactic Super-Accreting X-ray Binaries as Super-PeVatron Accelerators
- A Leptonic Interpretation of the UHE Gamma-ray Emission from V4641 Sgr
- The inner radio jet region and the complex environment of SS433
- Very high energy particle acceleration powered by the jets of the microquasar SS 433
- Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433
- Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems
- Fermi acceleration in astrophysical jets
- The Astrophysics of Ultrahigh Energy Cosmic Rays
- The First Measurement of Jet Collimation Profiles in an X-ray Binary: the Case of SS 433
- Energy spectra of gamma-rays, electrons and neutrinos produced at proton-proton interactions in the very high energy regime
- Parametrization of gamma-ray production cross-sections for pp interactions in a broad proton energy range from the kinematic threshold to PeV energies
- HI4PI: A full-sky HI survey based on EBHIS and GASS
- Revised equipartition & minimum energy formula for magnetic field strength estimates from radio synchrotron observations
- Analytical Solution of Magnetically Dominated Astrophysical Jets and Winds: Jet Launching, Acceleration, and Collimation
- SS433's jet trace from ALMA imaging and Global Jet Watch spectroscopy: evidence for post-launch particle acceleration
- naima: a Python package for inference of relativistic particle energy distributions from observed nonthermal spectra
- Energy estimation of high energy particles associated with the SS433/W50 system through radio observation at 1.4 GHz
- Energy spectra of gamma-rays, electrons and neutrinos produced at interactions of relativistic protons with low energy radiation
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